Open Quantum Systems III: Recent Developments (Lecture Notes in Mathematics 1882)

Lecture Notes in Mathematics Editors: J.-M. Morel, Cachan F. Takens, Groningen B. Teissier, Paris 1882 S. Attal · A...

Author: Stéphane Attal | Alain Joye | Claude-Alain Pillet | Editors

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Lecture Notes in Mathematics Editors: J.-M. Morel, Cachan F. Takens, Groningen B. Teissier, Paris

1882

S. Attal · A. Joye · C.-A. Pillet (Eds.)

Open Quantum Systems III Recent Developments

ABC

Editors Stéphane Attal Institut Camille Jordan Universit é Claude Bernard Lyon 1 21 av. Claude Bernard 69622 Villeurbanne Cedex France e-mail: [email protected]

Alain Joye Institut Fourier Universit é de Grenoble 1 BP 74 38402 Saint-Martin d'Hères Cedex France e-mail: [email protected]

Claude-Alain Pillet CPT-CNRS, UMR 6207 Université du Sud Toulon-Var BP 20132 83957 La Garde Cedex France e-mail: [email protected] Library of Congress Control Number: 2006923432 Mathematics Subject Classification (2000): 37A60, 37A30, 47A05, 47D06, 47L30, 47L90, 60H10, 60J25, 81Q10, 81S25, 82C10, 82C70 ISSN print edition: 0075-8434 ISSN electronic edition: 1617-9692 ISBN-10 3-540-30993-4 Springer Berlin Heidelberg New York ISBN-13 978-3-540-30993-2 Springer Berlin Heidelberg New York DOI 10.1007/b128453 This work is subject to copyright. All rights are reserved, whether the whole or part of the material is concerned, specifically the rights of translation, reprinting, reuse of illustrations, recitation, broadcasting, reproduction on microfilm or in any other way, and storage in data banks. Duplication of this publication or parts thereof is permitted only under the provisions of the German Copyright Law of September 9, 1965, in its current version, and permission for use must always be obtained from Springer. Violations are liable for prosecution under the German Copyright Law. Springer is a part of Springer Science+Business Media springer.com c Springer-Verlag Berlin Heidelberg 2006 Printed in The Netherlands The use of general descriptive names, registered names, trademarks, etc. in this publication does not imply, even in the absence of a specific statement, that such names are exempt from the relevant protective laws and regulations and therefore free for general use. A EX package Typesetting: by the authors and SPI Publisher Services using a Springer LT Cover design: design & production GmbH, Heidelberg

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Preface

This volume is the third and last of a series devoted to the lecture notes of the Grenoble Summer School on “Open Quantum Systems” which took place at the Institut Fourier from June 16th to July 4th 2003. The contributions presented in this volume correspond to expanded versions of the lecture notes provided by the authors to the students of the Summer School. The corresponding lectures were scheduled in the last part of the School devoted to recent developments in the study of Open Quantum Systems. Whereas the first two volumes were dedicated to a detailed exposition of the mathematical techniques and physical concepts relevant in the study of Open Systems with no a priori pre-requisites, the contributions presented in this volume request from the reader some familiarity with these aspects. Indeed, the material presented here aims at leading the reader already acquainted with the basics in quantum statistical mechanics, spectral theory of linear operators, C ∗ -dynamical systems, and quantum stochastic differential equations to the front of the current research done on various aspects of Open Quantum Systems. Nevertheless, pedagogical efforts have been made by the various authors of these notes so that this volume should be essentially self-contained for a reader with minimal previous exposure to the themes listed above. In any case, the reader in need of complements can always turn to these first two volumes. The topics covered in these lectures notes start with an introduction to nonequilibrium quantum statistical mechanics. The definitions of the physical concepts as well as the necessary mathematical framework suitable for their description are developed in a general setup. A simple non-trivial physically relevant example of independent electrons in a device connected to several reservoirs is treated in details in the second part of these notes in order to illustrate the notions of non-equilibrium steady states, entropy production and other thermodynamical notions introduced earlier. The next contribution is devoted to the many aspects of the Fermi Golden Rule used within the Hamiltonian approach of Open Quantum Systems in order to derive

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a Markovian approximation of the dynamics. In particular, the weak coupling or van Hove limit in both a time-dependent and stationary setting are discussed in an abstract framework. These results are then applied to the case of small systems interacting with reservoirs, within different algebraic representations of the relevant models. The links between the Fermi Golden Rule and the Detailed Balance Condition as well as explicit formulas are also discussed in different physical situations. The third text of this volume is concerned with the notion of decoherence, relevant, in particular, for a discussion of the measurement theory in Quantum Mechanics. The properties of the large time behavior of the dynamics reduced to a subsystem, which is not Markovian in general, are first reviewed. Then, the so-called isometric-sweeping decomposition of a dynamical semigroup is presented in an general setup and its links with decoherence phenomena are exposed. Applications to physical models such as spin systems or to the unravelling of the classical dynamics in certain regimes are then provided. The properties of dynamical semigroups on CCR algebras are discussed in details in the final section. The following contribution is devoted to a systematic study of the long time behavior of quantum dynamical semigroups, as they arise in Markovian approximations. More precisely, the key notions for applications of stationary states, convergence towards equilibrium as well as transience and recurrence of such quantum Markov semigroups are developed in an abstract framework. In particular, conditions on unbounded operators defined in the sense of forms to generate a bona fide quantum dynamical semigroup are formulated, as well as general criteria insuring the existence of stationary states for a given quantum dynamical semigroup. The relations between return to equilibrium for a quantum dynamical semigroup and the properties of its generator are also discussed. All these concepts are then illustrated by applications to concrete physical models used in quantum optics. The last notes of this volume provide a detailed account of the process of continual measurements in quantum optics, considered as an application of quantum stochastic calculus. The basics of this quantum stochastic calculus and the modelization of system-field interactions constructed on it are first explained. Then, indirect and continual measurement processes and the corresponding master equations are introduced and discussed. Physical interpretations of computations performed within this quantum stochastic modelization framework are spelled out for various specific processes in quantum optics. As revealed by this outline, the treatment of the different physical models proposed in this volume makes use of several tools and approximations discussed from a mathematical point of view, both in the Hamiltonian and Markovian approach. At the same time, the different mathematical topics addressed here are illustrated by physically relevant applications in the theory of Open Quantum Systems. We believe the contact made between the practicians of the Markovian and Hamiltonian during the School itself and within the contributions of these volumes is useful and will prove to be even more fruitful for the future developments of the field.

Preface

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Let us close this introduction by pointing out that some recent results in the theory of Open Quantum Systems are not discussed in these notes. These include notably the descriptions of return to equilibrium by means of renormalization analysis and scattering techniques. These demanding approaches were not addressed in the Grenoble Summer School, because a reasonably complete treatment would simply have required too much time. We hope the reader will benefit from the pedagogical efforts provided by all authors of these notes in order to introduce the concepts and problems, as well as recent developments in the theory of Open Quantum Systems.

Lyon, Grenoble, Toulon, September 2005

Stéphane Attal Alain Joye Claude-Alain Pillet

Contents

Topics in Non-Equilibrium Quantum Statistical Mechanics Walter Aschbacher, Vojkan Jakˇsić, Yan Pautrat, and Claude-Alain Pillet . . . . . 1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 2 Conceptual Framework . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 3 Mathematical Framework . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 3.1 Basic Concepts . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 3.2 Non-Equilibrium Steady States (NESS) and Entropy Production . . . 3.3 Structural Properties . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 3.4 C ∗ -Scattering and NESS . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 4 Open Quantum Systems . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 4.1 Definition . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 4.2 C ∗ -Scattering for Open Quantum Systems . . . . . . . . . . . . . . . . . . . . . . 4.3 The First and Second Law of Thermodynamics . . . . . . . . . . . . . . . . . . 4.4 Linear Response Theory . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 4.5 Fermi Golden Rule (FGR) Thermodynamics . . . . . . . . . . . . . . . . . . . . 5 Free Fermi Gas Reservoir . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 5.1 General Description . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 5.2 Examples . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 6 The Simple Electronic Black-Box (SEBB) Model . . . . . . . . . . . . . . . . . . . . . 6.1 The Model . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 6.2 The Fluxes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 6.3 The Equivalent Free Fermi Gas . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 6.4 Assumptions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 7 Thermodynamics of the SEBB Model . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 7.1 Non-Equilibrium Steady States . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 7.2 The Hilbert-Schmidt Condition . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 7.3 The Heat and Charge Fluxes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 7.4 Entropy Production . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 7.5 Equilibrium Correlation Functions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 7.6 Onsager Relations. Kubo Formulas. . . . . . . . . . . . . . . . . . . . . . . . . . . .

1 2 3 5 5 8 10 11 14 14 15 17 18 22 26 26 30 34 34 36 37 40 43 43 44 45 46 47 49

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FGR Thermodynamics of the SEBB Model . . . . . . . . . . . . . . . . . . . . . . . . . . 8.1 The Weak Coupling Limit . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 8.2 Historical Digression—Einstein’s Derivation of the Planck Law . . . . 8.3 FGR Fluxes, Entropy Production and Kubo Formulas . . . . . . . . . . . . . 8.4 From Microscopic to FGR Thermodynamics . . . . . . . . . . . . . . . . . . . . 9 Appendix . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 9.1 Structural Theorems . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 9.2 The Hilbert-Schmidt Condition . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . Fermi Golden Rule and Open Quantum Systems Jan Dereziński and Rafał Früboes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1.1 Fermi Golden Rule and Level Shift Operator in an Abstract Setting . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1.2 Applications of the Fermi Golden Rule to Open Quantum Systems . 2 Fermi Golden Rule in an Abstract Setting . . . . . . . . . . . . . . . . . . . . . . . . . . . 2.1 Notation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 2.2 Level Shift Operator . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 2.3 LSO for C0∗ -Dynamics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 2.4 LSO for W ∗ -Dynamics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 2.5 LSO in Hilbert Spaces . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 2.6 The Choice of the Projection P . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 2.7 Three Kinds of the Fermi Golden Rule . . . . . . . . . . . . . . . . . . . . . . . . . 3 Weak Coupling Limit . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 3.1 Stationary and Time-Dependent Weak Coupling Limit . . . . . . . . . . . . 3.2 Proof of the Stationary Weak Coupling Limit . . . . . . . . . . . . . . . . . . . . 3.3 Spectral Averaging . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 3.4 Second Order Asymptotics of Evolution with the First Order Term . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 3.5 Proof of Time Dependent Weak Coupling Limit . . . . . . . . . . . . . . . . . 3.6 Proof of the Coincidence of Mst and Mdyn with the LSO . . . . . . . . . 4 Completely Positive Semigroups . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 4.1 Completely Positive Maps . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 4.2 Stinespring Representation of a Completely Positive Map . . . . . . . . . 4.3 Completely Positive Semigroups . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 4.4 Standard Detailed Balance Condition . . . . . . . . . . . . . . . . . . . . . . . . . . 4.5 Detailed Balance Condition in the Sense of Alicki-FrigerioGorini-Kossakowski-Verri . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 5 Small Quantum System Interacting with Reservoir . . . . . . . . . . . . . . . . . . . . 5.1 W ∗ -Algebras . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 5.2 Algebraic Description . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 5.3 Semistandard Representation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 5.4 Standard Representation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .

50 50 53 54 56 58 58 60 63 67 68 68 69 71 71 72 73 74 74 75 75 77 77 80 83 85 87 88 88 89 89 90 91 93 93 94 95 95 96

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Two Applications of the Fermi Golden Rule to Open Quantum Systems . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 97 6.1 LSO for the Reduced Dynamics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 97 6.2 LSO for the Liouvillean . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 99 6.3 Relationship Between the Davies Generator and the LSO for the Liouvillean in Thermal Case. . . . . . . . . . . . . . . . . . . . . . . . . . . . 100 6.4 Explicit Formula for the Davies Generator . . . . . . . . . . . . . . . . . . . . . . 103 6.5 Explicit Formulas for LSO for the Liouvillean . . . . . . . . . . . . . . . . . . . 104 6.6 Identities Using the Fibered Representation . . . . . . . . . . . . . . . . . . . . . 106 7 Fermi Golden Rule for a Composite Reservoir . . . . . . . . . . . . . . . . . . . . . . . 108 7.1 LSO for a Sum of Perturbations . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 108 7.2 Multiple Reservoirs . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 109 7.3 LSO for the Reduced Dynamics in the Case of a Composite Reservoir . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 110 7.4 LSO for the Liovillean in the Case of a Composite Reservoir . . . . . . 111 A Appendix – One-Parameter Semigroups . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 112 References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 115 Decoherence as Irreversible Dynamical Process in Open Quantum Systems Philippe Blanchard, Robert Olkiewicz . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 117 1 Physical and Mathematical Prologue . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 118 1.1 Physical Background . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 118 1.2 Environmental Decoherence . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 119 1.3 Algebraic Framework . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 120 1.4 Quantum Dynamical Semigroups . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 121 1.5 A Model of a Discrete Pointer Basis . . . . . . . . . . . . . . . . . . . . . . . . . . . 123 2 The Asymptotic Decomposition of T . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 126 2.1 Notation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 126 2.2 Dynamics in the Markovian Regime . . . . . . . . . . . . . . . . . . . . . . . . . . . 127 2.3 The Unitary Decomposition of T2 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 130 2.4 The Isometric-Sweeping Decomposition . . . . . . . . . . . . . . . . . . . . . . . 133 2.5 Remarks . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 135 3 Review of Decoherence Effects in Infinite Spin Systems . . . . . . . . . . . . . . . 138 3.1 Infinite Spin Systems . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 138 3.2 Continuous Pointer States [10] . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 139 3.3 Decoherence-Induced Spin Algebra [6] . . . . . . . . . . . . . . . . . . . . . . . . 143 3.4 From Quantum to Classical Dynamical Systems [38] . . . . . . . . . . . . . 146 4 Dynamical Semigroups on CCR Algebras . . . . . . . . . . . . . . . . . . . . . . . . . . . 148 4.1 Algebras of Canonical Commutation Relations (CCR) . . . . . . . . . . . . 148 4.2 Promeasures on Locally Convex Topological Vector Spaces . . . . . . . 149 4.3 Perturbed Convolution Semigroups of Promeasures . . . . . . . . . . . . . . 151 4.4 Quantum Dynamical Semigroups on CCR Algebras . . . . . . . . . . . . . . 153 4.5 Example: Quantum Brownian Motion . . . . . . . . . . . . . . . . . . . . . . . . . . 155 5 Outlook . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 157

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References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 158 Notes on the Qualitative Behaviour of Quantum Markov Semigroups Franco Fagnola and Rolando Rebolledo . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 161 1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 162 1.1 Preliminaries . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 164 2 Ergodic Theorems . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 165 3 The Minimal Quantum Dynamical Semigroup . . . . . . . . . . . . . . . . . . . . . . . . 167 4 The Existence of Stationary States . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 172 4.1 A General Result . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 172 4.2 Conditions on the Generator . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 174 4.3 Examples . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 178 4.4 A Multimode Dicke Laser Model . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 178 4.5 A Quantum Model of Absorption and Stimulated Emission . . . . . . . . 182 4.6 The Jaynes-Cummings Model . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 183 5 Faithful Stationary States and Irreducibility . . . . . . . . . . . . . . . . . . . . . . . . . . 184 5.1 The Support of an Invariant State . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 184 5.2 Subharmonic Projections. The Case M = L(h) . . . . . . . . . . . . . . . . . . 186 5.3 Examples . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 188 6 The Convergence Towards the Equilibrium . . . . . . . . . . . . . . . . . . . . . . . . . . 189 6.1 Main Results . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 190 6.2 Examples . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 192 7 Recurrence and Transience of Quantum Markov Semigroups . . . . . . . . . . . 194 7.1 Potential . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 194 7.2 Defining Recurrence and Transience . . . . . . . . . . . . . . . . . . . . . . . . . . . 198 7.3 The Behavior of a d-Harmonic Oscillator . . . . . . . . . . . . . . . . . . . . . . . 201 References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 203 Continual Measurements in Quantum Mechanics and Quantum Stochastic Calculus Alberto Barchielli . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 207 1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 208 1.1 Three Approaches to Continual Measurements . . . . . . . . . . . . . . . . . . 208 1.2 Quantum Stochastic Calculus and Quantum Optics . . . . . . . . . . . . . . . 208 1.3 Some Notations: Operator Spaces . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 209 2 Unitary Evolution and States . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 210 2.1 Quantum Stochastic Calculus . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 210 2.2 The Unitary System–Field Evolution . . . . . . . . . . . . . . . . . . . . . . . . . . . 217 2.3 The System–Field State . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 223 2.4 The Reduced Dynamics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 225 2.5 Physical Basis of the Use of QSC . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 228 3 Continual Measurements . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 230 3.1 Indirect Measurements on SH . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 230 3.2 Characteristic Functionals . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 233 3.3 The Reduced Description . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 241

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XIII

3.4 Direct Detection . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 247 3.5 Optical Heterodyne Detection . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 252 3.6 Physical Models . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 257 4 A Three–Level Atom and the Shelving Effect . . . . . . . . . . . . . . . . . . . . . . . . 258 4.1 The Atom–Field Dynamics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 259 4.2 The Detection Process . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 262 4.3 Bright and Dark Periods: The V-Configuration . . . . . . . . . . . . . . . . . . 264 4.4 Bright and Dark Periods: The Λ-Configuration . . . . . . . . . . . . . . . . . . 267 5 A Two–Level Atom and the Spectrum of the Fluorescence Light . . . . . . . . 269 5.1 The Dynamical Model . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 270 5.2 The Master Equation and the Equilibrium State . . . . . . . . . . . . . . . . . . 274 5.3 The Detection Scheme . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 277 5.4 The Fluorescence Spectrum . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 282 References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 288 Index of Volume III . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 293 Information about the other two volumes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 297 Contents of Volume I . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 298 Index of Volume I . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 302 Contents of Volume II . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 306 Index of Volume II . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 309

List of Contributors

Walter Aschbacher Zentrum Mathematik M5 Technische Universität München D-85747 Garching, Germany e-mail: [email protected]

Alberto Barchielli Politecnico di Milano Dipartimento di Matematica Piazza Leonardo da Vinci 32 20133 Milano, Italy e-mail: [email protected]

Philippe Blanchard Physics Faculty and BiBoS University of Bielefeld Universitätsstrasse 25 33615 Bielefeld, Germany e-mail: blanchard@ physik.uni-bielefeld.de

´ Jan Derezinski Department of Mathematical Methods in Physics Warsaw University, Ho˙za 74 00-682, Warsaw, Poland e-mail: [email protected]

Franco Fagnola Politecnico di Milano Dipartmento di Matematica “F. Brioschi” Piazza Leonardo da Vinci 32 20133 Milano, Italy e-mail: [email protected] ¨ Rafał Fruboes Department of Mathematical Methods in Physics Warsaw University, Ho˙za 74 00-682, Warsaw, Poland e-mail: [email protected] Vojkan Jakˇsić Department of Mathematics and Statistics McGill University 805 Sherbrooke Street West Montreal, QC, H3A 2K6, Canada e-mail: [email protected] Robert Olkiewicz Institute of Theoretical Physics University of Wrocław pl. M. Borna 9 50-204 Wrocław, Poland e-mail: [email protected]

XVI

List of Contributors

Yan Pautrat Laboratoire de Mathématiques Université Paris-Sud 91405 Orsay cedex, France e-mail: [email protected] Claude-Alain Pillet CPT-CNRS, UMR 6207 Université du Sud Toulon-Var B.P. 20132 83957 La Garde Cedex, France e-mail: [email protected]

Rolando Rebolledo Facultad de Matemáticas Universidad Católica de Chile Casilla 306 Santiago 22, Chile e-mail: [email protected]

Topics in Non-Equilibrium Quantum Statistical Mechanics Walter Aschbacher1 , Vojkan Jakˇsić2 , Yan Pautrat3 , and Claude-Alain Pillet4 1

2

3

4

Zentrum Mathematik M5, Technische Universität München, D-85747 Garching, Germany e-mail: [email protected] Department of Mathematics and Statistics, McGill University, 805 Sherbrooke Street West, Montreal, QC, H3A 2K6, Canada e-mail: [email protected] Laboratoire de Mathématiques, Université Paris-Sud, 91405 Orsay cedex, France e-mail: [email protected] CPT-CNRS, UMR 6207, Université du Sud, Toulon-Var, B.P. 20132, 83957 La Garde Cedex, France e-mail: [email protected]

1

Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .

2

2

Conceptual Framework . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .

3

3

Mathematical Framework . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .

5

3.1 3.2 3.3 3.4 4

Open Quantum Systems . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 14 4.1 4.2 4.3 4.4 4.5

5

Definition . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . C ∗ -Scattering for Open Quantum Systems . . . . . . . . . . . . . . . . . . . . . The First and Second Law of Thermodynamics . . . . . . . . . . . . . . . . . Linear Response Theory . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . Fermi Golden Rule (FGR) Thermodynamics . . . . . . . . . . . . . . . . . . .

14 15 17 18 22

Free Fermi Gas Reservoir . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 26 5.1 5.2

6

Basic Concepts . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 5 Non-Equilibrium Steady States (NESS) and Entropy Production . . 8 Structural Properties . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 10 C ∗ -Scattering and NESS . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 11

General Description . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 26 Examples . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 30

The Simple Electronic Black-Box (SEBB) Model . . . . . . . . . . . . . . . . . . 34 6.1 6.2

The Model . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 34 The Fluxes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 36

2

Walter Aschbacher et al.

6.3 6.4 7

Thermodynamics of the SEBB Model . . . . . . . . . . . . . . . . . . . . . . . . . . . . 43 7.1 7.2 7.3 7.4 7.5 7.6

8

Non-Equilibrium Steady States . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . The Hilbert-Schmidt Condition . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . The Heat and Charge Fluxes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . Entropy Production . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . Equilibrium Correlation Functions . . . . . . . . . . . . . . . . . . . . . . . . . . . Onsager Relations. Kubo Formulas. . . . . . . . . . . . . . . . . . . . . . . . . . .

43 44 45 46 47 49

FGR Thermodynamics of the SEBB Model . . . . . . . . . . . . . . . . . . . . . . . 50 8.1 8.2 8.3 8.4

9

The Equivalent Free Fermi Gas . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 37 Assumptions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 40

The Weak Coupling Limit . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . Historical Digression—Einstein’s Derivation of the Planck Law . . . FGR Fluxes, Entropy Production and Kubo Formulas . . . . . . . . . . . From Microscopic to FGR Thermodynamics . . . . . . . . . . . . . . . . . . .

50 53 54 56

Appendix . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 58 9.1 9.2

Structural Theorems . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 58 The Hilbert-Schmidt Condition . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 60

References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 63

1 Introduction These lecture notes are an expanded version of the lectures given by the second and the fourth author in the summer school ”Open Quantum Systems” held in Grenoble, June 16–July 4, 2003. We are grateful to Stéphane Attal and Alain Joye for their hospitality and invitation to speak. The lecture notes have their root in the recent review article [JP4] and our goal has been to extend and complement certain topics covered in [JP4]. In particular, we will discuss the scattering theory of non-equilibrium steady states (NESS) (this topic has been only quickly reviewed in [JP4]). On the other hand, we will not discuss the spectral theory of NESS which has been covered in detail in [JP4]. Although the lecture notes are self-contained, the reader would benefit from reading them in parallel with [JP4]. Concerning preliminaries, we will assume that the reader is familiar with the material covered in the lecture notes [At, Jo, Pi]. On occasion, we will mention or use some material covered in the lectures [D1, Ja]. As in [JP4], we will work in the mathematical framework of algebraic quantum statistical mechanics. The basic notions of this formalism are reviewed in Section 3. In Section 4 we introduce open quantum systems and describe their basic properties. The linear response theory (this topic has not been discussed in [JP4]) is described

Topics in Non-Equilibrium Quantum Statistical Mechanics

3

in Subsection 4.4. The linear response theory of open quantum systems (Kubo formulas, Onsager relations, Central Limit Theorem) has been studied in the recent papers [FMU, FMSU, AJPP, JPR2]. The second part of the lecture notes (Sections 6–8) is devoted to an example. The model we will discuss is the simplest non-trivial example of the Electronic Black Box Model studied in [AJPP] and we will refer to it as the Simple Electronic Black Box Model (SEBB). The SEBB model is to a large extent exactly solvable— its NESS and entropy production can be exactly computed and Kubo formulas can be verified by an explicit computation. For reasons of space, however, we will not discuss two important topics covered in [AJPP]—the stability theory (which is essentially based on [AM, BM]) and the proof of the Central Limit Theorem. The interested reader may complement Sections 6–8 with the original paper [AJPP] and the recent lecture notes [JKP]. Section 5, in which we discuss statistical mechanics of a free Fermi gas, is the bridge between the two parts of the lecture notes. Acknowledgment. The research of V.J. was partly supported by NSERC. Part of this work was done while Y.P. was a CRM-ISM postdoc at McGill University and Centre de Recherches Mathématiques in Montreal.

2 Conceptual Framework The concept of reference state will play an important role in our discussion of nonequilibrium statistical mechanics. To clarify this notion, let us consider first a classical dynamical system with finitely many degrees of freedom and compact phase space X ⊂ Rn . The normalized Lebesgue measure dx on X provides a physically natural statistics on the phase space in the sense that initial configurations sampled according to it can be considered typical (see [Ru4]). Note that this has nothing to do with the fact that dx is invariant under the flow of the system—any measure of the form ρ(x)dx with a strictly positive density ρ would serve the same purpose. The situation is completely different if the system has infinitely many degrees of freedom. In this case, there is no natural replacement for the Lebesgue dx. In fact, a measure on an infinite-dimensional phase space physically describes a thermodynamic state of the system. Suppose for example that the system is Hamiltonian and is in thermal equilibrium at inverse temperature β and chemical potential µ. The statistics of such a system is described by the Gibbs measure (grand canonical ensemble). Since two Gibbs measures with different values of the intensive thermodynamic parameters β, µ are mutually singular, initial points sampled according to one of them will be atypical relative to the other. In conclusion, if a system has infinitely many degrees of freedom, we need to specify its initial thermodynamic state by choosing an appropriate reference measure. As in the finite-dimensional case, this measure may not be invariant under the flow. It also may not be uniquely determined by the physical situation we wish to describe.

4


The situation in quantum mechanics is very similar. The Schrödinger representation of a system with finitely many degrees of freedom is (essentially) uniquely determined and the natural statistics is provided by any strictly positive density matrix on the Hilbert space of the system. For systems with infinitely many degrees of freedom there is no such natural choice. The consequences of this fact are however more drastic than in the classical case. There is no natural choice of a Hilbert space in which the system can be represented. To induce a representation, we must specify the thermodynamic state of the system by choosing an appropriate reference state. The algebraic formulation of quantum statistical mechanics provides a mathematical framework to study such infinite system in a representation independent way. One may object that no real physical system has an infinite number of degrees of freedom and that, therefore, a unique natural reference state always exists. There are however serious methodological reasons to consider this mathematical idealization. Already in equilibrium statistical mechanics the fundamental phenomena of phase transition can only be characterized in a mathematically precise way within such an idealization: A quantum system with finitely many degrees of freedom has a unique thermal equilibrium state. Out of equilibrium, relaxation towards a stationary state and emergence of steady currents can not be expected from the quasi-periodic time evolution of a finite system. In classical non-equilibrium statistical mechanics there exists an alternative approach to this idealization. A system forced by a non-Hamiltonian or timedependent force can be driven towards a non-equilibrium steady state, provided the energy supplied by the external source is removed by some thermostat. This micro-canonical point of view has a number of advantages over the canonical, infinite system idealization. A dynamical system with a relatively small number of degrees of freedom can easily be explored on a computer (numerical integration, iteration of Poincaré sections, . . . ). A large body of “experimental facts” is currently available from the results of such investigations (see [EM, Do] for an introduction to the techniques and a lucid exposition of the results). From a more theoretical perspective, the full machinery of finite-dimensional dynamical system theory becomes available in the micro-canonical approach. The Chaotic Hypothesis introduced in [CG1, CG2] is an attempt to exploit this fact. It justifies phenomenological thermodynamics (Onsager relations, linear response theory, fluctuation-dissipation formulas,...) and has lead to more unexpected results like the Gallavotti-Cohen Fluctuation Theorem. The major drawback of the micro-canonical point of view is the non-Hamiltonian nature of the dynamics, which makes it inappropriate to quantummechanical treatment. The two approaches described above are not completely unrelated. For example, we shall see that the signature of a non-equilibrium steady state in quantum mechanics is its singularity with respect to the reference state, a fact which is well understood in the classical, micro-canonical approach (see Chapter 10 of [EM]). More speculatively, one can expect a general equivalence principle for dynamical (micro-canonical and canonical) ensembles (see [Ru5]). The results in this direction are quite scarce and much work remains to be done.


5

3 Mathematical Framework In this section we describe the mathematical formalism of algebraic quantum statistical mechanics. Our presentation follows [JP4] and is suited for applications to non-equilibrium statistical mechanics. Most of the material in this section is well known and the proofs can be found, for example, in [BR1, BR2, DJP, Ha, OP, Ta]. The proofs of the results described in Subsection 3.3 are given in Appendix 9.1. 3.1 Basic Concepts The starting point of our discussion is a pair (O, τ ), where O is a C ∗ -algebra with a unit I and τ is a C ∗ -dynamics (a strongly continuous group R t → τ t of ∗-automorphisms of O). The elements of O describe physical observables of the quantum system under consideration and the group τ specifies their time evolution. The pair (O, τ ) is sometimes called a C ∗ -dynamical system. In the sequel, by the strong topology on O we will always mean the usual norm topology of O as Banach space. The C ∗ -algebra of all bounded operators on a Hilbert space H is denoted by B(H). A state ω on the C ∗ -algebra O is a normalized (ω(I) = 1), positive (ω(A∗ A) ≥ 0), linear functional on O. It specifies a possible physical state of the quantum mechanical system. If the system is in the state ω at time zero, the quantum mechanical expectation value of the observable A at time t is given by ω(τ t (A)). Thus, states evolve in the Schrödinger picture according to ωt = ω ◦ τ t . The set E(O) of all states on O is a convex, weak-∗ compact subset of the Banach space dual O∗ of O. A linear functional η ∈ O∗ is called τ -invariant if η ◦ τ t = η for all t. The set of all τ -invariant states is denoted by E(O, τ ). This set is always non-empty. A state ω ∈ E(O, τ ) is called ergodic if 1 lim T →∞ 2T and mixing if

T

ω(B ∗ τ t (A)B) dt = ω(A)ω(B ∗ B),

−T

lim ω(B ∗ τ t (A)B) = ω(A)ω(B ∗ B),

|t|→∞

for all A, B ∈ O. Let (Hη , πη , Ωη ) be the GNS representation associated to a positive linear functional η ∈ O∗ . The enveloping von Neumann algebra of O associated to η is Mη ≡ πη (O) ⊂ B(Hη ). A linear functional µ ∈ O∗ is normal relative to η or η-normal, denoted µ η, if there exists a trace class operator ρµ on Hη such that µ(·) = Tr(ρµ πη (·)). Any η-normal linear functional µ has a unique normal extension to Mη . We denote by Nη the set of all η-normal states. µ η iff Nµ ⊂ Nη . A state ω is ergodic iff, for all µ ∈ Nω and A ∈ O, 1 lim T →∞ 2T

T

µ(τ t (A)) dt = ω(A). −T

6


For this reason ergodicity is sometimes called return to equilibrium in mean; see [Ro1, Ro2]. Similarly, ω is mixing (or returns to equilibrium) iff lim µ(τ t (A)) = ω(A),

|t|→∞

for all µ ∈ Nω and A ∈ O. Let η and µ be two positive linear functionals in O∗ , and suppose that η ≥ φ ≥ 0 for some µ-normal φ implies φ = 0. We then say that η and µ are mutually singular (or orthogonal), and write η ⊥ µ. An equivalent (more symmetric) definition is: η ⊥ µ iff η ≥ φ ≥ 0 and µ ≥ φ ≥ 0 imply φ = 0. Two positive linear functionals η and µ in O∗ are called disjoint if Nη ∩Nµ = ∅. If η and µ are disjoint, then η ⊥ µ. The converse does not hold— it is possible that η and µ are mutually singular but not disjoint. To elucidate further these important notions, we recall the following well-known results; see Lemmas 4.1.19 and 4.2.8 in [BR1]. Proposition 3.1. Let µ1 , µ2 ∈ O∗ be two positive linear functionals and µ = µ1 + µ2 . Then the following statements are equivalent: (i) µ1 ⊥ µ2 . (ii) There exists a projection P in πµ (O) such that µ2 (A) = (I − P )Ωµ , πµ (A)Ωµ . µ1 (A) = P Ωµ , πµ (A)Ωµ , (iii) The GNS representation (Hµ , πµ , Ωµ ) is a direct sum of the two GNS representations (Hµ1 , πµ1 , Ωµ1 ) and (Hµ2 , πµ2 , Ωµ2 ), i.e., Hµ = Hµ1 ⊕ Hµ2 ,

πµ = πµ1 ⊕ πµ2 ,

Ωµ = Ωµ1 ⊕ Ωµ2 .

Proposition 3.2. Let µ1 , µ2 ∈ O∗ be two positive linear functionals and µ = µ1 + µ2 . Then the following statements are equivalent: (i) µ1 and µ2 are disjoint. (ii) There exists a projection P in πµ (O) ∩ πµ (O) such that µ2 (A) = (I − P )Ωµ , πµ (A)Ωµ . µ1 (A) = P Ωµ , πµ (A)Ωµ , Let η, µ ∈ O∗ be two positive linear functionals. The functional η has a unique decomposition η = ηn + ηs , where ηn , ηs are positive, ηn µ, and ηs ⊥ µ. The uniqueness of the decomposition implies that if η is τ -invariant, then so are ηn and ηs . To elucidate the nature of this decomposition we need to recall the notions of the universal representation and the universal enveloping von Neumann algebra of O; see Section III.2 in [Ta] and Section 10.1 in [KR]. Set


Hun ≡

ω∈E(O)

Hω ,

πun ≡

πω ,

7

Mun ≡ πun (O) .

ω∈E(O)

(Hun , πun ) is a faithful representation. It is called the universal representation of O. Mun ⊂ B(Hun ) is its universal enveloping von Neumann algebra. For any ω ∈ E(O) the map πun (O) → πω (O) πun (A) → πω (A), extends to a surjective ∗-morphism π ˜ω : Mun → Mω . It follows that ω uniquely ˜ω (·)Ωω ) on Mun . Moreover, one easily extends to a normal state ω ˜ (·) ≡ (Ωω , π shows that (1) Ker π ˜ω = {A ∈ Mun | ν˜(A) = 0 for any ν ∈ Nω }. Since Ker π ˜ω is a σ-weakly closed two sided ideal in Mun , there exists an orthog˜ω = pω Mun . The orthogonal onal projection pω ∈ Mun ∩ Mun such that Ker π projection zω ≡ I − pω ∈ Mun ∩ Mun is called the support projection of the state ω. The restriction of π ˜ω to zω Mun is an isomorphism between the von Neumann algebras zω Mun and Mω . We shall denote by φω the inverse isomorphism. Let now η, µ ∈ O∗ be two positive linear functionals. By scaling, without loss of generality we may assume that they are states. Since η˜ is a normal state on Mun it follows that η˜ ◦ φµ is a normal state on Mµ and hence that ηn ≡ η˜ ◦ φµ ◦ πµ defines a µ-normal positive linear functional on O. Moreover, from the relation φµ ◦ πµ (A) = zµ πun (A) it follows that ηn (A) = (Ωη , π ˜η (zµ )πη (A)Ωη ). Setting ηs (A) ≡ (Ωη , π ˜η (pµ )πη (A)Ωη ), we obtain a decomposition η = ηn + ηs . To show that ηs ⊥ µ let ω be a µ-normal positive linear functional on O such that ηs ≥ ω. By the unicity of the normal extension η˜s one has η˜s (A) = η˜(pµ A) for A ∈ Mun . Since πun (O) is σ-strongly ˜ ◦πun that η˜(pµ A) ≥ ω ˜ (A) dense in Mun it follows from the inequality η˜s ◦πun ≥ ω for any positive A ∈ Mun . Since ω is µ-normal, it further follows from Equ. (1) ˜ (zµ πun (A)) ≤ η˜(pµ zµ πun (A)) = 0 for any positive that ω(A) = ω ˜ (πun (A)) = ω ˜η (zµ ) ∈ Mη ∩ Mη and, by A ∈ O, i.e., ω = 0. Since π ˜η is surjective, one has π Proposition 3.2, the functionals ηn and ηs are disjoint. Two states ω1 and ω2 are called quasi-equivalent if Nω1 = Nω2 . They are called unitarily equivalent if their GNS representations (Hωj , πωj , Ωωj ) are unitarily equivalent, namely if there is a unitary U : Hω1 → Hω2 such that U Ωω1 = Ωω2 and U πω1 (·) = πω2 (·)U . Clearly, unitarily equivalent states are quasi-equivalent. If ω is τ -invariant, then there exists a unique self-adjoint operator L on Hω such that πω (τ t (A)) = eitL πω (A)e−itL . LΩω = 0,

8


We will call L the ω-Liouvillean of τ . The state ω is called factor state (or primary state) if its enveloping von Neumann algebra Mω is a factor, namely if Mω ∩ Mω = CI. By Proposition 3.2 ω is a factor state iff it cannot be written as a nontrivial convex combination of disjoint states. This implies that if ω is a factor state and µ is a positive linear functional in O∗ , then either ω µ or ω ⊥ µ. Two factor states ω1 and ω2 are either quasi-equivalent or disjoint. They are quasi-equivalent iff (ω1 + ω2 )/2 is also a factor state (this follows from Theorem 4.3.19 in [BR1]). The state ω is called modular if there exists a C ∗ -dynamics σω on O such that ω is a (σω , −1)-KMS state. If ω is modular, then Ωω is a separating vector for Mω , and we denote by ∆ω , J and P the modular operator, the modular conjugation and the natural cone associated to Ωω . To any C ∗ -dynamics τ on O one can associate a unique self-adjoint operator L on Hω such that for all t πω (τ t (A)) = eitL πω (A)e−itL ,

e−itL P = P.

The operator L is called standard Liouvillean of τ associated to ω. If ω is τ -invariant, then LΩω = 0, and the standard Liouvillean is equal to the ω-Liouvillean of τ . The importance of the standard Liouvillean L stems from the fact that if a state η is ω-normal and τ -invariant, then there exists a unique vector Ωη ∈ Ker L ∩ P such that η(·) = (Ωη , πω (·)Ωη ). This fact has two important consequences. On one hand, if η is ω-normal and τ -invariant, then some ergodic properties of the quantum dynamical system (O, τ, η) can be described in terms of the spectral properties of L; see [JP2, Pi]. On the other hand, if Ker L = {0}, then the C ∗ -dynamics τ has no ω-normal invariant states. The papers [BFS, DJ2, FM1, FM2, FMS, JP1, JP2, JP3, Me1, Me2, Og] are centered around this set of ideas. In quantum statistical mechanics one also encounters Lp -Liouvilleans, for p ∈ [1, ∞] (the standard Liouvillean is equal to the L2 -Liouvillean). The Lp -Liouvilleans are closely related to the Araki-Masuda Lp -spaces [ArM]. L1 and L∞ -Liouvilleans have played a central role in the spectral theory of NESS developed in [JP5]. The use of other Lp -Liouvilleans is more recent (see [JPR2]) and they will not be discussed in this lecture. 3.2 Non-Equilibrium Steady States (NESS) and Entropy Production The central notions of non-equilibrium statistical mechanics are non-equilibrium steady states (NESS) and entropy production. Our definition of NESS follows closely the idea of Ruelle that a “natural” steady state should provide the statistics, over large time intervals [0, t], of initial configurations of the system which are typical with respect to the reference state [Ru3]. The definition of entropy production is more problematic since there is no physically satisfactory definition of the entropy itself out of equilibrium; see [Ga1, Ru2, Ru5, Ru7] for a discussion. Our definition of entropy production is motivated by classical dynamics where the rate of change of thermodynamic (Clausius) entropy can sometimes be related to the


9

phase space contraction rate [Ga2, RC]. The latter is related to the Gibbs entropy (as shown for example in [Ru3]) which is nothing else but the relative entropy with respect to the natural reference state; see [JPR1] for a detailed discussion in a more general context. Thus, it seems reasonable to define the entropy production as the rate of change of the relative entropy with respect to the reference state ω. Let (O, τ ) be a C ∗ -dynamical system and ω a given reference state. The NESS associated to ω and τ are the weak-∗ limit points of the time averages along the trajectory ω ◦ τ t . In other words, if 1 t ωt ≡ ω ◦ τ s ds, t 0 then ω+ is a NESS associated to ω and τ if there exists a net tα → ∞ such that ωtα (A) → ω+ (A) for all A ∈ O. We denote by Σ+ (ω, τ ) the set of such NESS. One easily sees that Σ+ (ω, τ ) ⊂ E(O, τ ). Moreover, since E(O) is weak-∗ compact, Σ+ (ω, τ ) is non-empty. As already mentioned, our definition of entropy production is based on the concept of relative entropy. The relative entropy of two density matrices ρ and ω is defined, by analogy with the relative entropy of two measures, by the formula Ent(ρ|ω) ≡ Tr(ρ(log ω − log ρ)).

(2)

It is easy to show that Ent(ρ|ω) ≤ 0. Let ϕi an orthonormal eigenbasis of ρ and Then p ∈ [0, 1] and by pi the corresponding eigenvalues. i i pi = 1. Let qi ≡ (ϕi , ω ϕi ). Clearly, qi ∈ [0, 1] and i qi = Tr ω = 1. Applying Jensen’s inequality twice we derive pi ((ϕi , log ω ϕi ) − log pi ) Ent(ρ|ω) = i

≤

i

pi (log qi − log pi ) ≤ log

qi = 0.

i

Hence Ent(ρ|ω) ≤ 0. It is also not difficult to show that Ent(ρ|ω) = 0 iff ρ = ω; see [OP]. Using the concept of relative modular operators, Araki has extended the notion of relative entropy to two arbitrary states on a C ∗ -algebra [Ar1,Ar2]. We refer the reader to [Ar1, Ar2, DJP, OP] for the definition of the Araki relative entropy and its basic properties. Of particular interest to us is that Ent(ρ|ω) ≤ 0 still holds, with equality if and only if ρ = ω. In these lecture notes we will define entropy production only in a perturbative context (for a more general approach see [JPR2]). Denote by δ the generator of the group τ i.e., τ t = etδ , and assume that the reference state ω is invariant under τ . For V = V ∗ ∈ O we set δV ≡ δ + i[V, ·] and denote by τVt ≡ etδV the corresponding perturbed C ∗ -dynamics (such perturbations are often called local, see [Pi]). Starting with a state ρ ∈ Nω , the entropy is pumped out of the system by the perturbation V at a mean rate

10


1 − (Ent(ρ ◦ τVt |ω) − Ent(ρ|ω)). t Suppose that ω is a modular state for a C ∗ -dynamics σωt and denote by δω the generator of σω . If V ∈ Dom (δω ), then one can prove the following entropy balance equation t

Ent(ρ ◦ τVt |ω) = Ent(ρ|ω) −

ρ(τVs (σV )) ds,

(3)

0

where σV ≡ δω (V ), is the entropy production observable (see [JP6, JP7]). In quantum mechanics σV plays the role of the phase space contraction rate of classical dynamical systems (see [JPR1]). We define the entropy production rate of a NESS tα 1 ρ ◦ τVs ds ∈ Σ+ (ρ, τV ), ρ+ = w∗ − lim α tα 0 by Ep(ρ+ ) ≡ − lim α

1 (Ent(ρ ◦ τVtα |ω) − Ent(ρ|ω)) = ρ+ (σV ). tα

Since Ent(ρ ◦ τVt |ω) ≤ 0, an immediate consequence of this equation is that, for ρ+ ∈ Σ+ (ρ, τV ), (4) Ep(ρ+ ) ≥ 0. We emphasize that the observable σV depends both on the reference state ω and on the perturbation V . As we shall see in the next section, σV is related to the thermodynamic fluxes across the system produced by the perturbation V and the positivity of entropy production is the statement of the second law of thermodynamics. 3.3 Structural Properties In this subsection we shall discuss structural properties of NESS and entropy production following [JP4]. The proofs are given in Appendix 9.1. First, we will discuss the dependence of Σ+ (ω, τV ) on the reference state ω. On physical grounds, one may expect that if ω is sufficiently regular and η is ω-normal, then Σ+ (η, τV ) = Σ+ (ω, τV ). Theorem 3.1. Assume that ω is a factor state on the C ∗ -algebra O and that, for all η ∈ Nω and A, B ∈ O, 1 T η([τVt (A), B]) dt = 0, lim T →∞ T 0 holds (weak asymptotic abelianness in mean). Then Σ+ (η, τV ) = Σ+ (ω, τV ) for all η ∈ Nω .


11

The second structural property we would like to mention is: Theorem 3.2. Let η ∈ O∗ be ω-normal and τV -invariant. Then η(σV ) = 0. In particular, the entropy production of the normal part of any NESS is equal to zero. If Ent(η|ω) > −∞, then Theorem 3.2 is an immediate consequence of the entropy balance equation (3). The case Ent(η|ω) = −∞ has been treated in [JP7] and the proof requires the full machinery of Araki’s perturbation theory. We will not reproduce it here. If ω+ is a factor state, then either ω+ ω or ω+ ⊥ ω. Hence, Theorem 3.2 yields: Corollary 3.1. If ω+ is a factor state and Ep(ω+ ) > 0, then ω+ ⊥ ω. If ω is also a factor state, then ω+ and ω are disjoint. Certain structural properties can be characterized in terms of the standard Liouvillean. Let L be the standard Liouvillean associated to τ and LV the standard Liouvillean associated to τV . By the well-known Araki’s perturbation formula, one has LV = L + V − JV J (see [DJP, Pi]). Theorem 3.3. Assume that ω is modular. (i) Under the assumptions of Theorem 3.1, if Ker LV = {0}, then it is onedimensional and there exists a unique normal, τV -invariant state ωV such that Σ+ (ω, τV ) = {ωV }. (ii) If Ker LV = {0}, then any NESS in Σ+ (ω, τV ) is purely singular. (iii) If Ker LV contains a separating vector for Mω , then Σ+ (ω, τV ) contains a unique state ω+ and this state is ω-normal. 3.4 C ∗ -Scattering and NESS Let (O, τ ) be a C ∗ -dynamical system and V a local perturbation. The abstract C ∗ scattering approach to the study of NESS is based on the following assumption: Assumption (S) The strong limit αV+ ≡ s − lim τ −t ◦ τVt , t→∞

exists. The map αV+ is an isometric ∗-endomorphism of O, and is often called Møller morphism. αV+ is one-to-one but it is generally not onto, namely O+ ≡ Ran αV+ = O. Since αV+ ◦ τVt = τ t ◦ αV+ , the pair (O+ , τ ) is a C ∗ -dynamical system and αV+ is an isomorphism between the dynamical systems (O, τV ) and (O+ , τ ).

12


If the reference state ω is τ -invariant, then ω+ = ω ◦ αV+ is the unique NESS associated to ω and τV and w∗ − lim ω ◦ τVt = ω+ . t→∞

Note in particular that if ω is a (τ, β)-KMS state, then ω+ is a (τV , β)-KMS state. The map αV+ is the algebraic analog of the wave operator in Hilbert space scattering theory. A simple and useful result in Hilbert space scattering theory is the Cook criterion for the existence of the wave operator. Its algebraic analog is: Proposition 3.3. (i) Assume that there exists a dense subset O0 ⊂ O such that for all A ∈ O0 , ∞

[V, τVt (A)] dt < ∞.

(5)

0

Then Assumption (S) holds. (ii) Assume that there exists a dense subset O1 ⊂ O such that for all A ∈ O1 , ∞ [V, τ t (A)] dt < ∞. (6) 0

Then O+ = O and αV+ is a ∗-automorphism of O. Proof. For all A ∈ O we have τ −t2 ◦ τVt2 (A) − τ −t1 ◦ τVt1 (A) = i

t2

τ −t ([V, τVt (A)]) dt,

t1

τV−t2 ◦ τ t2 (A) − τV−t1 ◦ τ t1 (A) = −i

(7)

t2 t1

τV−t ([V, τ t (A)]) dt,

and so τ −t2 ◦ τVt2 (A) − τ −t1 ◦ τVt1 (A) ≤

τV−t2 ◦ τ t2 (A) − τV−t1 ◦ τ t1 (A) ≤

t2

[V, τVt (A)] dt,

t1

(8) t2

[V, τ t (A)] dt.

t1

To prove Part (i), note that (5) and the first estimate in (8) imply that for A ∈ O0 the norm limit αV+ (A) ≡ lim τ −t ◦ τVt (A), t→∞

−t

exists. Since O0 is dense and τ ◦ τVt is isometric, the limit exists for all A ∈ O, and αV+ is a ∗-morphism of O. To prove Part (ii) note that the second estimate in (8) and (6) imply that the norm limit


13

βV+ (A) ≡ lim τV−t ◦ τ t (A), t→∞

also exists for all A ∈ O. Since αV+ ◦ βV+ (A) = A, αV+ is a ∗-automorphism of O. Until the end of this subsection we will assume that the Assumption (S) holds and that ω is τ -invariant. Let ω ˜ ≡ ω O+ and let (Hω˜ , πω˜ , Ωω˜ ) be the GNS-representation of O+ as˜ = ω. We denote by sociated to ω ˜ . Obviously, if αV+ is an automorphism, then ω (Hω+ , πω+ , Ωω+ ) the GNS representation of O associated to ω+ . Let Lω˜ and Lω+ be the standard Liouvilleans associated, respectively, to (O+ , τ, ω ˜ ) and (O, τV , ω+ ). Recall that Lω˜ is the unique self-adjoint operator on Hω˜ such that for A ∈ O+ , Lω˜ Ωω˜ = 0,

πω˜ (τ t (A)) = eitLω˜ πω˜ (A)e−itLω˜ ,

and similarly for Lω+ . Proposition 3.4. The map U πω˜ (αV+ (A))Ωω˜ = πω+ (A)Ωω+ , extends to a unitary U : Hω˜ → Hω+ which intertwines Lω˜ and Lω+ , i.e., U Lω˜ = Lω+ U.

Proof. Set πω˜ (A) ≡ πω˜ (αV+ (A)) and note that πω˜ (O)Ωω˜ = πω˜ (O+ )Ωω˜ , so that Ωω˜ is cyclic for πω˜ (O). Since ω+ (A) = ω(αV+ (A)) = ω ˜ (αV+ (A)) = (Ωω˜ , πω˜ (αV+ (A))Ωω˜ ) = (Ωω˜ , πω˜ (A)Ωω˜ ), (Hω˜ , πω˜ , Ωω˜ ) is also a GNS representation of O associated to ω+ . Since GNS representations associated to the same state are unitarily equivalent, there is a unitary U : Hω˜ → Hω+ such that U Ωω˜ = Ωω+ and U πω˜ (A) = πω+ (A)U. Finally, the identities U eitLω˜ πω˜ (A)Ωω˜ = U πω˜ (τ t (αV+ (A)))Ωω˜ = U πω˜ (αV+ (τVt (A)))Ωω˜ = πω+ (τVt (A))Ωω+ = eitLω+ πω+ (A)Ωω+ = eitLω+ U πω˜ (A)Ωω˜ , yield that U intertwines Lω˜ and Lω+ . We finish this subsection with:

14


Proposition 3.5.

(i) Assume that ω ˜ ∈ E(O+ , τ ) is τ -ergodic. Then Σ+ (η, τV ) = {ω+ },

for all η ∈ Nω . (ii) If ω ˜ is τ -mixing, then lim η ◦ τVt = ω+ ,

t→∞

for all η ∈ Nω . Proof. We will prove the Part (i); the proof of the Part (ii) is similar. If η ∈ Nω , ˜ yields then η O+ ∈ Nω˜ , and the ergodicity of ω 1 T →∞ T

lim

0

T

η(τ t (αV+ (A))) dt = ω ˜ (αV+ (A)) = ω+ (A).

This fact, the estimate η(τVt (A)) − η(τ t (αV+ (A))) ≤ τ −t ◦ τVt (A) − αV+ (A), and Assumption (S) yield the statement.

4 Open Quantum Systems 4.1 Definition Open quantum systems are the basic paradigms of non-equilibrium quantum statistical mechanics. An open system consists of a “small” system S interacting with a large “environment” or “reservoir” R. In these lecture notes the small system will be a ”quantum dot”—a quantum mechanical system with finitely many energy levels and no internal structure. The system S is described by a finite-dimensional Hilbert space HS = CN and a Hamiltonian HS . Its algebra of observables OS is the full matrix algebra MN (C) and its dynamics is given by τSt (A) = eitHS Ae−itHS = etδS (A), where δS (·) = i[HS , · ]. The states of S are density matrices on HS . A convenient reference state is the tracial state, ωS (·) = Tr(·)/ dim HS . In the physics literature ωS is sometimes called the chaotic state since it is of maximal entropy, giving the same probability 1/ dim HS to any one-dimensional projection in HS . The reservoir is described by a C ∗ -dynamical system (OR , τR ) and a reference state ωR . We denote by δR the generator of τR . The algebra of observables of the joint system S + R is O = OS ⊗ OR and its reference state is ω ≡ ωS ⊗ ωR . Its dynamics, still decoupled, is given by τ t = t . Let V = V ∗ ∈ O be a local perturbation which couples S to the reservoir τSt ⊗ τR


15

R. The ∗-derivation δV ≡ δR + δS + i[V, · ] generates the coupled dynamics τVt on O. The coupled joint system S + R is described by the C ∗ -dynamical system (O, τV ) and the reference state ω. Whenever the meaning is clear within the context, we will identify OS and OR with subalgebras of O via A ⊗ IOR , IOS ⊗ A. With a slight abuse of notation, in the sequel we denote IOR and IOS by I. We will suppose that the reservoir R has additional structure, namely that it consists of M parts R1 , · · · , RM , which are interpreted as subreservoirs. The subreservoirs are assumed to be independent—they interact only through the small system which allows for the flow of energy and matter between various subreservoirs. The subreservoir structure of R can be chosen in a number of different ways and the choice ultimately depends on the class of examples one wishes to describe. One obvious choice is the following: the j-th reservoir is described by the C ∗ -dynamical system (ORj , τRj ) and the reference state ωRj , and OR = ⊗ORj , τR = ⊗τRj , ω = ⊗ωRj [JP4, Ru1]. In view of the examples we plan to cover, we will choose a more general subreservoir structure. We will assume that the j-th reservoir is described by a C ∗ -subalgebra ORj ⊂ OR which is preserved by τR . We denote the restrictions of τR and ωR to ORj by τRj and ωRj . Different algebras ORj may not commute. However, we will assume that ORi ∩ ORj = CI for i = j. If Ak , 1 ≤ k ≤ N , are subsets of OR , we denote by A1 , · · · , AN the minimal C ∗ -subalgebra of OR that contains all Ak . Without loss of generality, we may assume that OR = OR1 , · · · , ORM . The system S is coupled to the reservoir Rj through a junction described by a self-adjoint perturbation Vj ∈ OS ⊗ ORj (see Fig. 1). The complete interaction is given by M V ≡ Vj . (9) j=1

An anti-linear, involutive, ∗-automorphism r : O → O is called a time reversal −t t = τR ◦ r. If r is a time reversal, if it satisfies r(HS ) = HS , r(Vj ) = Vj and r ◦ τR j j then r ◦ τVt = τV−t ◦ r, r ◦ τ t = τ −t ◦ r, and a state ω on O is time reversal invariant if ω ◦ r(A) = ω(A∗ ) for all A ∈ O. An open quantum system described by (O, τV ) and the reference state ω is called time reversal invariant (TRI) if there exists a time reversal r such that ω is time reversal invariant. 4.2 C ∗ -Scattering for Open Quantum Systems Except for Part (ii) of Proposition 3.3, the scattering approach to the study of NESS, described in Subsection 3.4, is directly applicable to open quantum systems. Concerning Part (ii) of Proposition 3.3, note that in the case of open quantum systems the Møller morphism αV+ cannot be onto (except in trivial cases). The best one may hope for is that O+ = OR , namely that αV+ is an isomorphism between the C ∗ dynamical systems (O, τV ) and (OR , τR ). The next theorem was proved in [Ru1].

16


Fig. 1. Junctions V1 , V2 between the system S and subreservoirs.

Theorem 4.1. Suppose that Assumption (S) holds. (i) If there exists a dense set OR0 ⊂ OR such that for all A ∈ OR0 , ∞ [V, τ t (A)] dt < ∞,

(10)

0

then OR ⊂ O+ . (ii) If there exists a dense set O0 ⊂ O such that for all X ∈ OS and A ∈ O0 , lim [X, τVt (A)] = 0,

t→+∞

(11)

then O+ ⊂ OR . (iii) If both (10) and (11) hold then αV+ is an isomorphism between the C ∗ dynamical systems (O, τV ) and (OR , τR ). In particular, if ωR is a (τR , β)KMS for some inverse temperature β, then ω+ is a (τV , β)-KMS state. Proof. The proof of Part (i) is similar to the proof of the Part (i) of Proposition 3.3. The assumption (10) ensures that the limits βV+ (A) = lim τVt ◦ τ −t (A), t→∞

exist for all A ∈ OR . Clearly, αV+ ◦ βV+ (A) = A for all A ∈ OR and so OR ⊂ Ran αV+ .


17

To prove Part (ii) recall that OS is a N 2 -dimensional matrix algebra. It has a basis {Ek | k = 1, · · · , N 2 } such that τ t (Ek ) = eitθk Ek for some θk ∈ R. From Assumption (S) and (11) we can conclude that 0 = lim eitθk τ −t ([Ek , τVt (A)]) = lim [Ek , τ −t ◦ τVt (A)] = [Ek , αV+ (A)], t→+∞

t→+∞

for all A ∈ O0 and hence, by continuity, for all A ∈ O. It follows that Ran αV+ belongs to the commutant of OS in O. Since O can be seen as the algebra MN (OR ) of N × N -matrices with entries in OR , one easily checks that this commutant is precisely OR . Part (iii) is a direct consequence of the first two parts. 4.3 The First and Second Law of Thermodynamics Let us denote by δj the generator of the dynamical group τRj . (Recall that this dynamical group is the restriction of the decoupled dynamics to the subreservoir Rj ). Assume that Vj ∈ Dom (δj ). The generator of τV is δV = δR + i[HS + V, · ] and it follows from (9) that the total energy flux out of the reservoir is given by d t τV (HS + V ) = τVt (δV (HS + V )) = τVt (δR (V )) = τVt (δj (Vj )). dt j=1 M

Thus, we can identify the observable describing the heat flux out of the j-th reservoir as Φj = δj (V ) = δj (Vj ) = δR (Vj ). We note that if r is a time-reversal, then r(Φj ) = −Φj . The energy balance equation M

Φj = δV (HS + V ),

j=1

yields the conservation of energy (the first law of thermodynamics): for any τV invariant state η, M η(Φj ) = 0. (12) j=1

Besides heat fluxes, there might be other fluxes across the system S + R (for example, matter and charge currents). We will not discuss here the general theory of such fluxes (the related information can be found in [FMU, FMSU, TM]). In the rest of this section we will focus on the thermodynamics of heat fluxes. Charge currents will be discussed in the context of a concrete model in the second part of this lecture. We now turn to the entropy production. Assume that there exists a C ∗ -dynamics t σR on OR such that ωR is (σR , −1)-KMS state and such that σR preserves each subalgebra ORj . Let δ˜j be the generator of the restriction of σR to ORj and assume

18


that Vj ∈ Dom (δ˜j ). The entropy production observable associated to the perturbation V and the reference state ω = ωS ⊗ ωR , where ωS (·) = Tr(·)/ dim HS , is M σV = δ˜j (Vj ). j=1

Until the end of this section we shall assume that the reservoirs ORj are in thermal equilibrium at inverse temperatures βj . More precisely, we will assume that ωRj is the unique (τRj , βj )-KMS state on ORj . Then δ˜j = −βj δj , and σV = −

M

βj Φj .

j=1

In particular, for any NESS ω+ ∈ Σ+ (ω, τV ), the second law of thermodynamics holds: M βj ω+ (Φj ) = −Ep(ω+ ) ≤ 0. (13) j=1

In fact, it is not difficult to show that Ep(ω+ ) is independent of the choice of the reference state of the small system as long as ωS > 0; see Proposition 5.3 in [JP4]. In the case of two reservoirs, the relation (β1 − β2 )ω+ (Φ1 ) = β1 ω+ (Φ1 ) + β2 ω+ (Φ2 ) ≤ 0, yields that the heat flows from the hot to the cold reservoir. 4.4 Linear Response Theory Linear response theory describes thermodynamics in the regime where the “forces” driving the system out of equilibrium are weak. In such a regime, to a very good approximation, the non-equilibrium currents depend linearly on the forces. The ultimate purpose of linear response theory is to justify well known phenomenological laws like Ohm’s law for charge currents or Fick’s law for heat currents. We are still far from a satisfactory derivation of these laws, even in the framework of classical mechanics; see [BLR] for a recent review on this matter. We also refer to [GVV6] for a rigorous discussion of linear response theory at the macroscopic level. A less ambitious application of linear response theory concerns transport properties of microscopic and mesoscopic quantum devices (the advances in nanotechnologies during the last decade have triggered a strong interest in the transport properties of such devices). Linear response theory of such systems is much better understood, as we shall try to illustrate. In our current setting, the forces that drive the system S + R out of equilibrium are the different inverse temperatures β1 , · · · , βM of the reservoirs attached to S. If all inverse temperatures βj are sufficiently close to some value βeq , we expect linear


19

response theory to give a good account of the thermodynamics of the system near thermal equilibrium at inverse temperature βeq . To emphasize the fact that the reference state ω = ωS ⊗ ωR depends on the βj we set X = (X1 , · · · , XM ) with Xj ≡ βeq − βj and denote by ωX this reference state. We assume that for some > 0 and all |X| < there exists a unique NESS ωX+ ∈ Σ+ (ωX , τV ) and that the functions X → ωX+ (Φj ) are C 2 . Note that ω0+ is the (unique) (τV , βeq )-KMS state on O. We will denote it simply by ωβeq . In phenomenological non-equilibrium thermodynamics, the duality between the driving forces Fα , also called affinities, and the steady currents φα they induce is expressed by the entropy production formula Ep = Fα φα , α

(see [DGM]). The steady currents are themselves functions of the affinities φα = φα (F1 , · · · ). In the linear response regime, these functions are given by the relations Lαγ Fγ , φα = γ

which define the kinetic coefficients Lαγ . Comparing with Equ. (13) and using energy conservation (12) we obtain in our case M Ep(ωX+ ) = Xj ωX+ (Φj ). j=1

Thus Xj is the affinity conjugated to the steady heat flux φj (X) = ωX+ (Φj ) out of Rj . We note in particular that the equilibrium entropy production vanishes. The kinetic coefficients Lji are given by ∂φj Lji ≡ = ∂Xi ωX+ (Φj )|X=0 . ∂Xi X=0 Taylor’s formula yields φj (X) = ωX+ (Φj ) =

M

Lji Xi + O(2 ),

(14)

i=1

Ep(ωX+ ) =

M

Lji Xi Xj + o(2 ).

(15)

i,j=1

Combining (14) with the first law of thermodynamics (recall (12)) we obtain that for all i, M Lji = 0. (16) j=1

20


Similarly, (15) and the second law (13) imply that the quadratic form M

Lji Xi Xj ,

i,j=1

on RM is non-negative. Note that this does not imply that the M × M -matrix L is symmetric ! Linear response theory goes far beyond the above elementary relations. Its true cornerstones are the Onsager reciprocity relations (ORR), the Kubo fluctuationdissipation formula (KF) and the Central Limit Theorem (CLT). All three of them deal with the kinetic coefficients. The Onsager reciprocity relations assert that the matrix Lji of a time reversal invariant (TRI) system is symmetric, Lji = Lij .

(17)

For non-TRI systems, similar relations hold between the transport coefficients of the system and those of the time reversed one. For example, if time reversal invariance is broken by the action of an external magnetic field B, then the Onsager-Casimir relations Lji (B) = Lij (−B), hold. The Kubo fluctuation-dissipation formula expresses the transport coefficients of a TRI system in terms of the equilibrium current-current correlation function Cji (t) ≡

1 ωβ (τ t (Φj )Φi + Φi τVt (Φj )), 2 eq V

namely Lji =

1 2

(18)

∞

−∞

Cji (t) dt.

(19)

The Central Limit Theorem further relates Lji to the statistics of the current fluctuations in equilibrium. In term of characteristic function, the CLT for open quantum systems in thermal equilibrium asserts that M √ t s M i ξj τV (Φj ) ds / t − 12 Dji ξj ξi j=1 i,j=1 0 , (20) lim ωβeq e =e t→∞

where the covariance matrix Dji is given by Dji = 2 Lji . If, for a self-adjoint A ∈ O, we denote by 1[a,b] (A) the spectral projection on the interval [a, b] of πωβeq (A), the probability of measuring a value of A in [a, b] when the system is in the state ωβeq is given by Probωβeq {A ∈ [a, b]} = (Ωωβeq , 1[a,b] (A) Ωωβeq ).


21

It then follows from (20) that

t b 2 2 a b 1 1 τVs (Φj ) ds ∈ √ , √ e−x /2Ljj dx. =√ lim Probωβeq t→∞ t 0 t t 2πLjj a (21) This is a direct translation to quantum mechanics of the classical central limit theorem. Because fluxes do not commute, [Φj , Φi ] = 0 for j = i, they can not be measured simultaneously and a simple classical probabilistic interpretation of (20) for the vector variable Φ = (Φ1 , · · · , ΦM ) is not possible. Instead, the quantum fluctuations of the vector variable Φ are described by the so-called fluctuation algebra [GVV1, GVV2, GVV3, GVV4, GVV5, Ma]. The description and study of the fluctuation algebra involve somewhat advanced technical tools and for this reason we will not discuss the quantum CLT theorem in this lecture. The mathematical theory of ORR, KF, and CLT is reasonably well understood in classical statistical mechanics (see the lecture [Re]). In the context of open quantum systems these important notions are still not completely understood (see however [AJPP, JPR2] for some recent results). We close this subsection with some general comments about ORR and KF. The definition (18) of the current-current correlation function involves a symmetrized product in order to ensure that the function Cji (t) is real-valued. The corresponding imaginary part, given by 1 i[Φi , τVt (Φj )], 2 is usually non-zero. However, since ωβeq is a KMS state, the stability condition (see [BR2]) yields ∞ ωβeq (i[Φi , τVt (Φj )]) dt = 0, (22) −∞

so that, in this case, the symmetrization is not necessary and one can rewrite KF as 1 ∞ ωβ (Φi τVt (Φj )) dt. Lji = 2 −∞ eq Finally, we note that ORR follow directly from KF under the TRI assumption. Indeed, if our system is TRI with time reversal r we have r(Φi ) = −Φi ,

r(τVt (Φj )) = −τV−t (Φj ),

ωβeq ◦ r = ωβeq ,

and therefore Cji (t) =

1 ωβ (τ −t (Φj )Φi + Φi τV−t (Φj )) = Cji (−t). 2 eq V

Since ωβeq is τV -invariant, this implies Cji (t) =

1 ωβ (Φj τVt (Φi ) + τVt (Φi )Φj ) = Cij (t), 2 eq

22


and ORR (17) follows from KF (19). In the second part of the lecture we will show that the Onsager relations and the Kubo formula hold for the SEBB model. The proof of the Central Limit Theorem for this model is somewhat technically involved and can be found in [AJPP]. 4.5 Fermi Golden Rule (FGR) Thermodynamics Let λ ∈ R be a control parameter. We consider an open quantum system with coupling λV and write τλ for τλV , ωλ+ for ω+ , etc. The NESS and thermodynamics of the system can be described, to second order of perturbation theory in λ, using the weak coupling (or van Hove) limit. This approach is much older than the ”microscopic” Hamiltonian approach discussed so far, and has played an important role in the development of the subject. The classical references are [Da1,Da2,Haa,VH1,VH2,VH3]. The weak coupling limit is also discussed in the lecture notes [D1]. In the weak coupling limit one “integrates” the degrees of freedom of the reservoirs and follows the reduced dynamics of S on a large time scale t/λ2 . In the limit λ → 0 the dynamics of S becomes irreversible and is described by a semigroup, often called the quantum Markovian semigroup (QMS). The generator of this QMS describes the thermodynamics of the open quantum system to second order of perturbation theory. The “integration” of the reservoir variables is performed as follows. As usual, we use the injection A → A ⊗ I to identify OS with a subalgebra of O. For A ∈ OS and B ∈ OR we set PS (A ⊗ B) = AωR (B). (23) The map PS extends to a projection PS : O → OS . The reduced dynamics of the system S is described by the family of maps Tλt : OS → OS defined by Tλt (A) ≡ PS τ0−t ◦ τλt (A ⊗ I) . Obviously, Tλt is neither a group nor a semigroup. Let ωS be an arbitrary reference state (density matrix) of the small system and ω = ωS ⊗ ωR . Then for any A ∈ OS , ω(τ0−t ◦ τλt (A ⊗ I)) = TrHS (ωS Tλt (A)). In [Da1, Da2] Davies proved that under very general conditions there exists a linear map KH : OS → OS such that t/λ2

lim Tλ

λ→0

(A) = etKH (A).

The operator KH is the QMS generator (sometimes called the Davies generator) in the Heisenberg picture. A substantial body of literature has been devoted to the study of the operator KH (see the lecture notes [D1]). Here we recall only a few basic results concerning thermodynamics in the weak coupling limit (for additional


23

information see [LeSp]). We will assume that the general conditions described in the lecture notes [D1] are satisfied. The operator KH generates a positivity preserving contraction semigroup on OS . Obviously, KH (I) = 0. We will assume that zero is the only purely imaginary eigenvalue of KH and that Ker KH = CI. This non-degeneracy condition can be naturally characterized in algebraic terms, see [D1,Sp]. It implies that the eigenvalue 0 of KH is semi-simple, that the corresponding eigenprojection has the form A → Tr(ωS + A)I, where ωS + is a density matrix, and that for any initial density matrix ωS , lim Tr(ωS etKH (A)) = Tr(ωS + A) ≡ ωS + (A). t→∞

The density matrix ωS + describes the NESS of the open quantum system in the weak coupling limit. One further shows that the operator KH has the form KH =

M

KH,j ,

j=1

where KH,j is the QMS generator obtained by considering the weak coupling limit of the coupled system S + Rj , i.e., −t/λ2 t/λ2 ◦ τλ,j (A ⊗ I) , (24) etKH,j (A) = lim PS τ0 λ→0

where τλ,j is generated by δj + i[HS + λVj , · ]. One often considers the QMS generator in the Schrödinger picture, denoted KS . The operator KS is the adjoint of KH with respect to the inner product (X, Y ) = Tr(X ∗ Y ). The semigroup etKS is positivity and trace preserving. One similarly defines KS,j . Obviously, KS (ωS + ) = 0,

KS =

M

KS,j .

j=1

Recall our standing assumption that the reservoirs ORj are in thermal equilibrium at inverse temperature βj . We denote by ωβ = e−βHS /Tr(e−βHS ), the canonical density matrix of S at inverse temperature β (the unique (τS , β)-KMS state on OS ). Araki’s perturbation theory of KMS-states (see [DJP,BR2]) yields that for A ∈ OS , t ωβj ⊗ ωRj (τ0−t ◦ τλ,j (A ⊗ I)) = ωβj (A) + O(λ),

uniformly in t. Hence, for all t ≥ 0, ωβj (etKH,j (A)) = ωβj (A),

24


and so KS,j (ωβj ) = 0. In particular, if all βj ’s are the same and equal to β, then ωS+ = ωβ . Let Od ⊂ OS be the ∗-algebra spanned by the eigenprojections of HS . Od is commutative and preserved by KH , KH,j , KS and KS,j [D1]. The NESS ωS+ commutes with HS . If the eigenvalues of HS are simple, then the restriction KH Od is a generator of a Markov process whose state space is the spectrum of HS . This process has played an important role in the early development of quantum field theory (more on this in Subsection 8.2). We now turn to the thermodynamics in the weak coupling limit, which we will call Fermi Golden Rule (FGR) thermodynamics. The observable describing the heat flux out of the j-th reservoir is Φfgr,j = KH,j (HS ). Note that Φfgr,j ∈ Od . Since KS (ωS + ) = 0 we have M

ωS + (Φfgr,j ) = ωS + (KH (HS )) = 0,

j=1

which is the first law of FGR thermodynamics. The entropy production observable is σfgr = −

M

βj Φfgr,j ,

(25)

j=1

and the entropy production of the NESS ωS + is Epfgr (ωS+ ) = ωS+ (σfgr ). Since the semigroup generated by KS,j is trace-preserving we have d Ent(etKS,j ωS + |ωβj )|t=0 = −βj ωS+ (Φfgr,j ) − Tr(KS,j (ωS+ ) log ωS+ ), dt where the relative entropy is defined by (2). The function t → Ent(etKS,j ωS + |ωβj ), is non-decreasing (see [Li]), and so M d Ent(etKS,j ωS + |ωβj )|t=0 ≥ 0, Epfgr (ωS + ) = dt j=1

which is the second law of FGR thermodynamics. Moreover, under the usual nondegeneracy assumptions, Epfgr (ωS + ) = 0 if and only if β1 = · · · = βM (see [LeSp] for details).


25

Let us briefly discuss linear response theory in FGR thermodynamics using the same notational conventions as in Subsection 4.4. The kinetic coefficients are given by Lfgr,ji = ∂Xi ωS + (Φfgr,j )|X=0 . For |X| < one has ωS + (Φfgr,j ) =

M

Lfgr,ji Xi + O(2 ),

i=1 M

Epfgr (ωS + ) =

Lfgr,ji Xi Xj + o(2 ).

i,j=1

The first and the second law yield that for all i, M

Lfgr,ji = 0,

j=1

and that the quadratic form M

Lfgr,ji Xi Xj ,

i,j=1

is non-negative. The Kubo formula ∞ Lfgr,ji = ωβeq (etKH (Φj ) Φi ) dt,

(26)

0

and the Onsager reciprocity relations Lfgr,ji = Lfgr,ij ,

(27)

are proven in [LeSp]. Finally, we wish to comment on the relation between microscopic and FGR thermodynamics. One naturally expects FGR thermodynamics to produce the first non-trivial contribution (in λ) to the microscopic thermodynamics. For example, the following relations are expected to hold for small λ: ωλ+ = ωS+ + O(λ), (28) ωλ+ (Φj ) = λ2 ωS+ (Φfgr,j ) + O(λ3 ). Indeed, it is possible to prove that if the microscopic thermodynamics exists and is sufficiently regular, then (28) hold. On the other hand, establishing existence and regularity of the microscopic thermodynamics is a formidable task which has been so far carried out only for a few models. FGR thermodynamics is very robust and the weak coupling limit is an effective tool in the study of the models whose microscopic thermodynamics appears beyond reach of the existing techniques. We will return to this topic in Section 8 where we will discuss the FGR thermodynamics of the SEBB model.

26


5 Free Fermi Gas Reservoir In the SEBB model, which we shall study in the second part of this lecture, the reservoir will be described by an infinitely extended free Fermi gas. Our description of the free Fermi gas in this section is suited to this application. The basic properties of the free Fermi gas are discussed in the lecture [Me3] and in Examples 4.6 and 5.6 of the lecture [Pi] and we will assume that the reader is familiar with the terminology and results described there. A more detailed exposition can be found in [BR2] and in the recent lecture notes [D2]. The free Fermi gas is described by the so called CAR (canonical anticommutation relations) algebra. The mathematical structure of this algebra is well understood (see [D2] for example). In Subsection 5.1 we will review the results we need. Subsection 5.2 contains a few useful examples. 5.1 General Description Let h and h be the Hilbert space and the Hamiltonian of a single Fermion. We will always assume that h is bounded below. Let Γ− (h) be the anti-symmetric Fock space over h and denote by a∗ (f ), a(f ) the creation and annihilation operators for a single Fermion in the state f ∈ h. The corresponding self-adjoint field operator 1 ϕ(f ) ≡ √ (a(f ) + a∗ (f )) , 2 satisfies the anticommutation relation ϕ(f )ϕ(g) + ϕ(g)ϕ(f ) = Re(f, g)I. In the sequel a# stands for either a or a∗ . Let CAR(h) be the C ∗ -algebra generated by {a# (f ) | f ∈ h}. We will refer to CAR(h) as the Fermi algebra. The C ∗ -dynamics induced by h is τ t (A) ≡ eitdΓ (h) Ae−itdΓ (h) . The pair (CAR(h), τ ) is a C ∗ -dynamical system. It preserves the Fermion number in the sense that τ t commutes with the gauge group ϑt (A) ≡ eitdΓ (I) Ae−itdΓ (I) . Recall that N ≡ dΓ (I) is the Fermion number operator on Γ− (h) and that τ and ϑ are the groups of Bogoliubov automorphisms τ t (a# (f )) = a# (eith f ),

ϑt (a# (f )) = a# (eit f ).

To every self-adjoint operator T on h such that 0 ≤ T ≤ I one can associate a state ωT on CAR(h) satisfying ωT (a∗ (fn ) · · · a∗ (f1 )a(g1 ) · · · a(gm )) = δn,m det{(gi , T fj )}.

(29)


27

This ϑ-invariant state is usually called the quasi-free gauge-invariant state generated by T . It is completely determined by its two point function ωT (a∗ (f )a(g)) = (g, T f ). We will often call T the density operator or simply the generator of the state ωT . Alternatively, quasi-free gauge-invariant states can be described by their action on the field operators. For any integer n we define Pn as the set of all permutations π of {1, . . . , 2n} such that π(2j − 1) < π(2j),

and

π(2j − 1) < π(2j + 1),

for every j ∈ {1, . . . , n}. Denote by (π) the signature of π ∈ Pn . ωT is the unique state on CAR(h) with the following properties: 1 (f1 , f2 ) − i Im(f1 , T f2 ), 2 n ωT (ϕ(f1 ) · · · ϕ(f2n )) = (π) ωT (ϕ(fπ(2j−1) )ϕ(fπ(2j) )), ωT (ϕ(f1 )ϕ(f2 )) =

j=1

π∈Pn

ωT (ϕ(f1 ) · · · ϕ(f2n+1 )) = 0. If h = h1 ⊕ h2 and T = T1 ⊕ T2 , then for A ∈ CAR(h1 ) and B ∈ CAR(h2 ) one has (30) ωT (A B) = ωT1 (A) ωT2 (B). ωT is a factor state. It is modular iff Ker T = Ker (I − T ) = {0}. Two states ωT1 and ωT2 are quasi-equivalent iff the operators 1/2

T1

1/2

− T2

and

(I − T1 )1/2 − (I − T2 )1/2 ,

(31)

are Hilbert-Schmidt; see [De, PoSt, Ri]. Assume that Ker Ti = Ker (I − Ti ) = {0}. Then the states ωT1 and ωT2 are unitarily equivalent iff (31) holds. If T = F (h) for some function F : σ(h) → [0, 1], then ωT describes a free Fermi gas with energy density per unit volume F (ε). The state ωT is τ -invariant iff T commutes with eith for all t. If the spectrum of h is simple this means that T = F (h) for some function F : σ(h) → [0, 1]. For any β, µ ∈ R, the Fermi-Dirac distribution ρβµ (ε) ≡ (1 + eβ(ε−µ) )−1 induces the unique β-KMS state on CAR(h) for the dynamics τ t ◦ ϑ−µt . This state, which we denote by ωβµ , describes the free Fermi gas at thermal equilibrium in the grand canonical ensemble with inverse temperature β and chemical potential µ. The GNS representation of CAR(h) associated to ωT can be explicitly computed as follows. Fix a complex conjugation f → f¯ on h and extend it to Γ− (h). Denote by Ω the vacuum vector and N the number operator in Γ− (h). Set HωT = Γ− (h) ⊗ Γ− (h), ΩωT = Ω ⊗ Ω, πωT (a(f )) = a((I − T )1/2 f ) ⊗ I + (−I)N ⊗ a∗ (T¯1/2 f¯).

28


The triple (HωT , πωT , ΩωT ) is the GNS representation of the algebra CAR(h) associated to ωT . (This representation was constructed in [AW] and if often called Araki-Wyss representation.) If ωT is τ -invariant, the corresponding ωT -Liouvillean is ¯ L = dΓ (h) ⊗ I − I ⊗ dΓ (h). If h has purely (absolutely) continuous spectrum so does L, except for the simple eigenvalue 0 corresponding to the vector ΩωT . On the other hand, 0 becomes a degenerate eigenvalue as soon as h has some point spectrum. Thus (see the lecture notes [Pi]) the ergodic properties of τ -invariant, gauge-invariant quasi-free states can be described in terms of the spectrum of h. The state ωT is ergodic iff h has no eigenvalues. If h has purely absolutely continuous spectrum, then ωT is mixing. If ωT is modular, then its modular operator is log ∆ωT = dΓ (s) ⊗ I − I ⊗ dΓ (¯ s), where s = log T (I −T )−1 . The corresponding modular conjugation is J(Φ⊗Ψ ) = ¯ where u = (−I)N (N +I)/2 . uΨ¯ ⊗ uΦ, Let θ be the ∗-automorphism of CAR(h) defined by θ(a(f )) = −a(f ).

(32)

A ∈ CAR(h) is called even if θ(A) = A and odd if θ(A) = −A. Every element A ∈ CAR(h) can be written in a unique way as a sum A = A+ + A− where A± = (A ± θ(A))/2 is even/odd. The set of all even/odd elements is a vector subspace of CAR(h) and CAR(h) is a direct sum of these two subspaces. It follows from (29) that ωT (A) = 0 if A is odd. Therefore one has ωT (A) = ωT (A+ ) and ωT ◦ θ = ωT .

(33)

The subspace of even elements is a C ∗ -subalgebra of CAR(h). This subalgebra is called even CAR algebra and is denoted by CAR+ (h). It is generated by {a# (f1 ) · · · a# (f2n ) | n ∈ N, fj ∈ h}. The even CAR algebra plays an important role in physics. It is preserved by τ and ϑ and the pair (CAR+ (h), τ ) is a C ∗ -dynamical system. We denote the restriction of ωT to CAR+ (h) by the same letter. In particular, ωβµ is the unique β-KMS state on CAR+ (h) for the dynamics τ t ◦ ϑ−µt . Let B = a# (g1 ) · · · a# (gm ), A = a# (f1 ) · · · a# (fn ), be two elements of CAR(h), where m is even. It follows from CAR that |(fi , eith gj )|, [A, τ t (B)] ≤ C i,j

where one can take C = (max(fi , gj ))n+m−2 . If the functions |(fi , eith gj )| belong to L1 (R, dt), then


∞

−∞

[A, τ t (B)] dt < ∞.

29

(34)

Let h0 ⊂ h be a subspace such that for any f, g ∈ h0 the function t → (f, eith g) is integrable. Let O0 = {a# (f1 ) · · · a# (fn ) | n ∈ N, fj ∈ h0 } and let O0+ be the even subalgebra of O0 . Then for A ∈ O0 and B ∈ O0+ (34) holds. If h0 is dense in h, then O0 is dense in CAR(h) and O0+ is dense in CAR+ (h). Let h1 and h2 be two Hilbert spaces, and let Ωh1 , Ωh2 be the vaccua in Γ− (h1 ) and Γ− (h2 ). The exponential law for Fermions (see [BSZ] and [BR2], Example 5.2.20) states that there exists a unique unitary map U : Γ− (h1 ⊕ h2 ) → Γ− (h1 ) ⊗ Γ− (h2 ) such that U Ωh1 ⊕h2 = Ωh1 ⊗ Ωh2 , U a(f ⊕ g)U −1 = a(f ) ⊗ I + (−I)N ⊗ a(g), U a∗ (f ⊕ g)U −1 = a∗ (f ) ⊗ I + (−I)N ⊗ a∗ (g),

(35)

U dΓ (h1 ⊕ h2 )U −1 = dΓ (h1 ) ⊗ I + I ⊗ dΓ (h2 ). The presence of the factors (−I)N in the above formulas complicates the description of a system containing several reservoirs. The following discussion should help the reader to understand its physical origin. Consider two boxes R1 , R2 with one particle Hilbert spaces hi ≡ L2 (Ri ). Denote by R the combined box i.e., the disjoint union of R1 and R2 . The corresponding one particle Hilbert space is h ≡ L2 (R). Identifying the wave function Ψ1 of an electron in R1 with Ψ1 ⊕ 0 and similarly for an electron in R2 we can replace h with the direct sum h1 ⊕ h2 . Assume that each box Ri contains a single electron with wave functions Ψi (see Fig. 2). If the boxes are in thermal contact, the two electrons can exchange energy, but the first one will always stay in R1 and the second one in R2 . Thus they are distinguishable and the total wave function is just Ψ1 ⊗ Ψ2 . The situation is completely different if the electrons are free to move from one box into the other. In this case, the electrons are indistinguishable and Pauli’s principle requires the total wave function to be antisymmetric—the total wave function is Ψ1 ∧ Ψ2 . Generalizing this argument to many electrons states we conclude that the second quantized Hilbert

Fig. 2. Thermal contact and open gate between R1 and R2 .

30


space is Γ− (h1 ) ⊗ Γ− (h2 ) in the case of thermal contact and Γ− (h1 ⊕ h2 ) in the other case. The exponential law provides a unitary map U between these two Hilbert and one easily checks that U Ψ1 ∧ Ψ2 = U a∗ (Ψ1 ⊕ 0)a∗ (0 ⊕ Ψ2 )Ωh1 ⊕h2 = (a∗ (Ψ1 )(−I)N ⊗ a∗ (Ψ2 ))Ωh1 ⊗ Ωh2 = Ψ1 ⊗ Ψ2 . Denoting by OR1 , OR2 and OR the CAR (or more appropriately the CAR+ ) algebras of the boxes R1 , R2 and R, the algebra of the combined system in the case of thermal contact is OR1 ⊗ OR2 , while it is OR in the other case. We emphasize that the unitary map U does not yield an isomorphism between these algebras i.e., U OR U ∗ = OR1 ⊗ OR2 . This immediately follows from the observation that (−I)N ∈ OR1 (unless, of course, OR1 is finite dimensional, see Subsection 6.3), which implies U a∗ (0 ⊕ Ψ2 )U ∗ = (−I)N ⊗ a∗ (Ψ2 ) ∈ OR1 ⊗ OR2 . Note in particular that a∗ (Ψ1 ) ⊗ I and I ⊗ a∗ (Ψ2 ) commute while a∗ (Ψ1 ⊕ 0) and a∗ (0 ⊕ Ψ2 ) anticommute. The factor (−I)N is required in order for a∗ (Ψ1 ) ⊗ I and (−I)N ⊗ a∗ (Ψ2 ) to anticommute. 5.2 Examples Recall that the Pauli matrices are defined by 01 0 −i σx ≡ , σy ≡ , 10 i 0

1 0 σz ≡ . 0 −1

We set σ± ≡ (σx ± iσy )/2. Clearly, σx2 = σy2 = σz2 = I and σx σy = −σy σx = iσz . More generally, with σ = (σx , σy , σz ) and u, v ∈ R3 one has (u · σ )(v · σ ) = u · v I + i(u × v ) · σ .

Example 5.1. Assume that dim h = 1, i.e., that h = C and that h is the operator of multiplication by the real constant ω. Then Γ− (h) = C⊕C = C2 and dΓ (h) = ωN with 1 00 N ≡ dΓ (I) = = (I − σz ). 01 2 Moreover, one easily checks that


00 01 a(1) = , a∗ (1) = , 10 00 10 00 , a(1)a∗ (1) = , a∗ (1)a(1) = 00 01

31

(36)

which shows that CAR(h) is the algebra of 2 × 2 matrices M2 (C) and CAR+ (h) its subalgebra of diagonal matrices. A self-adjoint operator 0 ≤ T ≤ I on H is multiplication by a constant γ, 0 ≤ γ ≤ 1. The associated state ωT on CAR(h) is given by the density matrix 1−γ 0 . 0 γ Example 5.2. Assume that dim h = n. Without loss of generality we can set h = Cn and assume that hfj = ωj fj for some ωj ∈ R, where {fj } is the standard basis of Cn . Then, Γ− (h) = C ⊕ Cn ⊕ Cn ∧ Cn ⊕ · · · ⊕ (Cn )∧n

n

C2 ,

i=1

and CAR(h) is isomorphic to the algebra of 2n × 2n matrices M2n (C). This isomorphism is explicitly given by n a(fj ) ⊗j−1 i=1 σz ⊗ σ+ ⊗ ⊗i=j+1 I , for j = 1, . . . , n. It follows that a∗ (fj )a(fj )

1 j−1 ⊗i=1 I ⊗ (I − σz ) ⊗ ⊗ni=j+1 I . 2

The map described by the above formulas is called the Jordan-Wigner transformation. It is a useful tool in the study of quantum spin systems (see [LMS, AB, Ar3]). For β, µ ∈ R, the quasi-free gauge-invariant state associated to T = (I + eβ(h−µ) )−1 is given by the density matrix e−β(H−µN ) , Tr e−β(H−µN ) with H ≡ dΓ (h) =

n j=1

ωj a∗ (fj )a(fj ),

N ≡ dΓ (I) =

n

a∗ (fj )a(fj ).

j=1

It is an instructive exercise to work out the thermodynamics of the finite dimensional free Fermi gas following Section 3 in [Jo].

32


Example 5.3. In this example we will briefly discuss the finite dimensional approximation of a free Fermi gas. Assume that h is a separable Hilbert space and let Λn ⊂ Dom h be an increasing sequence of finite dimensional subspaces. The algebras CAR(Λn ) are identified with subalgebras of CAR(h). We also assume that ∪n Λn is dense in h. Let pn be the orthogonal projection on Λn . Set hn = pn hpn and let τn be the corresponding C ∗ -dynamics on CAR(Λn ). Since pn converges strongly to I one has, for f ∈ H, lim a# (pn f ) − a# (f ) = 0,

lim τnt (a# (pn f )) − τ t (a# (f )) = 0.

n→∞

n→∞

Let ωT be the gauge-invariant quasi-free state on CAR(h) associated to T . Let Tn = pn T pn . Then lim ωTn (a∗ (pn f )a(pn g)) = ωT (a∗ (f )a(g)).

n→∞

Assume that µ and η are two faithful ωT -normal states and let Ent(µ|η) be their Araki relative entropy. Let µn and ηn be the restrictions of µ and η to CAR+ (Λn ). Then the function n → Ent(µn |ηn ) = TrΛn (µn (log µn − log ηn )), is monotone increasing and lim Ent(µn |ηn ) = Ent(µ|η).

n→∞

Additional information about the last result can be found in [BR2], Proposition 6.2.33. Example 5.4. The tight binding approximation for an electron in a single Bloch band of a d-dimensional (cubic) crystal is defined by h ≡ 2 (Zd ) with the translation invariant Hamiltonian 1 ψ(y), (37) (hψ)(x) ≡ 2d |x−y|=1

where |x| ≡ i |xi |. In the sequel δx denotes the Kronecker delta function at x ∈ Zd . Writing ax ≡ a(δx ), the second quantized energy and number operators are given by 1 ∗ dΓ (h) = ax ay , dΓ (I) = a∗x ax . 2d x |x−y|=1

ˆ The Fourier transform ψ(k) ≡

x

ψ(x) e−ix·k maps h unitarily onto

ˆ ≡ L2 ([−π, π]d , dk ). h (2π)d


33

The set [−π, π]d is the Brillouin zone of the crystal and k is the quasi-momentum of the electron. The Fourier transform diagonalizes the Hamiltonian which becomes multiplication by the band function ε(k) ≡ d1 i cos(ki ). Thus h has purely absolutely continuous spectrum σ(h) = [−1, 1], and in particular is bounded. A simple stationary phase argument shows that (f, eith g) = O(t−n ), for arbitrary n provided fˆ and gˆ are smooth and vanish in a neighborhood of the critical set {k | |∇k ε(k)| = 0}. Since this set has Lebesgue measure 0, such functions are dense in h. If f and g have bounded support in Zd , then (f, eith g) = O(t−d/2 ).

Example 5.5. The tight binding approximation of a semi-infinite wire is obtained by restricting the Hamiltonian (37), for d = 1, to the space of odd functions ψ ∈ 2 (Z) and identifying such ψ with elements of 2 (Z+ ), where Z+ ≡ {1, 2, · · · }. This is clearly equivalent to imposing a Dirichlet boundary condition at x = 0 and ∞

h=

1 ((δx , · )δx+1 + (δx+1 , · )δx ) . 2 x=1

2 ˜ The Fourier-sine transform ψ(k) ≡ x∈Z+ ψ(x) sin(kx) maps unitarily (Z+ ) onto the space L2 ([0, π], 2dk π ) and the Hamiltonian becomes multiplication by cos k. By a simple change of variable r = cos k we obtain the spectral representation of the Hamiltonian h: (hψ)# (r) = rψ # (r),

where ψ # (r) ≡

2 ˜ √ ψ(arccos(r)), π 1 − r2

2 maps unitarily the Fourier space L2 ([0, π], 2dk π ) onto L ([−1, 1], dr). A straightforward integration by parts shows that

(f, eith g) = O(t−n ), if f # , g # ∈ C0n ((−1, 1)). A more careful analysis shows that (f, eith g) = O(t−3/2 ), if f and g have bounded support in Z+ .

34


Example 5.6. The non-relativistic spinless Fermion of mass m is described in the position representation by the Hilbert space L2 (Rd , dx) and the Hamiltonian h = −∆/2m, where ∆ is the usual Laplacian in Rd . The cases of physical interest are d = 1, 2, 3. In the momentum representation the Hilbert space of the Fermion is L2 (Rd , dk) and its Hamiltonian (which we will again denote by h) is the operator of multiplication by |k|2 /2m. The spectrum of h is purely absolutely continuous. Integration by parts yields that (f, eith g) = O(t−n ), for arbitrary n provided fˆ and gˆ are smooth, compactly supported and vanish in a neighborhood of the origin. Such functions are dense in h. If f, g ∈ h are compactly supported in the position representation, then (f, eith g) = O(t−d/2 ).

6 The Simple Electronic Black-Box (SEBB) Model In the second part of this lecture we shall study in detail the non-equilibrium statistical mechanics of the simplest non-trivial example of the electronic black box model introduced in [AJPP]. The electronic black-box model is a general, independent electron model for a localized quantum device S connected to M electronic reservoirs R1 , · · · , RM . The device is called black-box since, according to the scattering approach introduced in Subsection 4.2, the thermodynamics of the coupled system is largely independent of the internal structure of the device. The NESS and the steady currents are completely determined by the Møller morphism which in our simple model further reduces to the one-particle wave operator. 6.1 The Model The black-box itself is a two level system. Its Hilbert space is HS ≡ C2 , its algebra of observables is OS ≡ M2 (C), and its Hamiltonian is 0 0 HS ≡ . 0 ε0 The associated C ∗ -dynamics is τSt (A) = eitHS A e−itHS . The black-box has a oneparameter family of steady states with density matrices 1−γ 0 ωS ≡ , γ ∈ [0, 1], 0 γ which we shall use as the reference states. According to Example 5.1 of Subsection 5.2, we can also think of S as a free Fermi gas over C, namely HS = Γ− (C), HS = dΓ (ε0 ) = ε0 a∗ (1)a(1) and OS =


35

CAR(C). In this picture, the black-box S can only accommodate a single Fermion of energy ε0 . We denote by NS = a∗ (1)a(1) the corresponding number operator. In physical terms, S is a quantum dot without internal structure. We also note that ωS is the quasi-free gauge-invariant state generated by TS ≡ γ. Therefore, we can interpret γ as the occupation probability of the box. Let hR be a Hilbert space and hR a self-adjoint operator on hR . We set OR ≡ CAR(hR ) and t (A) ≡ eitdΓ (hR ) A e−itdΓ (hR ) . τR The reference state of the reservoir, ωR , is the quasi-free gauge-invariant state associated to the radiation density operator TR . We assume that hR is bounded from below and that TR commutes with hR . To introduce the subreservoir structure we shall assume that hR = ⊕M j=1 hRj ,

hR = ⊕M j=1 hRj ,

TR = ⊕M j=1 TRj .

The algebra of observables of the j-th reservoir is ORj ≡ CAR(hRj ) and its dynamics τRj ≡ τR ORj is generated by the Hamiltonian dΓ (hRj ). The state ωRj = ωR ORj is the gauge-invariant quasi-free state associated to TRj . If pj is the orthogonal projection on hRj , then NRj = dΓ (pj ) is the charge (or number) operator associated to the j-th reservoir. The total charge operator of the reservoir M is NR = j=1 NRj . The algebra of observables of the joint system S + R is O ≡ OS ⊗ OR , its reference state is ω = ωS ⊗ ωR , and its decoupled dynamics is τ0 = τS ⊗ τR . Note that τ0t (A) = eitH0 A e−itH0 , where H0 ≡ HS ⊗ I + I ⊗ dΓ (hR ). The junction between the box S and the reservoir Rj works in the following way: The box can make a transition from its ground state to its excited state by absorbing an electron of Rj in state fj /fj . Reciprocally, the excited box can relax to its ground state by emitting an electron in state fj /fj in Rj . These processes have a fixed rate λ2 fj 2 . More precisely, the junction is described by λVj ≡ λ (a(1) ⊗ a∗ (fj ) + a∗ (1) ⊗ a(fj )) , where λ ∈ R and the fj ∈ hj . The normalization is fixed by the condition 2 j fj = 1. The complete interaction is given by λV ≡

M

λVj = λ(a(1) ⊗ a∗ (f ) + a∗ (1) ⊗ a(f )),

j=1

where f ≡ ⊕M j=1 fj . Note that “charge” is conserved at the junction, i.e., V commutes with the total number operator N ≡ NS ⊗ I + I ⊗ NR . The full Hamiltonian is

36


Hλ ≡ H0 + λV, and the corresponding C ∗ -dynamics τλt (A) ≡ eitHλ A e−itHλ , is charge-preserving. In other words, τλ commutes with the gauge group ϑt (A) ≡ eitN A e−itN , and [Hλ , N ] = 0. The C ∗ -dynamical system (O, τλ ) with its decoupled dynamics τ0t and the reference state ω = ωS ⊗ ωR is our simple electronic black box model (SEBB). This model is an example of the class of open quantum systems described in Section 4. 6.2 The Fluxes The heat flux observables have been defined in Subsection 4.3. The generator of τRj is given by δj (·) = i[dΓ (hRj ), · ]. Note that Vj ∈ Dom δj iff fj ∈ Dom hRj . If Vj ∈ Dom δj , then the observable describing the heat flux out of Rj is Φj = λδj (Vj ) = λ(a(1) ⊗ a∗ (ihRj fj ) + a∗ (1) ⊗ a(ihRj fj )). In a completely similar way we can define the charge current. The rate of change of the charge in the box S is d t τ (NS )|t=0 = i [dΓ (Hλ ), NS ] dt λ = −λ i [NS , V ] = λ i [NR , V ] =

M

(38) λ i [NRj , V ],

j=1

which allows us to identify Jj ≡ λ i [NRj , V ] = λ i [NRj , Vj ] = λ i [NR , Vj ] = λ(a(1) ⊗ a∗ (ifj ) + a∗ (1) ⊗ a(ifj ), as the observable describing the charge current out of Rj . Let us make a brief comment concerning these definitions. If hRj is finite dimensional, then the energy and the charge of Rj are observables, given by the Hamiltonian dΓ (hRj ) and the number operator NRj = dΓ (pj ), and d t τ (dΓ (hRj ))|t=0 = λ i[dΓ (hRj ), Vj ] = Φj , dt λ d − τλt (dΓ (pj ))|t=0 = λ i[dΓ (pj ), Vj ] = Jj . dt

−


37

When hRj becomes infinite dimensional (recall Example 5.3 in Subsection 5.2), dΓ (hRj ) and NRj are no longer observables. However, the flux observables Φj and Jj are still well-defined and they are equal to the limit of the flux observables corresponding to finite-dimensional approximations. The first law of thermodynamics (energy conservation) has been verified in Subsection 4.3—for any τλ -invariant state η one has M

η(Φj ) = 0.

j=1

The analogous statement for charge currents is proved in a similar way. By (38), M

Jj =

j=1

d t τ (NS )|t=0 , dt λ

and so for any τλ -invariant state η one has M

η(Jj ) = 0.

(39)

j=1

6.3 The Equivalent Free Fermi Gas In this subsection we shall show how to use the exponential law for fermionic systems to map the SEBB model to a free Fermi gas. Let ⎞ ⎛ M ˜ ≡ CAR(h), O h0 ≡ ε0 ⊕ hR , hRj ⎠ , h ≡ C ⊕ hR = C ⊕ ⎝ j=1

and, with a slight abuse of notation, denote by 1, f1 , · · · , fM the elements of h canonically associated with 1 ∈ C and fj ∈ hRj . Then vj ≡ (1, · )fj + (fj , · )1, is a finite rank, self-adjoint operator on h and so is the sum v ≡ set hλ ≡ h0 + λv,

M j=1

vj . We further

and define the dynamical group τ˜λt (A) ≡ eitdΓ (hλ ) A e−itdΓ (hλ ) , ˜ Finally, we set on O.

T˜ ≡ TS ⊕ TR ,

˜ generated by T˜. and denote by ω ˜ be the quasi-free gauge-invariant state on O

(40)

38


Theorem 6.1. Let U : Γ− (C⊕hR ) → Γ− (C)⊗Γ− (hR ) be the unitary map defined by the exponential law (35) and set φ(A) ≡ U −1 AU . ˜ is a ∗-isomorphism. (i) φ : O → O t ◦ φ. (ii) For any λ, t ∈ R one has φ ◦ τλt = τ˜−λ (iii) ω = ω ˜ ◦ φ. (iv) For j = 1, · · · , M , one has Φ˜j ≡ φ(Φj ) = −λ (a∗ (ihj fj )a(1) + a∗ (1)a(ihj fj )) , and

J˜j ≡ φ(Jj ) = −λ(a∗ (ifj )a(1) + a∗ (1)a(ifj )).

Proof. Clearly, φ is a ∗-isomorphism from B(Γ− (C ⊕ h)) onto B(Γ− (C) ⊗ Γ− (h)). Using the canonical injections C → h and hR → h we can identify OS and OR ˜ generated by a(1 ⊕ 0) and {a(0 ⊕ f ) | f ∈ hR }. With with the subalgebras of O this identification, (35) gives φ(a(α) ⊗ I + (−I)NS ⊗ a(f )) = a(α) + a(f ), for α ∈ C and f ∈ hR . We conclude that φ(A ⊗ I) = A,

(41)

for any A ∈ OS . In particular, since b ≡ (−I)NS = [a(1), a∗ (1)] ∈ OS , we have φ(b ⊗ I) = b. Relation b2 = I yields φ(I ⊗ a(f )) = b a(f ). Since [b, a(f )] = 0, we conclude that for A ∈ OR

+ A if A ∈ OR , (42) φ(I ⊗ A) = − , b A if A ∈ OR ± where OR denote the even and odd parts of OR . Equ. (41) and (42) show that ˜ Since O ˜ = OS , O+ , O− , it follows from φ(OS ⊗ I) = OS , φ(I ⊗ φ(O) ⊂ O. R R + + − − ˜ This proves Part (i). OR ) = OR and φ(b ⊗ OR ) = OR that φ(O) ⊃ O. −1 From (35) we can see that U H0 U = dΓ (h0 ) and from (41) and (42) that

U −1 Vj U = φ(Vj ) = a(1) b a∗ (fj ) + a∗ (1) b a(fj ). Since it also follows from CAR that a(1) b = −a(1),

a∗ (1) b = a∗ (1),

(43)

we get U −1 Vj U = −a(1) a∗ (fj )+a∗ (1) a(fj ) = −a(1) a∗ (fj )−a(fj ) a∗ (1) = −dΓ (vj ). Therefore U −1 Hλ U = dΓ (h−λ ) from which Part (ii) follows. A similar computation yields Part (iv).


39

It remains to prove Part (iii). Using the morphism θ (recall Equ. (32)) to express the even and odd parts of B ∈ OR , we can rewrite (41) and (42) as φ(A ⊗ B) = A(B + θ(B))/2 + A b (B − θ(B))/2, from which we easily get φ(A ⊗ B) = Aa(1)a∗ (1)B + Aa∗ (1)a(1)θ(B). It follows from the factorization property (30) and the invariance property (33) of quasi-free states that ω (B) + ω ˜ (Aa∗ (1)a(1))˜ ω (B) ω ˜ ◦ φ(A ⊗ B) = ω ˜ (Aa(1)a∗ (1))˜ ∗ ∗ =ω ˜ (Aa(1)a (1)B + Aa (1)a(1)B) =ω ˜ (AB) = ω ˜ (A)˜ ω (B) = ωS (A)ωR (B) = ω(A ⊗ B). By Theorem 6.1, the SEBB model can be equivalently described by the C ∗ ˜ τ˜−λ ) and the reference state ω ˜ . The heat and charge flux dynamical system (O, T ˜ observables are Φj and J˜j . Since the change λ → −λ affects neither the model nor ˜ τ˜λ ) and we will drop the the results, in the sequel we will work with the system (O, ∗ ∼. Hence, we will use the C -algebra O = CAR(C ⊕ hR ) and C ∗ -dynamics τλt (A) = eitdΓ (hλ ) Ae−itdΓ (hλ ) , with the reference state ω, the quasi-free gauge-invariant state generated by T = TS ⊕ TR . The corresponding heat and charge flux observables are Φj ≡ λ (a∗ (ihj fj )a(1) + a∗ (1)a(ihj fj )) , Jj ≡ λ(a∗ (ifj )a(1) + a∗ (1)a(ifj )). The entropy production observable associated to ω is computed as follows. Assume that for j = 1, · · · , M one has Ker TRj = Ker (I − TRj ) = {0} and set sj ≡ − log TRj (I − TRj )−1 ,

sR = ⊕M j=1 sj .

We also assume that 0 < γ < 1 and set sS = log γ(1 − γ)−1 . Let s ≡ −sS ⊕ sR . Under the above assumptions, the reference state ω is modular and its modular automorphism group is σωt (A) = eitdΓ (s) A e−itdΓ (s) . If fj ∈ Dom(sj ), then the entropy production observable is σ = −λ (a∗ (f )a(isS ) + a∗ (isS )a(f )) − λ (a∗ (isR f )a(1) + a∗ (1)a(isR f )) . (44)

40


The entropy balance equation Ent(ω ◦ τλt |ω) = −

t

ω(τλs (σ)) ds, 0

holds and so, as in Subsection 3.2, the entropy production of any NESS ω+ ∈ Σ+ (ω, τλ ) is non-negative. In fact, it is not difficult to show that the entropy production of ω+ is independent of γ as long as γ ∈ (0, 1) (see Proposition 5.3 in [JP4]). In the sequel, whenever we speak about the entropy production, we will assume that γ = 1/2 and hence that σ = −λ (a∗ (isR f )a(1) + a∗ (1)a(isR f )) . In particular, if

(45)

TRj = (I + eβj (hRj −µj ) ),

then sj = −βj (hRj − µj ), and σ=−

M

βj (Φj − µj Jj ).

(46)

j=1

We finish with the following remark. In the physics literature, the Hamiltonian (40) is sometimes called the Wigner-Weisskopf atom [WW] (see [JKP] for references and additional information). The operators of this type are also often called Friedrich Hamiltonians [Fr]. The point we wish to emphasize is that such Hamiltonians are often used as toy models which allow for simple mathematical analysis of physically important phenomena. 6.4 Assumptions In this subsection we describe a set of assumptions under which we shall study the thermodynamics of the SEBB model. Assumption (SEBB1) hRj = L2 ((e− , e+ ), dr) for some −∞ < e− < e+ ≤ ∞ and hRj is the operator of multiplication by r. The assumption (SEBB1) yields that hR = L2 ((e− , e+ ), dr; CM ) and that hR is the operator of multiplication by r. With a slight abuse of the notation we will sometimes denote hRj and hR by r. Note that the spectrum of hR is purely absolutely continuous and equal to [e− , e+ ] with uniform multiplicity M . With the shorthand f ≡ (f1 , · · · , fM ) ∈ hR , the Hamiltonian (40) acts on C ⊕ hR and has the form (47) hλ = ε0 ⊕ r + λ((1, · )f + (f, · )1). Assumption (SEBB2) The functions


gj (t) ≡

e+

41

eitr |fj (r)|2 dr,

e−

belong to L1 (R, dt). Assumption (SEBB2) implies that the function e+ ∞ |f (r)|2 G(z) ≡ dr = −i g(t) e−itz dt, r−z 0 e− which is obviously analytic in the lower half-plane C− ≡ {z | Im z < 0}, is con¯ − . We denote by G(r − io) the value of this tinuous and bounded on its closure C function at r ∈ R. Assumption (SEBB3) For j = 1, · · · , M , the generator TRj is the operator of multiplication by a continuous function ρj (r) such that 0 < ρj (r) < 1 for r ∈ (e− , e+ ). Moreover, if ρj (r) sj (r) ≡ log , 1 − ρj (r) we assume that sj (r)fj (r) ∈ L2 ((e− , e+ ), dr). Assumption (SEBB3) ensures that the reference state ωR of the reservoir is modular. The function ρj (r) is the energy density of the j-th reservoir. The second part of this assumption ensures that the entropy production observable (44) is well defined. The study of SEBB model depends critically on the spectral and scattering properties of hλ . Our final assumption will ensure that Assumption (S) of Subsection 3.4 holds and will allow us to use a simple scattering approach to study SEBB. Assumption (SEBB4) ε0 ∈ (e− , e+ ) and |f (ε0 )| = 0. We set

F (r) ≡ ε0 − r − λ G(r − io) = ε0 − r − λ 2

e+

2 e−

|f (r )|2 dr . r − r + io

(48)

By a well-known result in harmonic analysis (see, e.g., [Ja] or any harmonic analysis textbook), (49) Im F (r) = λ2 π|f (r)|2 , for r ∈ (e− , e+ ). We also mention that for any g ∈ hR = L2 ((e− , e+ ), dr; CM ), the function e+ ¯ f (r ) · g(r ) dr , r → e− r − r + io is also in hR . The main spectral and scattering theoretic results on hλ are given in the following Theorem which is an easy consequence of the techniques described in [Ja]. Its proof can be found in [JKP].

42


Theorem 6.2. Suppose that Assumptions (SEBB1), (SEBB2) and (SEBB4) hold. Then there exists a constant Λ > 0 such that, for any 0 < |λ| < Λ: (i) The spectrum of hλ is purely absolutely continuous and equal to [e− , e+ ]. (ii) The wave operators W± ≡ s − lim eith0 e−ithλ , t→±∞

exist and are complete, i.e., Ran W± = hR and W± : h → hR are unitary. Moreover, if ψ = α ⊕ g ∈ h, then e+ ¯ f (r ) · g(r ) −1 dr f (r). (50) α−λ (W− ψ)(r) = g(r) − λF (r) e− r − r + io Needless to say, the thermodynamics of the SEBB model can be studied under much more general assumptions than (SEBB1)-(SEBB4). However, these assumptions allow us to describe the results of [AJPP] with the least number of technicalities. Parenthetically, we note that the SEBB model is obviously time-reversal invariant. Write fj (r) = eiθj (r) |fj (r)|, and let ¯ ⊕ (e2iθ1 g¯1 , · · · , e2iθM g¯M ), j(α ⊕ (g1 , · · · , gM )) = α where ¯· denotes the usual complex conjugation. Then the map r(A) = Γ (j)AΓ (j−1 ). is a time reversal and ω is time reversal invariant. Finally, as an example, consider a concrete SEBB model where each reservoir is a semi-infinite wire in the tight-binding approximation described in Example 5.5 of Subsection 5.2. Thus, for each j, hRj = 2 (Z+ ) and hRj is the discrete Laplacian on Z+ with Dirichlet boundary condition at 0. Choosing fj = δ1 we obtain, in the spectral representation of hRj , hRj = L2 ((−1, 1), dr), hRj = r, fj# (r) =

2 (1 − r2 )1/4 . π

Thus, Assumptions (SEBB1) and (SEBB4) hold. Since, as t → ∞, one has 1 2M J1 (t) = O(t−3/2 ), eitr |f # (r)|2 dr = t −1 where J1 denotes a Bessel function of the first kind, Assumption (SEBB2) is also satisfied. Hence, if 0 ∈ (−1, 1), then the conclusions of Theorem 6.2 hold. In fact one can show that in this case 1 − |ε0 | . Λ= 2M


43

7 Thermodynamics of the SEBB Model Throughout this and the next section we will assume that Assumptions (SEBB1)(SEBB4) hold.

7.1 Non-Equilibrium Steady States In this subsection we show that the SEBB model has a unique NESS ωλ+ which does not depend on the choice of the initial state η ∈ Nω . Recall that the reference state ω of the SEBB model is the quasi-free gauge-invariant state generated by T = TS ⊕ TR , where TS = γ ∈ (0, 1) and TR = ⊕j ρj (r). Theorem 7.1. Let Λ > 0 be the constant introduced in Theorem 6.2. Then, for any real λ such that 0 < |λ| < Λ the following hold: (i) The limit

αλ+ (A) ≡ lim τ0−t ◦ τλt (A), t→∞

(51)

exists for all A ∈ O. Moreover, Ran αλ+ = OR and αλ+ is an isomorphism between the C ∗ -dynamical systems (O, τλ ) and (OR , τR ). (ii) Let ωλ+ ≡ ωR ◦ αλ+ . Then lim η ◦ τλt = ωλ+ ,

t→∞

for all η ∈ Nω . (iii) ωλ+ is the gauge-invariant quasi-free state on O generated by T+ ≡ W−∗ TR W− , where W− is the wave operator of Theorem 6.2. Proof. Recall that τλt is a group of Bogoliubov automorphisms, τλt (a# (f )) = a# (eithλ f ). Hence, for any observable of the form A = a# (ψ1 ) · · · a# (ψn ),

(52)

τ0−t ◦ τλt (A) = a# (e−ith0 eithλ ψ1 ) · · · a# (e−ith0 eithλ ψn ). It follows from Theorem 6.2 that lim τ −t t→∞ 0

◦ τλt (A) = a# (W− ψ1 ) · · · a# (W− ψn ).

Since the linear span of set of elements of the form (52) is dense in O, the limit (51) exists and is given by the Bogoliubov morphism αλ+ (a# (f )) = a# (W− f ). Since W− is a unitary operator between h and hR , Ran αλ+ = CAR(hR ) = OR , which proves Part (i).

44


Since hR has purely absolutely continuous spectrum, it follows from our discussion of quasi-free states in Subsection 5.1 that ωR is mixing for τ0t . Part (ii) is thus a restatement of Proposition 3.5. If A = a∗ (ψn ) · · · a∗ (ψ1 )a(φ1 ) · · · a(φm ) is an element of O, then ω + (A) = ωR (a∗ (W− ψn ) · · · a∗ (W− ψ1 )a(W− φ1 ) · · · a(W− φm )) = δn,m det {(W− φi , TR W− ψj )} = δn,m det {(φi , T+ ψj )}. and Part (iii) follows. 7.2 The Hilbert-Schmidt Condition Since ω and ωλ+ are factor states, they are either quasi-equivalent (Nω = Nωλ+ ) or disjoint (Nω ∩ Nωλ+ = ∅). Since Ker T = Ker (I − T ) = {0}, we also have Ker T+ = Ker (I − T+ ) = {0}, and so ω and ωλ+ are quasi-equivalent iff they are unitarily equivalent. Let α > 0. A function h : (e− , e+ ) → C is α-Hölder continuous if there exists a constant C such that for all r, r ∈ (e− , e+ ), |h(r) − h(r )| ≤ C|r − r |α . Theorem 7.2. Assume that all the densities ρj (r) are the same and equal to ρ(r). Assume further that the functions ρ(r)1/2 and (1−ρ(r))1/2 are α-Hölder continuous for some α > 1/2. Then the operators (T+ )1/2 − T 1/2

and

(I − T+ )1/2 − (I − T )1/2

are Hilbert-Schmidt. In particular, the reference state ω and the NESS ωλ+ are unitarily equivalent and Ep(ωλ+ ) = 0. Remark. We will prove this theorem in Appendix 9.2. Although the Hölder continuity assumption is certainly not optimal, it covers most cases of interest and allows for a technically simple proof. Theorem 7.2 requires a comment. By the general principles of statistical mechanics, one expects that Ep(ωλ+ ) = 0 if and only if all the reservoirs are in thermal equilibrium at the same inverse temperature β and chemical potential µ (see Section 4.3 in [JP4]). This is not the case in the SEBB model because the perturbations Vj are chosen in such a special way that the coupled dynamics is still given by a Bogoliubov automorphism. Following the strategy of [JP4], one can show that the Planck law ρ(r) = (1 + eβ(r−µ) )−1 can be deduced from the stability requirement Ep(ωλ+ ) = 0 for a more general class of interactions Vj . For reasons of space we will not discuss this subject in detail in these lecture notes (the interested reader may consult [AJPP]). We will see below that the entropy production of the SEBB model is nonvanishing whenever the density operators of the reservoirs are not identical.


45

7.3 The Heat and Charge Fluxes Recall that the observables describing heat and charge currents out of the j-th reservoir are Φj = λ(a∗ (irfj )a(1) + a∗ (1)a(irfj )), Jj = λ(a∗ (ifj )a(1) + a∗ (1)a(ifj )). The expectation of the currents in the state ωλ+ are thus ωλ+ (Φj ) = iλωλ+ a∗ (rfj )a(1) − a∗ (1)a(rfj ) = 2λIm (rfj , T+ 1) = 2λIm (W− rfj , TR W− 1), and ωλ+ (Jj ) = iλωλ+ a∗ (fj )a(1) − a∗ (1)a(fj ) = 2λIm (fj , T+ 1) = 2λIm (W− fj , TR W− 1). Setting

Gj (r) ≡

e+

e−

r|fj (r )|2 dr , r − r + io

it easily follows from Formula (50) that for k = 1, · · · , M , (TR W− 1)k (r) = −λ

ρk (r)fk (r) , F (r)

(W− rfj )k (r) = δkj rfj (r) + λ2

Gj (r)fk (r) , F (r)

from which we obtain M

(W− rfj , TR W− 1) = −λ

e+

e−

k=1

|fk (r)|2 ρk (r) ¯ ¯ j (r) dr. rF (r)δkj + λ2 G |F (r)|2

¯ j (r) = From Equ. (49) we have Im F¯ (r) = −λ2 π|f (r)|2 and similarly Im G πr|fj (r)|2 . Hence, ωλ+ (Φj ) = 2πλ4

M

e−

k=1

Since |f |2 =

k

e+

r|fk (r)|2 ρk (r) |f (r)|2 δkj − |fj (r)|2 dr. 2 |F (r)|

|fk |2 , the last formula can be rewritten as

ωλ+ (Φj ) = 2πλ4

M k=1

e+

e−

|fj (r)|2 |fk (r)|2 (ρj (r) − ρk (r))

rdr . |F (r)|2

(53)

46


In a completely similar way one obtains ωλ+ (Jj ) = 2πλ

4

M

e+

|fj (r)|2 |fk (r)|2 (ρj (r) − ρk (r))

e−

k=1

dr . |F (r)|2

(54)

An immediate consequence of Formulas (53) and (54) is that all the fluxes vanish if ρ1 = · · · = ρM . Note also the antisymmetry in k and j of the integrands which ensures that the conservation laws M

ωλ+ (Φj ) =

j=1

M

ωλ+ (Jj ) = 0,

j=1

hold. 7.4 Entropy Production By the Assumption (SEBB3) the entropy production observable of the SEBB model is well defined and is given by Equ. (45) which we rewrite as σ = −λ

M

(a∗ (isj fj )a(1) + a∗ (1)a(isj fj )) .

(55)

j=1

Proceeding as in the previous section we obtain ωλ+ (σ) = −2λ

M

Im (W− sj fj , TR W− 1),

j=1

which yields ωλ+ (σ) = 2πλ4

M j,k=1

e+

e−

|fj (r)|2 |fk (r)|2 (sj (r) − sk (r)) ρk (r) dr. |F (r)|2

Finally, symmetrizing the sum over j and k we get

ωλ+ (σ) = πλ4

M j,k=1

e+

e−

|fj (r)|2 |fk (r)|2 (sj (r) − sk (r)) (ρk (r) − ρj (r)) dr. |F (r)|2

Since ρj = (1 + esj )−1 is a strictly decreasing function of sj , (sj (r) − sk (r))(ρk (r) − ρj (r)) ≥ 0, with equality if and only if ρk (r) = ρj (r). We summarize:


47

Theorem 7.3. The entropy production of ωλ+ is ωλ+ (σ) = πλ

4

M j,k=1

e+

e−

|fj (r)|2 |fk (r)|2 (sj (r) − sk (r)) (ρk (r) − ρj (r)) dr. |F (r)|2

In particular, Ep(ω+ ) ≥ 0 (something we already know from the general principles) and Ep(ω+ ) = 0 if and only if ρ1 = · · · = ρM . Since ω and ωλ+ are factor states, they are either quasi-equivalent or disjoint. By Theorem 3.2, if Ep(ωλ+ ) > 0, then ωλ+ is not ω-normal. Hence, Theorem 7.3 implies that if the densities ρj are not all equal, then the reference state ω and the NESS ωλ+ are disjoint states. Until the end of this section we will assume that the energy density of the j-th reservoir is 1 , ρβj µj (r) ≡ 1 + eβj (r−µj ) where βj is the inverse temperature and µj ∈ R is the chemical potential of the j-th reservoir. Then, by (46), Ep(ωλ+ ) can be written as Ep(ωλ+ ) = Epheat (ωλ+ ) + Epcharge (ωλ+ ), where Epheat (ωλ+ ) = −

M

βj ωλ+ (Φj ),

j=1

is interpreted as the entropy production due to the heat fluxes and Epcharge (ωλ+ ) =

M

βj µj ωλ+ (Jj ).

j=1

as the entropy production due to the electric currents. 7.5 Equilibrium Correlation Functions In this subsection we compute the integrated current-current correlation functions 1 T →∞ 2

Lρ (A, B) ≡ lim

T

−T

ωρ+ (τλt (A)B) dt,

where A and B are heat or charge flux observables and ωρ+ denotes the NESS ωλ+ in the equilibrium case ρ1 = · · · = ρM = ρ. To do this, note that Φl = dΓ (ϕl ) and Jl = dΓ (jl ) where ϕl = i[hRl , λv] = −i[hλ , hRj ], jl = i[pj , λv] = −i[hλ , pj ],

48


are finite rank operators. We will only consider Lρ (Φj , Φk ), the other cases are completely similar. Using the CAR, Formula (29) and the fact that ωρ+ (Φl ) = 0, one easily shows that ωρ+ (τλt (Φj )Φk ) = Tr (T+ eithλ ϕj e−ithλ (I − T+ )ϕk ). Since

d ithλ e hRj e−ithλ , dt the integration can be explicitly performed and we have eithλ ϕj e−ithλ = −

T 1 ithλ −ithλ Lρ (Φj , Φk ) = − lim Tr (T+ e hRj e (I − T+ )ϕk ) . T →∞ 2 −T Writing eithλ hRj e−ithλ = eithλ e−ith0 hRj eith0 e−ithλ and using the fact that ϕk is finite rank, we see that the limit exists and can be expressed in terms of the wave operators W± as Lρ (Φj , Φk ) =

1 Tr (T+ W−∗ hRj W− (I − T+ )ϕk ) 2 − Tr (T+ W+∗ hRj W+ (I − T+ )ϕk ) .

The intertwining property of the wave operators gives T+ = W−∗ ρ(hR )W− = ρ(hλ ) = W+∗ ρ(hR )W+ , from which we obtain Lρ (Φj , Φk ) =

1 Tr (TR (I − TR )hRj (W− ϕk W−∗ − W+ ϕk W+∗ )), 2

with TR = ρ(hR ). Time reversal invariance further gives W+ = jW− j,

j ϕk j = −ϕk ,

and so Lρ (Φj , Φk ) =

1 Tr (TR (I − TR )hRj (W− ϕk W−∗ + j W− ϕk W−∗ j)) 2

= Tr (TR (I − TR )hRj W− ϕk W−∗ ). The last trace is easily evaluated (use the formula ϕk = λi[hRk , v] and follow the steps of the computation in Subsection 7.3). The result is


49

r2 dr Lρ (Φj , Φk ) = −2πλ4 |fj (r)|2 |fk (r)|2 − δjk |f (r)|2 ρ(r)(1 − ρ(r)) , |F (r)|2 e− e+ rdr 4 |fj (r)|2 |fk (r)|2 − δjk |f (r)|2 ρ(r)(1 − ρ(r)) , Lρ (Jj , Φk ) = −2πλ |F (r)|2 e− e+ rdr , Lρ (Φj , Jk ) = −2πλ4 |fj (r)|2 |fk (r)|2 − δjk |f (r)|2 ρ(r)(1 − ρ(r)) |F (r)|2 e− e+ dr . Lρ (Jj , Jk ) = −2πλ4 |fj (r)|2 |fk (r)|2 − δjk |f (r)|2 ρ(r)(1 − ρ(r)) |F (r)|2 e− (56) e+

Note the following symmetries: Lρ (Φj , Φk ) = Lρ (Φk , Φj ), Lρ (Jj , Jk ) = Lρ (Jk , Jj ), Lρ (Φj , Jk ) = Lρ (Jk , Φj ).

(57)

Note also that Lρ (Φj , Φk ) ≤ 0 and Lρ (Jj , Jk ) ≤ 0 for j = k while Lρ (Φj , Φj ) ≥ 0 and Lρ (Jj , Jj ) ≥ 0. 7.6 Onsager Relations. Kubo Formulas. Let βeq and µeq be given equilibrium values of the inverse temperature and the chemical potential. The affinities (thermodynamic forces) conjugated to the currents Φj and Jj are Yj = βj µj − βeq µeq . Xj = βeq − βj , Indeed, it follows from the conservations laws (12) and (39) that Ep(ωλ+ ) =

M

(Xj ωλ+ (Φj ) + Yj ωλ+ (Jj )) .

j=1

Since ρβj µj (r) =

1 , 1 + eβeq (r−µeq )−(Xj r+Yj )

we have ∂Xk ρβj µj (r)|X=Y =0 = δkj ρ(r)(1 − ρ(r)) r, ∂Yk ρβj µj (r)|X=Y =0 = δkj ρ(r)(1 − ρ(r)), where ρ ≡ ρβeq µeq . Using these formulas, and explicit differentiation of the steady currents (53) and (54) and comparison with (56) lead to ∂Xk ωλ+ (Φj )|X=Y =0 = Lρ (Φj , Φk ), ∂Yk ωλ+ (Φj )|X=Y =0 = Lρ (Φj , Jk ), ∂Xk ωλ+ (Jj )|X=Y =0 = Lρ (Jj , Φk ), ∂Yk ωλ+ (Jj )|X=Y =0 = Lρ (Jj , Jk ),

50


which are the Kubo Fluctuation-Dissipation Formulas. The symmetry (57) gives the Onsager reciprocity relations ∂Xj ωλ + (Φk )|X=Y =0 = ∂Xk ωλ + (Φj )|X=Y =0 , ∂Yj ωλ + (Jk )|X=Y =0 = ∂Yk ωλ + (Jj )|X=Y =0 , ∂Yj ωλ + (Φk )|X=Y =0 = ∂Xk ωλ + (Jj )|X=Y =0 . The fact that Lρ (Φj , Φj ) ≥ 0 and Lρ (Jj , Jj ) ≥ 0 while Lρ (Φj , Φk ) ≤ 0 and Lρ (Jj , Jk ) ≤ 0 for j = k means that increasing a force results in an increase of the conjugated current and a decrease of the other currents. This is not only true in the linear regime. Direct differentiation of (53) and (54) yields e+ r2 dr |fj (r)|2 |fk (r)|2 ρβk µk (r)(1 − ρβk µk (r)) ≥ 0, ∂Xk ωλ + (Φk ) = 2πλ4 |F (r)|2 j =k e− e+ dr |fj (r)|2 |fk (r)|2 ρβk µk (r)(1 − ρβk µk (r)) ≥ 0, ∂Yk ωλ + (Jk ) = 2πλ4 |F (r)|2 j =k e− e+ r2 dr 4 ∂Xk ωλ + (Φj ) = −2πλ |fj (r)|2 |fk (r)|2 ρβk µk (r)(1 − ρβk µk (r)) ≤ 0, |F (r)|2 e− e+ dr ≤ 0. ∂Yk ωλ + (Jj ) = −2πλ4 |fj (r)|2 |fk (r)|2 ρβk µk (r)(1 − ρβk µk (r)) |F (r)|2 e− Note that these derivatives do not depend on the reference states of the reservoirs Rj for j = k.

8 FGR Thermodynamics of the SEBB Model For j = 1, · · · , M , we set g˜j (t) ≡

e+

eitr ρj (r)|fj (r)|2 dr. e−

In addition to (SEBB1)-(SEBB4) in this section we will assume Assumption (SEBB5) g˜j (t) ∈ L1 (R, dt) for j = 1, · · · , M .

8.1 The Weak Coupling Limit In this subsection we study the dynamics restricted to the small system on the van Hove time scale t/λ2 . Recall that by Theorem 6.1 the algebra of observables OS of the small system is the 4-dimensional subalgebra of O = CAR(C ⊕ hR ) generated by a(1). It is


51

the full matrix algebra of the subspace hS ⊂ Γ− (C ⊕ hR ) generated by the vectors {Ω, a(1)Ω}. In this basis, the Hamiltonian and the reference state of the small system are 0 0 1−γ 0 . , ωS = HS = 0 ε0 0 γ Let A ∈ OS be an observable of the small system. We will study the expectation values t/λ2 (58) ω(τλ (A)), as λ → 0. If A = a# (1), then (58) vanishes, so we need only to consider the Abelian 2-dimensional even subalgebra OS+ ⊂ OS . Since a∗ (1)a(1) = NS and a(1)a∗ (1) = I − NS , it suffices to consider A = NS . In this case we have t/λ2

ω ◦ τλ

(NS ) = ω(a∗ (eithλ /λ 1)a(eithλ /λ 1)) 2

2

2

2

= (eithλ /λ 1, (γ ⊕ TR )eithλ /λ 1).

(59)

Using the projection pj on the Hilbert space hRj of the j-th reservoir we can rewrite this expression as t/λ2

ω ◦ τλ

2

(NS ) = γ|(1, eithλ /λ 1)|2 +

M

2

2

(pj eithλ /λ 1, TRj pj eithλ /λ 1).

j=1

Theorem 8.1. Assume that Assumptions (SEBB1)-(SEBB5) hold. (i) For any t ≥ 0,

lim |(1, eithλ /λ 1)|2 = e−2πt|f (ε0 )| . 2

2

λ→0

(60)

(ii) For any t ≥ 0 and j = 1, · · · , M , 2

2

lim (pj eithλ /λ 1, TRj pj eithλ /λ 1) =

λ→0

|fj (ε0 )|2 −2πt|f (ε0 )|2 . ρ (ε ) 1 − e j 0 |f (ε0 )|2 (61)

The proof of Theorem 8.1 is not difficult—for Part (i) see [Da1, D1], and for Part (ii) [Da2]. These proofs use the regularity Assumption (SEBB5). An alternative proof of Theorem 8.1, based on the explicit form of the wave operator W− , can be found in [JKP]. Theorem 8.1 implies that t/λ2

γ(t) ≡ lim ω ◦ τλ λ→0

(NS )

M 2 2 |fj (ε0 )|2 = γ e−2πt|f (ε0 )| + 1 − e−2πt|f (ε0 )| ρj (ε0 ), |f (ε0 )|2 j=1

from which we easily conclude that for all A ∈ OS one has

52

Walter Aschbacher et al. t/λ2

lim ω ◦ τλ

λ→0

(A) = Tr(ωS (t)A),

1 − γ(t) 0 ωS (t) = . 0 γ(t)

where

According to the general theory described in Section 4.5 we also have ωS (t) = etKS ωS , where KS is the QMS generator in the Schrödinger picture. We shall now discuss its restriction to the algebra of diagonal 2 × 2-matrices. In the basis 10 00 , , (62) 00 01 of this subalgebra we obtain the matrix representation M −ρj (ε0 ) 1 − ρj (ε0 ) 2 KS = 2π |fj (ε0 )| . ρj (ε0 ) −(1 − ρj (ε0 )) j=1 In the Heisenberg picture we have t/λ2

lim ωS ◦ τλ

λ→0

(A) = Tr(ωS etKH A),

where KH is related to KS by the duality Tr(KS (ωS )A) = Tr(ωS KH (A)). The restriction of KH to the subalgebra of diagonal 2 × 2-matrices has the following matrix representation relative to the basis (62), M ρj (ε0 ) −ρj (ε0 ) 2 KH = 2π |fj (ε0 )| . 1 − ρj (ε0 ) −(1 − ρj (ε0 )) j=1 We stress that KS and KH are the diagonal parts of the full Davies generators in the Schrödinger and Heisenberg pictures discussed in the lecture notes [D1]. As we have discussed in Section 4.5, an important property of the generators KS and KH is the decomposition KS =

M j=1

KS,j ,

KH =

M

KH,j ,

j=1

where KS,j and KH,j are the generators describing interaction of S with the j-th reservoir only. Explicitly,


KS,j KH,j

53

−ρj (ε0 ) 1 − ρj (ε0 ) = 2π|fj (ε0 )|2 , ρj (ε0 ) −(1 − ρj (ε0 )) ρj (ε0 ) −ρj (ε0 ) = 2π|fj (ε0 )|2 . 1 − ρj (ε0 ) −(1 − ρj (ε0 ))

Finally, we note that ωS+ ≡ lim ωS (t) = t→∞

M |fj (ε0 )|2 j=1

1 − ρj (ε0 )

0

0

ρj (ε0 )

|f (ε0 )|2

.

ωS+ is the NESS on the Fermi Golden Rule time scale: for any observable A of the small system, t/λ2

lim lim ω ◦ τλ

t→∞ λ→0

(A) = Tr(ωS+ A) = ωS+ (A).

In the sequel we will refer to ωS+ as the FGR NESS. 8.2 Historical Digression—Einstein’s Derivation of the Planck Law Einstein’s paper [Ei], published in 1917, has played an important role in the historical development of quantum mechanics and quantum field theory. In this paper Einstein made some deep insights into the nature of interaction between radiation and matter which have led him to a new derivation of the Planck law. For the history of these early developments the interested reader may consult [Pa]. The original Einstein argument can be paraphrased as follows. Consider a twolevel quantum system S with energy levels 0 and ε0 , which is in equilibrium with a radiation field reservoir with energy density ρ(r). Due to the interaction with the reservoir, the system S will make constant transitions between the energy levels 0 and ε0 . Einstein conjectured that the corresponding transition rates (transition probabilities per unit time) have the form k(ε0 , 0) = Aε0 (1 − ρ(ε0 )),

k(0, ε0 ) = Bε0 ρ(ε0 ),

where Aε0 and Bε0 are the coefficients which depend on the mechanics of the interaction. (Of course, in 1917 Einstein considered the bosonic reservoir (the light)—in this case in the first formula one has 1 + ρ(ε0 ) instead of 1 − ρ(ε0 )). These formulas are the celebrated Einstein’s A and B laws. Let p¯0 and p¯ε0 be probabilities that in equilibrium the small system has energies 0 and ε0 respectively. If S is in thermal equilibrium at inverse temperature β, then by the Gibbs postulate, p¯0 = (1 + e−βε0 )−1 ,

p¯ε0 = e−βε0 (1 + e−βε0 )−1 .

The equilibrium condition k(0, ε0 )¯ p0 = k(ε0 , 0)¯ pε0 ,

54


yields ρ(ε0 ) =

Aε0 (1 − ρ(ε0 ))e−βε0 . Bε0

In 1917 Einstein naturally could not compute the coefficients Aε0 and Bε0 . However, if Aε0 /Bε0 = 1 for all ε0 , then the above relation yields the Planck law for energy density of the free fermionic reservoir in thermal equilibrium, ρ(ε0 ) =

1 . 1 + eβε0

In his paper Einstein points out that to compute the numerical value of Aε0 and Bε0 one would need an exact [quantum] theory of electro-dynamical and mechanical processes. The quantum theory of mechanical processes was developed in the 1920’s by Schrödinger, Heisenberg, Jordan, Dirac and others. In 1928, Dirac extended quantum theory to electrodynamical processes and computed the coefficients Aε0 and Bε0 from the first principles of quantum theory. Dirac’s seminal paper [Di] marked the birth of quantum field theory. To compute Aε0 and Bε0 Dirac developed the so-called time-dependent perturbation theory, which has been discussed in lecture notes [D1, JKP] (see also Chapter XXI in [Mes], or any book on quantum mechanics). In his 1949 Chicago lecture notes [Fer] Fermi called the basic formulas of Dirac’s theory the Golden Rule, and since then they have been called the Fermi Golden Rule. In this section we have described the mathematically rigorous Fermi Golden Rule theory of the SEBB model. In this context Dirac’s theory reduces to the computation of KS and KH since the matrix elements of these operators give the transition probabilities k(ε0 , 0) and k(0, ε0 ). In particular, in the case of a single reservoir with energy density ρ(r), Aε0 = Bε0 = 2π|f (ε0 )|2 . Einstein’s argument can be rephrased as follows: if the energy density ρ is such that 0 −βHS −βHS −βε0 −1 1 /Tr(e ) = (1 + e ) ωS+ = e , 0 e−βε0 for all ε0 (namely HS ), then ρ(ε0 ) =

1 . 1 + eβε0

8.3 FGR Fluxes, Entropy Production and Kubo Formulas Any diagonal observable A ∈ OS+ of the small system is a function of the Hamiltonian HS . We identify such an observable with a function g : {0, ε0 } → R. Occasionally, we will write g as a column vector with components g(0) and g(ε0 ). In


55

the sequel we will use such identifications without further comment. A vector ν is called a probability vector if ν(0) ≥ 0, ν(ε0 ) ≥ 0 and ν(0) + ν(ε0 ) = 1. The diagonal part of any density matrix defines a probability vector. We denote the probability vector associated to FGR NESS ωS+ by the same letter. Similarly, to a probability vector one uniquely associates a diagonal density matrix. With these conventions, the Hamiltonian and the number operator of the small system are 0 0 ∗ ∗ HS = ε0 a (1)a(1) = . , NS = a (1)a(1) = ε0 1

The Fermi Golden Rule (FGR) heat and charge flux observables are ρj (ε0 ) Φfgr,j = KH,j (HS ) = 2πε0 |fj (ε0 )|2 , −(1 − ρj (ε0 )) ρj (ε0 ) . Jfgr,j = KH,j (NS ) = 2π|fj (ε0 )|2 −(1 − ρj (ε0 )) The steady heat and the charge currents in the FGR NESS are given by ωS+ (Φfgr,j ) = 2π

M |fj (ε0 )|2 |fk (ε0 )|2

|f (ε0 )|2

k=1

ωS+ (Jfgr,j ) = 2π

M |fj (ε0 )|2 |fk (ε0 )|2

|f (ε0 )|2

k=1

ε0 (ρj (ε0 ) − ρk (ε0 )), (63) (ρj (ε0 ) − ρk (ε0 )).

The conservation laws M

ωS+ (Φfgr,j ) = 0,

j=1

M

ωS+ (Jfgr,j ) = 0,

j=1

follow from the definition of the fluxes and the relation KS (ωS+ ) = 0. Of course, they also follow easily from the above explicit formulas. Until the end of this subsection we will assume that ρj (r) =

1 1+

eβj (r−µj )

.

Using Equ. (63), we can also compute the expectation of the entropy production in the FGR NESS ωS+ . The natural extension of the definition (25) is σfgr ≡ −

M j=1

from which we get

βj (Φfgr,j − µj Jfgr,j ) ,

56


ωS+ (σfgr ) = 2π

M |fj (ε0 )|2 |fk (ε0 )|2 (ρk (ε0 ) − ρj (ε0 ))βj (ε0 − µj ). |f (ε0 )|2

(64)

j,k=1

Writing ρj (ε0 ) = βj (ε0 − µj ), 1 − ρj (ε0 ) and symmetrizing the sum in Equ. (64) we obtain sj ≡ log

ωS+ (σfgr ) = π

M |fj (ε0 )|2 |fk (ε0 )|2 (ρk (ε0 ) − ρj (ε0 ))(sj − sk ), |f (ε0 )|2

j,k=1

which is non-negative since ρl (ε0 ) is a strictly decreasing function of sl . The FGR entropy production vanishes iff all sj ’s are the same. Note however that this condition does not require that all the βj ’s and µj ’s are the same. Let βeq and µeq be given equilibrium values of the inverse temperature and chemical potential, and (1 + e−βeq ε0 )−1 0 −βeq (HS −µeq ) −βeq (HS −µeq ) ωSeq = e /Tr(e )= , 0 (1 + eβeq ε0 )−1 the corresponding NESS. As in Subsection 7.6, the affinities (thermodynamic forces) are Xj = βeq − βj and Yj = βj µj − βeq µeq . A simple computation yields the FGR Onsager reciprocity relations ∂Xj ωS+ (Φfgr,k )|X=Y =0 = ∂Xk ωS+ (Φfgr,j )|X=Y =0 , ∂Yj ωS+ (Jfgr,k )|X=Y =0 = ∂Yk ωS+ (Jfgr,i )|X=Y =0 ,

(65)

∂Yj ωS+ (Φfgr,k )|X=Y =0 = ∂Xk ωS+ (Jfgr,i )|X=Y =0 .

We set Lfgr (A, B) =

∞

ωSeq (etKH (A)B) dt,

0

where A and B are the FGR heat or charge flux observables. Explicit computations yield the FGR Kubo formulas ∂Xk ωS+ (Φfgr,j )|X=Y =0 = Lfgr (Φfgr,j , Φfgr,k ), ∂Yk ωS+ (Φfgr,j )|X=Y =0 = Lfgr (Φfgr,j , Jfgr,k ), ∂Xk ωS+ (Jfgr,j )|X=Y =0 = Lfgr (Jfgr,j , Φfgr,k ), ∂Yk ωS+ (Jfgr,j )|X=Y =0 = Lfgr (Jfgr,j , Jfgr,k ).

(66)

8.4 From Microscopic to FGR Thermodynamics At the end of Subsection 4.5 we have briefly discussed the passage from the microscopic to the FGR thermodynamics. We now return to this subject in the context of the SEBB model. The next theorem is a mathematically rigorous version of the heuristic statement that the FGR thermodynamics is the first non-trivial contribution (in λ) to the microscopic thermodynamics.


Theorem 8.2.

57

(i) For any diagonal observable A ∈ OS , lim ωλ+ (A) = ωS+ (A).

λ→0

(ii) For j = 1, · · · , M , lim λ−2 ωλ+ (Φj ) = ωS+ (Φfgr,j ),

lim λ−2 ωλ+ (Jj ) = ωS+ (Jfgr,j ).

λ→0

λ→0

(iii) Let sj ≡ log ρj (ε0 )/(1 − ρj (ε0 )) and define the FGR entropy production by σfgr ≡ 2π

M

−ρj (ε0 ) . 1 − ρj (ε0 )

|fj (ε0 )|2 sj

j=1

Then

lim λ−2 Ep(ωλ+ ) = ωS+ (σfgr ).

λ→0

The proof of this theorem is an integration exercise. We will restrict ourselves to an outline of the proof of Part (i) and several comments. Let A = NS = a∗ (1)a(1). Then ωλ+ (A) = (W− 1, TR W− 1) =

M

e+

λ2

j=1

e−

|fj (r)|2 ρj (r) dr, |F (r)|2

and ωS+ (A) =

M |fj (ε0 )|2 j=1

|f (ε0 )|2

ρj (ε0 ).

Hence, to prove Part (i) we need to show that e+ |fj (r)|2 |fj (ε0 )|2 lim λ2 ρ (r) dr = ρj (ε0 ). j 2 λ→0 |f (ε0 )|2 e− |F (r)| By Assumption (SEBB2), R(r) ≡ Re G(r − io) and π|f (r)|2 = Im G(r − io) are bounded continuous functions. The same is true for ρj (r) by Assumption (SEBB3). Since F (r) = ε0 − r − λ2 R(r) + iλ2 π|f (r)|2 , we have e+ e−

|fj (r)|2 ρj (r) dr = |F (r)|2

e+

e−

|fj (r)|2 ρj (r) dr. (r − ε0 + λ2 R(r))2 + π 2 λ4 |f (r)|4

Using the above-mentioned continuity and boundedness properties it is not hard to show that

58


e+

lim λ2

λ→0

e−

|fj (r)|2 ρj (r) dr |F (r)|2 2

= ρj (ε0 )|fj (ε0 )| lim λ λ→0

e−

= ρj (ε0 )|fj (ε0 )|2 lim λ2 λ→0

=

e+

dr

2

∞

−∞

(r − ε0 +

λ2 R(r))2

+ π 2 λ4 |f (r)|4

dr r2 + π 2 λ4 |f (ε0 )|4

|fj (ε0 )|2 ρj (ε0 ). |f (ε0 )|2

The proofs of Parts (ii) and (iii) are similar. Clearly, under additional regularity assumptions one can get information on the rate of convergence in Parts (i)-(iii). Finally, it is not difficult to show, using the Kubo formulas described in Subsection 7.6 and 8.3, that lim λ−2 Lρ (A, B) = Lfgr (Afgr , Bfgr ), λ→0

where A, B are the microscopic heat or charge flux observables and Afgr , Bfgr are their FGR counterparts.

9 Appendix 9.1 Structural Theorems Proof of Theorem 3.1 Recall that πω (O) is the Banach space dual of Nω . If A ∈ O and A˜ ∈ πω (O) is a weak-∗ accumulation point of the net 1 t πω (τVs (A)) ds, t 0 t ≥ 0, it follows from the asymptotic abelianness in mean that A˜ ∈ πω (O) . Since ω is a factor state we have πω (O) ∩ πω (O) = CI and therefore, for any η ∈ Nω , one has ˜ = ω(A). ˜ η(A) (67) Let µ, ν ∈ Nω and µ+ ∈ Σ+ (µ, τV ). Let tα → ∞ be a net such that tα 1 lim µ ◦ τVs (A) ds = µ+ (A), α tα 0 for all A ∈ O. Passing to a subnet, we may also assume that for all A ∈ O and some ν+ ∈ Σ+ (ν, τV ), tα 1 ν ◦ τVs (A) ds = ν+ (A). lim α tα 0


59

By the Banach-Alaoglu theorem, for any A ∈ O there exists a subnet tγ (A) of the net tα and A# ∈ πω (O) such that, for all η ∈ Nω lim γ

1 tγ (A)

tγ (A)

η(πω (τVs (A))) ds = η(A# ). 0

Hence, µ+ (A) = µ(A# ) and ν+ (A) = ν(A# ). By (67) we also have µ(A# ) = ω(A# ) = ν(A# ) and so µ+ (A) = ν+ (A). We conclude that µ+ = ν+ and that Σ+ (µ, τV ) ⊂ Σ+ (ν, τV ). By symmetry, the reverse inclusion also holds and Σ+ (µ, τV ) = Σ+ (ω, τV ) for all µ ∈ Nω .

Proof of Theorem 3.3 To prove this theorem we use the correspondence between ω-normal states and elements of the standard cone P obtained from ω (see Theorem 4.41 in [Pi]); this is possible since ω is modular by assumption. Note that if Ker LV = {0}, then there is an ω-normal, τV -invariant state η. By Theorem 3.1, Σ+ (ω, τV ) = Σ+ (η, τV ) and obviously Σ+ (η, τV ) = {η}. Two nonzero elements in Ker LV therefore yield the same vector state and are represented by the same vector in the standard cone, i.e., Ker LV ∩ P is a one-dimensional half-line. Recall that any ζ ∈ hω can be uniquely decomposed as ζ = ζ1 − ζ2 + iζ3 − iζ4 , with ζi in P. Since eitLV preserves the standard cone, eitLV ζ = ζ iff eitLV ζi = ζi for all i (i.e., ζi ∈ Ker LV ∩ P for all i). Hence, Ker LV is one-dimensional and Part (i) follows. The proof of Part (ii) is simple. Any NESS η ∈ Σ+ (ω, τV ) can be uniquely decomposed as ηn + ηs where ηn ω and ηs ⊥ ω. Since η is τV -invariant, ηn and ηs are also τV -invariant. Therefore ηn is represented by a vector ζ in Ker LV ∩ P. If Ker LV = {0}, then ηn = 0 and η ⊥ ω. It remains to prove Part (iii). Let ϕ ∈ Ker LV be a separating vector for Mω . Let B ∈ πω (O) be such that Bϕ = 1 and let νB be the vector state associated to Bϕ, νB (·) = (Bϕ, ·Bϕ). For any A ∈ πω (O), 1 t

0

t

1 νB τVs (A) ds = t

t

Bϕ, eisLV πω (A)e−isLV Bϕ ds

0

t 1 −isLV ∗ = e B B ϕ ds, πω (A)ϕ . t 0

60


Hence, by the von Neumann ergodic theorem, 1 t s νB+ (A) ≡ lim νB τV (A) ds = PKer LV B ∗B ϕ, πω (A)ϕ , t→∞ t 0 where PKer LV is the projection on Ker LV . Since ϕ is cyclic for πω (O) , for every n ∈ N we can find a Bn such that ω − νBn < 1/n. The sequence νBn is Cauchy in norm and for all ω+ ∈ Σ+ (ω, τV ), ω+ − νBn + ≤ ω − νBn < 1/n. This implies that the norm limit of νBn is the unique NESS in Σ+ (ω, τV ). Since νBn + ∈ Nω and Nω is a norm closed subset of O∗ , this NESS is ω-normal. 9.2 The Hilbert-Schmidt Condition Proof of Theorem 7.2 1/2

We will prove that T+ − T 1/2 is Hilbert-Schmidt. The proof that (I − T+ )1/2 − (I − T )1/2 is also Hilbert-Schmidt is identical. For an elementary introduction to Hilbert-Schmidt operators (which suffices for the proof below) the reader may consult Section VI.6 in [RS]. By our general assumptions, the functions f (r) and F (r)−1 are bounded and continuous. By the assumption of Theorem 7.2, all the densities ρj (r) are the same and equal to ρ(r). Hence, TR =

M

ρj (r) = ρ(hR ).

j=1

Let pR be the orthogonal projection on the reservoir Hilbert space hR . Since T 1/2 − 1/2 1/2 1/2 1/2 TR = TS , T+ (I−pR ), (I−pR )T+ are obviously Hilbert-Schmidt, it suffices 1/2 1/2 to show that pR T+ pR − TR is a Hilbert-Schmidt operator on the Hilbert space hR . Since 1/2 1/2 1/2 pR T+ pR − TR = −pR W−∗ [W− pR , TR ], 1/2

it suffices to show that K ≡ [W− pR , TR ] is a Hilbert-Schmidt operator on hR . By Theorem 6.2, for g ∈ hR , f (r) e+ ρ(r )1/2 − ρ(r)1/2 ¯ (Kg)(r) = λ2 f (r ) · g(r ) dr . F (r) e− r − r + io Let Kij be an operator on L2 ((e− , e+ ), dr) defined by (Kij h)(r) = λ2

fi (r) F (r)

e+

e−

ρ(r )1/2 − ρ(r)1/2 ¯ fj (r )h(r ) dr . r − r + io


61

To prove that K is Hilbert-Schmidt on hR , it suffices to show that Kij is HilbertSchmidt on L2 ((e− , e+ ), dr) for all i, j. Let h1 , h2 ∈ L2 ((e− , e+ ), dr) be bounded continuous functions. Then e+ ¯ h1 (r)fi (r)g2 (r) (h1 , Kij h2 ) = λ2 dr, (68) F (r) e− where

e+

g2 (r) = lim ↓0

e−

ρ(r )1/2 − ρ(r)1/2 ¯ fj (r )h2 (r ) dr . r − r + i

Using the identity r

1 r − r i = − , − r + i (r − r)2 + 2 (r − r)2 + 2

and the fact that, for r ∈ (e− , e+ ), one has lim ↓0

e+

e−

ρ(r )1/2 − ρ(r)1/2 ¯ fj (r )h2 (r ) dr = π(ρ(r)1/2 − ρ(r)1/2 )f¯j (r)h2 (r) (r − r)2 + 2 = 0,

(see the Lecture [Ja]), we obtain e+ (r − r)(ρ(r )1/2 − ρ(r)1/2 ) ¯ fj (r )h2 (r ) dr . g2 (r) = lim − r)2 + 2 ↓0 e (r − Since fj and h2 are bounded and ρ(r)1/2 is 12 -Hölder continuous, we have e+ (r − r)(ρ(r )1/2 − ρ(r)1/2 ) ¯j (r )h2 (r ) dr sup f (r − r)2 + 2 >0,r∈(e− ,e+ ) e− ≤C

e+

sup r∈(e− ,e+ )

e−

f¯j (r )h2 (r ) dr < ∞. |r − r|1/2

¯ 1 (r)F (r)−1 fi (r) ∈ L1 ((e− , e+ ), dr), we can invoke the domiMoreover, since h nated convergence theorem to rewrite Equ. (68) as (h1 , Kij h2 ) = lim(h1 , Kij, h2 ) ↓0

where Kij, is the integral operator on L2 ((e− , e+ ), dr) with kernel k (r, r ) = λ2

fi (r)f¯j (r ) (r − r)(ρ(r )1/2 − ρ(r)1/2 ) . F (r) (r − r)2 + 2

We denote by · HS the Hilbert-Schmidt norm. Then

(69)

62


Kij, 2HS =

|k (r, r )|2 dr dr .

Since ρ(r)1/2 is α-Hölder continuous for α > 1/2 and F (r)−1 is bounded there exists a constant C such that, for r, r ∈ (e− , e+ ) and > 0, one has the estimate |k (r, r )|2 ≤ C

|fi (r)|2 |fj (r )|2 . |r − r |2(1−α)

Therefore, since 2(1 − α) < 1, we conclude that 2 sup Kij, HS = sup |k (r, r )|2 dr dr < ∞. >0

>0

The Hilbert-Schmidt class of operators on L2 ((e− , e+ ), dr) is a Hilbert space with the inner product (X, Y ) = Tr(X ∗ Y ). Since {Kij, }>0 is a bounded set in this ˜ ij such Hilbert space, there is a sequence n → 0 and a Hilbert-Schmidt operator K that for any Hilbert-Schmidt operator X on L2 ((e− , e+ ), dr), ˜ ij ). lim Tr(X ∗ Kij,n ) = Tr(X ∗ K

n→∞

Taking X = (h1 , ·)h2 , where hi ∈ L2 ((e− , e+ ), dr) are bounded and continuous, ˜ ij h2 ) = (h1 , Kij h2 ). Since the set of such h’s is we derive from (69) that (h1 , K ˜ ij = Kij and so Kij is Hilbert-Schmidt. dense in L2 ((e− , e+ ), dr), K


63

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[Ru3] [Ru4] [Ru5] [Ru6] [Ru7] [RS] [Sp] [Ta] [TM]

[VH1] [VH2] [VH3]

[WW]

Fermi Golden Rule and Open Quantum Systems ´ ¨ Jan Derezinski and Rafał Fruboes Department of Mathematical Methods in Physics, Warsaw University, Ho˙za 74, 00-682, Warsaw, Poland email: [email protected], [email protected]

1

Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 68 1.1 1.2

2

Fermi Golden Rule in an Abstract Setting . . . . . . . . . . . . . . . . . . . . . . . . 71 2.1 2.2 2.3 2.4 2.5 2.6 2.7

3

Notation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . Level Shift Operator . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . LSO for C0∗ -Dynamics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . LSO for W ∗ -Dynamics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . LSO in Hilbert Spaces . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . The Choice of the Projection P . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . Three Kinds of the Fermi Golden Rule . . . . . . . . . . . . . . . . . . . . . . . .

71 72 73 74 74 75 75

Weak Coupling Limit . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 77 3.1 3.2 3.3 3.4 3.5 3.6

4

Fermi Golden Rule and Level Shift Operator in an Abstract Setting . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 68 Applications of the Fermi Golden Rule to Open Quantum Systems 69

Stationary and Time-Dependent Weak Coupling Limit . . . . . . . . . . . Proof of the Stationary Weak Coupling Limit . . . . . . . . . . . . . . . . . . Spectral Averaging . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . Second Order Asymptotics of Evolution with the First Order Term . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . Proof of Time Dependent Weak Coupling Limit . . . . . . . . . . . . . . . . Proof of the Coincidence of Mst and Mdyn with the LSO . . . . . . . .

77 80 83 85 87 88

Completely Positive Semigroups . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 88 4.1 4.2 4.3 4.4 4.5

Completely Positive Maps . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . Stinespring Representation of a Completely Positive Map . . . . . . . . Completely Positive Semigroups . . . . . . . . . . . . . . . . . . . . . . . . . . . . . Standard Detailed Balance Condition . . . . . . . . . . . . . . . . . . . . . . . . . Detailed Balance Condition in the Sense of Alicki-FrigerioGorini-Kossakowski-Verri . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .

89 89 90 91 93

68

5

Jan Dereziński and Rafał Früboes

Small Quantum System Interacting with Reservoir . . . . . . . . . . . . . . . . 93 5.1 5.2 5.3 5.4

6

6.4 6.5 6.6

LSO for the Reduced Dynamics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 97 LSO for the Liouvillean . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 99 Relationship Between the Davies Generator and the LSO for the Liouvillean in Thermal Case. . . . . . . . . . . . . . . . . . . . . . . . . . . 100 Explicit Formula for the Davies Generator . . . . . . . . . . . . . . . . . . . . . 103 Explicit Formulas for LSO for the Liouvillean . . . . . . . . . . . . . . . . . . 104 Identities Using the Fibered Representation . . . . . . . . . . . . . . . . . . . . 106

Fermi Golden Rule for a Composite Reservoir . . . . . . . . . . . . . . . . . . . . 108 7.1 7.2 7.3 7.4

A

94 95 95 96

Two Applications of the Fermi Golden Rule to Open Quantum Systems . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 97 6.1 6.2 6.3

7

W ∗ -Algebras . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . Algebraic Description . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . Semistandard Representation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . Standard Representation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .

LSO for a Sum of Perturbations . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 108 Multiple Reservoirs . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 109 LSO for the Reduced Dynamics in the Case of a Composite Reservoir . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 110 LSO for the Liovillean in the Case of a Composite Reservoir . . . . . 111

Appendix – One-Parameter Semigroups . . . . . . . . . . . . . . . . . . . . . . . . . 112

References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 115

1 Introduction These lecture notes are an expanded version of the lectures given by the first author in the summer school ”Open Quantum Systems” held in Grenoble, June 16—July 4, 2003. We are grateful to Stéphane Attal, Alain Joye, and Claude-Alain Pillet for their hospitality and invitation to speak. Acknowledgments. The research of both authors was partly supported by the EU Postdoctoral Training Program HPRN-CT-2002-0277 and the Polish grants SPUB127 and 2 P03A 027 25. A part of this work was done during a visit of the first author to University of Montreal and to the Schrödinger Institute in Vienna. We acknowledge useful conversations with H. Spohn, C. A. Pillet, W. A. Majewski, and especially with V. Jakˇsić. 1.1 Fermi Golden Rule and Level Shift Operator in an Abstract Setting We will use the name “the Fermi Golden Rule” to describe the well-known second order perturbative formula for the shift of eigenvalues of a family of operators Lλ = L0 + λQ. Historically, the Fermi Golden Rule can be traced back to the early years of Quantum Mechanics, and in particular to the famous paper by Dirac [Di]. Two

Fermi Golden Rule and Open Quantum Systems

69

“Golden Rules” describing the second order calculations for scattering amplitudes can be found in the Fermi lecture notes [Fe] on pages 142 and 148. In its traditional form the Fermi Golden Rule is applied to Hamiltonians of quantum systems – self-adjoint operators on a Hilbert space. A nonzero imaginary shift of an eigenvalue of L0 indicates that the eigenvalue is unstable and that it has turned into a resonance under the influence of the perturbation λQ. In our lectures we shall use the term Fermi Golden Rule in a slightly more general context, not restricted to Hilbert spaces. More precisely, we shall be interested in the case when Lλ is a generator of a 1-parameter group of isometries on a Banach space. For example, Lλ could be an anti-self-adjoint operator on a Hilbert space or the generator of a group of ∗-automorphisms of a W ∗ -algebra. These two special cases will be of particular importance for us. Note that the spectrum of the generator of a group of isometries is purely imaginary. The shift computed by the Fermi Golden Rule may have a negative real part and this indicates that the eigenvalue has turned into a resonance. Hence, our convention differs from the traditional one by the factor of i. In these lecture notes, we shall discuss several mathematically rigorous versions of the Fermi Golden Rule. In all of them, the central role is played by a certain operator that we call the Level Shift Operator (LSO). This operator will encode the second order shift of eigenvalues of Lλ under the influence of the perturbation. To define the LSO for Lλ = L0 + λQ, we need to specify the projection P commuting with L0 (typically, the projection onto the point spectrum of L0 ) and a perturbation Q. For the most part, we shall assume that PQP = 0, which guarantees the absence of the first order shift of the eigenvalues. Given the datum (P, L0 , Q), we shall define the LSO as a certain operator on the range of the projection P. We shall describe several rigorous applications of the LSO for (P, L0 , Q). One of them is the “weak coupling limit”, called also the “van Hove limit”. (We will not, however, use the latter name, since it often appears in a different meaning in statistical physics, denoting a special form of the thermodynamical limit). The time-dependent form of the weak coupling limit says that the reduced and rescaled 2 2 dynamics e−tL0 /λ PetLλ /λ P converges to the semigroup generated by the LSO. The time dependent weak coupling limit in its abstract form was proven by Davies [Da1, Da2, Da3]. In our lectures we give a detailed exposition of his results. We describe also the so-called “stationary weak coupling limit”, based on the recent work [DF2]. The stationary weak coupling limit says that appropriately rescaled and reduced resolvent of Lλ converges to the resolvent of the LSO. The LSO has a number of other important applications. It can be used to describe approximate location and multiplicities of eigenvalues and resonances of Lλ for small nonzero λ. It also gives an upper bound on the number of eigenvalues of Lλ for small nonzero λ. 1.2 Applications of the Fermi Golden Rule to Open Quantum Systems In these lectures, by an open quantum system we shall mean a “small” quantum system S interacting with a large “environment” or “reservoir” R. The small quantum

70


system is described by a finite dimensional Hilbert space K and a Hamiltonian K. The reservoir is described by a W ∗ -dynamical system (M, τ ) and a reference state ωR (for a discussion of reference states see the lecture [AJPP]). We shall assume that ωR is normal and τR -invariant. If ωR is a (τR , β)-KMS state, then we say that that the reservoir at inverse temperature β and that the open quantum system is thermal. Another important special case is when R has additional structure, namely consists of n independent parts R1 , · · · , Rn , which are interpreted as sub-reservoirs. If the reference state of the sub-reservoir Rj is βj -KMS (for j = 1, · · · , n), then we shall call the corresponding open quantum system multi-thermal. In the literature one can find at least two distinct important applications of the Fermi Golden Rule to the study of open quantum systems. In the first application one considers the weak coupling limit for the dynamics in the Heisenberg picture reduced to the small system. This limit turns out to be an irreversible Markovian dynamics—a completely positive semigroup preserving the identity acting on the observables of the small system S (n × n matrices). The generator of this semigroup is given by the LSO for the generator of the dynamics. We will denote it by M . The weak coupling limit and the derivation of the resulting irreversible Markovian dynamics goes back to the work of Pauli, Wigner-Weisskopf and van Hove [WW, VH1, VH2, VH3] see also [KTH, Haa]. In the mathematical literature it was studied in the well known papers of Davies [Da1, Da2, Da3], see also [LeSp, AL]. Therefore, the operator M is sometimes called the Davies generator in the Heisenberg picture. One can also look at the dynamics in the Schrödinger picture (on the space of density matrices). In the weak coupling limit one then obtains a completely positive semigroup preserving the trace. It is generated by the adjoint of M , denoted by M ∗ , which is sometimes called the Davies generator in the Schrödinger picture. The second application of the Fermi Golden Rule to the study of open quantum systems is relatively recent. It has appeared in papers on the so-called return to equilibrium [JP1, DJ1, DJ2, BFS2, M]. The main goal of these papers is to show that certain W ∗ -dynamics describing open quantum systems has only one stationary normal state or no stationary normal states at all. This problem can be reformulated into a question about the point spectrum of the so-called Liouvillean—the generator of the natural unitary implementation of the dynamics. To study this problem, it is convenient to introduce the LSO for the Liouvillean. We shall denote it by iΓ . It is an operator acting on Hilbert-Schmidt operators for the system S—again n × n matrices. The use of iΓ in the spectral theory hinges on analytic techniques (Mourre theory, complex deformations), which we shall not describe in our lectures. We shall take it for granted that under suitable technical conditions such applications are possible and we will focus on the algebraic properties of M , iΓ and M ∗ . To the best of our knowledge, some of these properties have not been discussed previously in the literature. In Theorem 6.7 we give a simple characterization of the kernel of the imaginary part the operator Γ . This characterization implies that Γ has no nontrivial real


71

eigenvalues in a generic nonthermal case. In [DJ2], this result was proven in the context of Pauli-Fierz systems and was used to show the absence of normal stationary states in a generic multithermal case. In our lectures we generalize the result of [DJ2] to a more general setting. The characterization of the kernel of the imaginary part of Γ in the thermal case is given in Theorem 6.8. It implies that generically this kernel consists only of multiples of the square root of the Gibbs density matrix for the small system. In [DJ2], this result was proven in the more restrictive context of Pauli-Fierz systems and was used to show the return to equilibrium in the generic thermal case. A similar result was obtained earlier by Spohn [Sp]. The operators M , iΓ and M ∗ act on the same vector space (the space of n × n matrices) and have similar forms. Naively, one may expect that iΓ interpolates in some sense between M and M ∗ . Although this expectation is correct, its full description involves some advanced algebraic tools (the so-called noncommutative Lp -spaces associated to a von Neumann algebra), and for reasons of space we will not discuss it in these lecture notes (see [DJ4, JP6]). In the thermal case, the relation between the operators M , iΓ and M ∗ is considerably simpler—they are mutually similar and in particular have the same spectrum. This result has been recently proven in [DJ3] and we will describe it in detail in our lectures. The similarity of iΓ and M in the thermal case is closely related to the Detailed Balance Condition for M . In the literature one can find a number of different definitions of the Detailed Balance Condition applicable to irreversible quantum dynamics. In these lecture notes we shall propose another one and we will compare it with the definition due to Alicki [A] and Frigerio-Gorini-Kossakowski-Verri [FGKV]. For reason of space we have omitted many important topics in our lectures— they are treated in the review [DJ4], which is a continuation of these lecture notes. Some additional information about the weak coupling limit and the Davies generator can be also found in the lecture notes [AJPP].

2 Fermi Golden Rule in an Abstract Setting 2.1 Notation Let L be an operator on a Banach space X . spL, spess L, spp L will denote the spectrum, the essential spectrum and the point spectrum (the set of eigenvalues) of the operator L. If e is an isolated point in spL, then 1e (L) will denote the spectral projection of L onto e given by the usual contour integral. Sometimes we can also define 1e (L) if e is not an isolated point in the spectrum. This is well known if L is a normal operator on a Hilbert space. The definition of 1e (L) for some other classes of operators is discussed in Appendix, see (69), (70). Let us now assume that L is a self-adjoint operator on a Hilbert space. Let A, B be bounded operators. Suppose that p ∈ R. We define A(p ± i0 − L)−1 B := lim A(p ± i − L)−1 B, 0

(1)

72


provided that the right hand side of (1) exists. We will say that A(p ± i0 − L)−1 B exists if the limit in (1) exists. The principal value of (p − L)−1 AP(p − L)−1 B :=

1 A(p + i0 − L)−1 B + A(p − i0 − L)−1 B 2

and the delta function of p − L Aδ(p − L)B :=

i A(p + i0 − L)−1 B − A(p − i0 − L)−1 B 2π

are then well defined. B(X ) denotes the algebra of bounded operators on X . If X is a Hilbert space, then B 1 (X ) denotes the space of trace class operators and B 2 (X ) the space of Hilbert-Schmidt operators on X . By a density matrix on X we mean ρ ∈ B1 (X ) such that ρ ≥ 0 and Trρ = 1. We say that ρ is nondegenerate if Kerρ = {0}. For more background material useful in our lectures we refer the reader to Appendix. 2.2 Level Shift Operator In this subsection we introduce the definition of the Level Shift Operator. First we describe the basic setup needed to make this definition. Assumption 2.1 We assume that X is a Banach space, P is projection of norm 1 on X and etL0 is a 1-parameter C0 - group of isometries commuting with P. ! := 1 − P. Clearly, E is the generator of a 1We set E := L0 and P RanP generates a 1-parameter group parameter group of isometries on RanP, and L0 Ran! P ! of isometries on RanP. ! instead of L0 . For instance, in (2) ((ie + Later on, we will often write L0 P P Ran! ˜ This is ! −1 will denote the inverse of (ie + ξ)1 − L0 restricted to RanP. ! − L0 P) ξ)P a slight abuse of notation, which we will make often without a comment. Most of the time we will also assume that Assumption 2.2 P is finite dimensional. Under Assumption 2.1 and 2.2, the operator E is diagonalizable and we can write its spectral decomposition: E= ie1ie (E). ie∈spE

Note that 1ie (E) are projections of norm one. In the remaining assumptions we impose our conditions on the perturbation:


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Assumption 2.3 We suppose that Q is an operator with DomQ ⊃ DomL0 and, for |λ| < λ0 , Lλ := L0 + λQ is the generator of a 1-parameter C0 -semigroup of contractions. ! ! are well defined. Assumption 2.3 implies that PQP and PQP Assumption 2.4 PQP = 0. The above assumption is needed to guarantee that the first nontrivial contribution for the shift of eigenvalues of Lλ is 2nd order in λ. ! ! are It is also useful to note that if Assumption 2.2 holds, then PQP and PQP ! ! bounded. Note also that in the definition of LSO only the terms PQP and PQP will ! P ! will be irrelevant. play a role and the term PQ Assumption 2.5 We assume that for all ie ∈ spE there exists ! − L0 P) ! −1 Q1ie (E) 1ie (E)Q((ie + 0)P ! − L0 P) ! −1 Q1ie (E) := lim 1ie (E)Q((ie + ξ)P

(2)

ξ0

Under Assumptions 2.1, 2.2, 2.3, 2.4 and 2.5 we set ! − L0 P) ! −1 Q1ie (E) M := 1ie (E)Q((ie + 0)P

(3)

ie∈spE

and call it the Level Shift Operator (LSO) associated to the triple (P, L0 , Q). It is instructive to give time-dependent formulas for the LSO: ∞ M = lim 1ie (E) 0 e−ξs QQ(s)1ie (E)ds ξ0 ie∈spE

= lim

ξ0 ie∈spE

1ie (E)

∞ 0

e−ξs Q(−s/2)Q(s/2)1ie (E)ds,

where Q(t) := etL0 Qe−tL0 . 2.3 LSO for C0∗ -Dynamics In the previous subsection we assumed that Lλ is a generator of a C0 -semigroup. In one of our applications, however, we will deal with another type of semigroups, the so-called C0∗ -semigroups (see Appendix for definitions and a discussion). In this case, we will need to replace Assumptions 2.1 and 2.3 by their “dual versions”, which we state below: Assumption 2.1* We assume that Y is a Banach space and X is its dual, that is X = Y ∗ , P is a w* continuous projection of norm 1 on X and etL0 is a 1-parameter C0∗ - group of isometries commuting with P. Assumption 2.3* We suppose that Q is an operator with DomQ ⊃ DomL0 and, for |λ| < λ0 , Lλ := L0 + λQ is the generator of a 1-parameter C0∗ -semigroup of contractions.

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2.4 LSO for W ∗ -Dynamics The formalism of the Level Shift Operator will be applied to open quantum systems in two distinct situations. In the first application, the Banach space X is a W ∗ -algebra, P is a normal conditional expectation and etL0 is a W ∗ -dynamics. Note that W ∗ -algebras are usually not reflexive and W ∗ -dynamics are usually not C0 -groups. However, W ∗ -algebras are dual Banach spaces and W ∗ -dynamics are C0∗ -groups. The perturbation has the form i[V, ·] with V being a self-adjoint element of the W ∗ -algebra. Therefore, etLλ will be a W ∗ -dynamics for all real λ – again a C0∗ group. 2.5 LSO in Hilbert Spaces In our second application, X is a Hilbert space. Hilbert spaces are reflexive, therefore we do not need to distinguish between C0 and C0∗ -groups. All strongly continuous groups of isometries on a Hilbert space are unitary groups. Therefore, the operator L0 has to be anti-self-adjoint (that means L0 = iL0 , where L0 is self-adjoint). All projections of norm one on a Hilbert space are orthogonal. Therefore, the distinguished projection has to be orthogonal. In our applications to open quantum systems etLλ is a unitary dynamics. This means in particular that Q has the form Q = iQ, where Q is hermitian. In the case of a Hilbert space the LSO will be denoted iΓ . Thus we will isolate the imaginary unit “i”, which is consistent with the usual conventions for operators in Hilbert spaces, and also with the convention that was adopted in [DJ2]. Remark 2.1. In [DJ2] we used a formalism similar to that of Subsection 2.2 in the context of a Hilbert space. Note, however, that the terminology that was adopted there is not completely consistent with the terminology used in these lectures. In [DJ2] we considered a Hilbert space X , an orthogonal projection P , and self-adjoint operators L0 , Q. If Γ is the LSO for the triple (P, L0 , Q) according to [DJ2], then iΓ is the LSO for (P, iL0 , iQ) according to the present definition. Let us quote the following easy fact valid in the case of a Hilbert space. Theorem 2.1. Suppose that X is a Hilbert space, Assumptions 2.1, 2.2, 2.3 and 2.5 hold and Q is self-adjoint. Then eitΓ is contractive for t > 0. Proof. We use the notation E = iE, L0 = iL, Q = iQ. We have 1 (Γ − Γ ∗ ) = − 1e (E)Qδ(e − L0 )Q1e (E) ≤ 0 2i e∈spE

Therefore, iΓ is a dissipative operator and eitΓ is contractive for t > 0. 2


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Note that in Theorem 3.4 we will show that the LSO is the generator of a contractive semigroup also in a more general situation, when X is a Banach space. The proof of this fact will be however more complicated and will require some additional technical assumptions. 2.6 The Choice of the Projection P In typical application of the LSO, the operators L0 and Q are given and our goal is to study the operator (4) Lλ := L0 + λQ. More precisely, we want to know what happens with its eigenvalues when we switch on the perturbation. Therefore, it is natural to choose the projection P as “the projection onto the point spectrum of L0 ”, that is P= 1ie (L0 ), (5) e∈R

provided that (5) is well defined. More generally, if we were interested only about what happens around some eigenvalues {ie1 , . . . , ien } ⊂ spp L0 , then we could use the LSO defined with the projection n 1iej (L0 ). (6) P= j=1

Clearly, if X is a Hilbert space and L0 is anti-self-adjoint, then 1ie (L0 ) are well defined for all e ∈ R. Moreover, both (5) and (6) are projections of norm one commuting with L0 , and hence they satisfy Assumption 2.1. There is no guarantee that the spectral projections 1ie (L0 ) are well defined in the more general case when L0 is the generator of a group of isometries on a Banach space. If they are well defined, then they have norm one, however, we seem to have no guarantee that their sums have norm one. In Appendix we discuss the problem of defining spectral projections onto eigenvalues in this more general case. Note, however, that in the situation considered by us later, we will have no such problems. In fact, P will be always given by (5) and will always have norm one. If 1ie (L0 ) is well defined for all e ∈ R and we take P defined by (5), then P will be determined by the operator L0 itself. We will speak about “the LSO for Lλ ”, if we have this projection in mind. 2.7 Three Kinds of the Fermi Golden Rule Suppose that Assumptions 2.1, 2.2, 2.3, 2.4 and 2.5, or 2.1*, 2.2, 2.3*, 2.4 and 2.5 are satisfied. Let P be given by (5) and M be the LSO for (P, L0 , Q). Our main object of interest is the operator Lλ .

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The assumption 2.4 (PQP = 0) guarantees that there are no first order effects of the perturbation. The operator M describes what happens with the eigenvalues of L0 under the influence of the perturbation λQ at the second order of λ. Following the tradition of quantum physics, we will use the name “the Fermi Golden Rule” to describe the second order effects of the perturbation. The Fermi Golden Rule can be made rigorous in many ways under various technical assumptions. We can distinguish at least three varieties of the rigorous Fermi Golden Rule: – Analytic Fermi Golden Rule: E + λ2 M predicts the approximate location (up to o(λ2 )) and the multiplicity of the resonances and eigenvalues of Lλ in a neighborhood of spp L0 for small λ. The Analytic Fermi Golden Rule is valid under some analyticity assumptions on Lλ . It is well known and follows essentially by the standard perturbation theory for isolated eigenvalues ( [Ka,RS4], see also [DF1]). The perturbation arguments are applied not to Lλ directly, but to the analytically deformed Lλ . More or less explicitly, this idea was applied to Liouvilleans describing open quantum systems [JP1, JP2, BFS1, BFS2]. One can also apply it to the W ∗ -dynamics of open quantum systems [JP4, JP5]. The stationary weak coupling (or van Hove) limit of [DF2], described in Theorem 3.1 and 3.4, can be viewed as an infinitesimal version of the Analytic Fermi Golden Rule. – Spectral Fermi Golden Rule: The intersection of the spectrum of E + λ2 M with the imaginary line predicts possible location of eigenvalues of Lλ for small nonzero λ. It also gives an upper bound on their multiplicity. Note that if the Analytic Fermi Golden Rule is true, then so is the Spectral Fermi Golden Rule. However, to prove the Analytic Fermi Golden Rule we need strong analytic assumption, whereas the Spectral Fermi Golden Rule can be shown under much weaker conditions. Roughly speaking, these assumptions should allow us to apply the so-called positive commutator method. The Spectral Fermi Golden Rule is stated in Theorem 6.7 of [DJ2], which is proven in [DJ1]. Strictly speaking, the analysis of [DJ1] and [DJ2] is restricted to Pauli-Fierz operators, but it is easy to see that their arguments extend to much larger classes of operators. To illustrate the usefulness of the Spectral Fermi Golden Rule, suppose that X is a Hilbert space, Lλ = iLλ with Lλ self-adjoint and iΓ is the LSO. Then the Spectral Fermi Golden Rule implies the bound dim Ran1p (Lλ ) ≤ dim KerΓ I , 1 (Γ − Γ ∗ ). Bounds of this type were used in various papers where Γ I := 2i related to the Return to Equilibrium [JP1, JP2, DJ2, BFS2, M]. 2 – Dynamical Fermi Golden Rule. The operator et(E+λ M ) describes approximately the reduced dynamics PetLλ P for small λ. The Dynamical Fermi Golden Rule was rigorously expressed in the form of the weak coupling by Davies [Da1, Da2, Da3, LeSp]. Davies showed that under


77

some weak assumptions we have lim e−tE/λ PetLλ /λ P = etM . 2

2

λ→0

We describe his result in Theorems 3.2 and 3.4.

3 Weak Coupling Limit 3.1 Stationary and Time-Dependent Weak Coupling Limit In this section we describe in an abstract setting the weak coupling limit. We will show that, under some conditions, the dynamics restricted to an appropriate subspace, rescaled and renormalized by the free dynamics, converges to the dynamics generated by the LSO. We will give two versions of the weak coupling limit: the time dependent and the stationary one. The time-dependent version is well known and in its rigorous form is due to Davies [Da1, Da2, Da3]. Our exposition is based on [Da3]. The stationary weak coupling limit describes the same phenomenon on the level of the resolvent. Our exposition is based on recent work [DF2]. Formally, one can pass from the time-dependent to stationary weak coupling limit by the Laplace transformation. However, one can argue that the assumptions needed to prove the stationary weak coupling limit are sometimes easier to verify. In fact, they involve the existence of certain matrix elements of the resolvent (a kind of the “Limiting Absorption Principle”) only at the spectrum of E, a discrete subset of the imaginary line. This is often possible to show by positive commutator methods. Throughout the section we suppose that most of the assumptions of Subsection 2.2 are satisfied. We will, however, list explicitely the assumptions that we need for each particular result. The first theorem describes the stationary weak coupling limit. Theorem 3.1. Suppose that Assumptions 2.1, 2.2, 2.3 and 2.4, or 2.1*, 2.2, 2.3* and 2.4 are true. We also assume the following conditions: ! ! λ P. 1) For ie ∈ spE, ξ > 0, we have ie + ξ ∈ spPL 2) There exists an operator Mst on RanP such that, for any ξ > 0, −1 ! − PL ! λP ! Mst := lim 1ie (E)Q (ie + λ2 ξ)P Q1ie (E). (7) ie∈spE

λ→0

(Note that a priori the right hand side of (7) may depend on ξ; we assume that it does not). 3) For any ie, ie ∈ spE, e = e and ξ > 0, −1 ! − PL ! λP ! lim λ1ie (E)Q (ie + λ2 ξ)P Q1ie (E) = 0, λ→0 −1 ! − PL ! λP ! lim λ1ie (E)Q (ie + λ2 ξ)P Q1ie (E) = 0. λ→0

78


Then the following holds: 1. etMst is a contractive semigroup. 2. For any ξ > 0 −1 lim 1ie (E) ξ − λ−2 (Lλ − ie) P = (ξP − Mst )−1 . ie∈spE

λ→0

3. For any f ∈ C0 ([0, ∞[), ∞ 2 2 lim f (t)e−tE/λ PetLλ /λ Pdt = λ→0

0

∞

f (t)etMst dt.

(8)

0

Next we describe the time-dependent version of the weak coupling limit for C0 groups. Theorem 3.2. Suppose that Assumptions 2.1, 2.3 and 2.4 are true. We make also the following assumptions: ! and PQP ! ! λP ! 1) PQP are bounded. (Note that this assumption guarantees that PL ! is the generator of a C0 -semigroup on RanP). 2) Set

λ−2 t

Kλ (t) :=

e−sE PQes!PLλ!P QPds.

0

We suppose that for all t0 > 0, there exists c such that sup Kλ (t) ≤ c.

sup

|λ| 0, lim sup e−Et/λ PetLλ /λ Py − etMdyn y = 0. 2

λ→0 0≤t≤t0

2

(9)


79

One of possible C0∗ -versions of the above theorem is given below. Theorem 3.2* Suppose that Assumptions 2.1*, 2.3* and 2.4 are true. We make also the following assumptions: 0) etE is a C0 -group. (We already know that it is a C0∗ -group). ! and PQP ! 1) PQP are w* continuous. (Note that this assumption guarantees that ! ! ! PLλ P is a generator of a C0∗ -semigroup on RanP). 2) In the sense of a w* integral [BR1] we set λ−2 t e−sE PQes!PLλ!P QPds. (10) Kλ (t) := 0

We suppose that for all t0 > 0, there exists c such that sup Kλ (t) ≤ c.

sup

|λ| 0, there exists c such that sup Kλ (t) ≤ c.

sup

|λ| 0, lim sup e−Et/λ PetLλ /λ P − etMdyn = 0. 2

2

λ→0 0≤t≤t0

(11)

Note that if there exists an operator Mst satisfying (8), and an operator Mdyn satisfying (11), then they clearly coincide. In our last theorem of this section we will describe a connection between Mst , Mdyn and the LSO. Theorem 3.4. Suppose that Assumptions 2.1, 2.2, 2.3 and 2.4, or 2.1*, 2.2, 2.3* and 2.4 are true. Suppose also that the following conditions hold: ∞ 1) 0 sup PQes!PLλ!P QPds < ∞. |λ|≤λ0

2) For any s > 0, lim PQes!PLλ!P QP = PQes!PL0 QP. λ→0

Then 1. Assumption 2.5 holds, and hence the LSO for (P, L0 , Q), defined in (3) and denoted M , exists. 2. etM is a contractive semigroup. 3. The assumptions of Theorem 3.1 hold and M = Mst , consequently, for any ξ>0 −1 1ie (E) ξ − λ−2 (Lλ − ie) P = (ξP − M )−1 . lim λ→0

ie∈spE

4. The assumptions of Theorem 3.3 hold and M = Mdyn , consequently lim sup e−Et/λ PetLλ /λ P − etM = 0. 2

2

λ→0 0≤t≤t0

3.2 Proof of the Stationary Weak Coupling Limit Proof of Theorem 3.1. We follow [DF2]. Let ie ∈ spE. Set Gλ (ξ, ie) := ξP + λ−2 (ieP − E) −1 ! − PL ! λP ! −PQ (λ2 ξ + ie)P QP. By the so-called Feshbach formula (see e.g. [DJ1, BFS1]), for ξ > 0 we have −1 Gλ (ξ, ie)−1 = P ξ + λ−2 (ie − Lλ ) P This and the dissipativity of Lλ implies the bound


Gλ (ξ, ie)−1 ≤ ξ −1 .

81

(12)

Write for shortness G instead of Gλ (ξ, ie). For ie ∈ spE, set Pe := 1ie (E), Pe := P − 1ie (E). Decompose G = Gdiag + Goff into its diagonal and off-diagonal part: Pe GPe , Gdiag := ie ∈spE

Goff :=

ie ∈spE

Pe GPe =

ie ∈spE

Pe GPe .

First we would like to show that for ξ > 0 and small enough λ, Gdiag is invertible. By an application of the Neumann series, Pe Gdiag is invertible on RanPe , and we have the bound 2 (13) Pe G−1 diag ≤ cλ . It is more complicated to prove that Pe Gdiag is inverible on RanPe . We fix ξ > 0. We know that G is invertible and G−1 ≤ ξ −1 . Hence we can write Gdiag G−1 = 1 − Goff G−1 . Therefore

Pe Gdiag G−1 = Pe − Pe Goff Pe G−1 , Pe Gdiag G−1 = Pe − Pe Goff G−1 .

(14)

The latter identity can be for small enough λ transformed into −1 −1 Pe G−1 = G−1 . diag Pe − Gdiag Pe Goff G

(15)

We insert (15) into the first identity of (14) to obtain −1 −1 . Pe Gdiag G−1 = Pe − Pe Goff Pe G−1 diag + Pe Goff Pe Gdiag Goff G

(16)

We multiply (16) from the right by Pe to get −1 Pe Gdiag Pe G−1 Pe = Pe + Pe Goff Pe G−1 Pe . diag Goff G

(17)

lim λGoff = 0,

(18)

Now, using λ→0

(12) and (13) we obtain −1 lim Pe Goff Pe G−1 Pe = 0. diag Goff G

λ→0

Thus, for small enough λ,

82


Pe Gdiag B1 = Pe , where

−1 −1 B1 := Pe G−1 Pe Pe + Pe Goff Pe G−1 G G P . off e diag

Similarly, for small enough λ, we find B2 such that B2 Pe Gdiag = Pe . This implies that Pe Gdiag is invertible on RanPe . Next, we can write −1 −1 −1 −1 −1 . G−1 = G−1 diag − Gdiag Goff Gdiag + Gdiag Goff Gdiag Goff G

Hence, −1 −1 −1 Pe G−1 = Pe G−1 . diag 1 − Goff Pe Gdiag + Goff Pe Gdiag Goff G

(19)

Therefore, for a fixed ξ, by (12), (13) and (18) we see that as λ → 0 we have −1 −1 → 0. −Goff Pe G−1 diag + Goff Pe Gdiag Goff G

Therefore, for small enough λ, we can invert the expression in the bracket of (19). Consequently, −1 −1 −1 −1 Pe (G−1 ) = Pe G−1 1 − Goff Pe G−1 diag − G diag + Goff Pe Gdiag Goff G −1 −1 . × Goff Pe G−1 diag − Goff Pe Gdiag Goff G (20) Therefore, for a fixed ξ, by (12), (13) and (18) we see that, as λ → 0, we have −1 Pe (G−1 ) → 0. diag − G

(21)

Hence, (12) and (21) imply that Pe G−1 diag is uniformly bounded as λ → 0. We know that (22) Pe Gdiag → Pe ξ − Pe Mst . Therefore, ξPe − Pe Mst is invertible on RanPe and −1 . Pe G−1 diag → (Pe ξ − Pe Mst )

Using again (21), we see that Pe G−1 → (Pe ξ − Pe Mst )−1 . Summing up (23) over e, we obtain Pe Gλ (ξ, ie)−1 → (ξP − Mst )−1 , ie∈spE

(23)

(24)


83

which ends the proof of 2. Let us now prove 1. We have

∞

Pe Gλ (ξ, ie)−1 =

ie∈spE

−2

e−t(ξ+λ

ie)

2

Pe etLλ /λ Pdt

ie∈spE 0

=

∞

e

(25)

−tξ −tE/λ2

e

Pe

tLλ /λ2

Pdt

0

Clearly, e−tE/λ PetLλ /λ P ≤ 1. Therefore, " " " " " " −1 " " Pe Gλ (ξ, ie) " ≤ ξ −1 . " "ie∈spE " 2

2

Hence, by (24),

" " "(ξP − Mst )−1 " ≤ ξ −1 ,

which proves 1. Let f ∈ C0 ([0, ∞[) and δ > 0. By the Stone-Weierstrass Theorem, we can find a finite linear combination of functions of the form e−tξ for ξ > 0, denoted g, such that etδ f − g∞ < . Set Aλ (t) := e−tE/λ PetLλ /λ P, 2

2

A0 (t) := etMdyn .

Note that Aλ (t) ≤ 1 and A0 (t) ≤ 1. Now f (t)(Aλ (t) − A0 (t))dt ≤ e−δt g(t)(Aλ (t) − A0 (t))dt + (f (t) − e−δt g(t))Aλ (t)dt + (f (t) − e−δt g(t))A0 (t)dt. By 2. and by the Laplace transformation, the first term ∞ on the right hand side goes to 0 as λ → 0. The last two terms are estimated by 0 e−δt dt, which can be made arbitrarily small by choosing small. This proves 3. 2

3.3 Spectral Averaging Before we present the time-dependent version of the weak coupling limit, we discuss the spectral averaging of operators, following [Da3]. In this subsection, Y is an arbitrary Banach space and etE is a 1-parameter C0 group of isometries on Y. For K ∈ B(Y) we define

K := s− lim t t→∞

provided that the right hand side exists.

−1

0

t

esE Ke−sE ds,

(26)

84


Theorem 3.5. Suppose that K exists. Then, for any t0 > 0, y ∈ Y, lim sup e−tE/λ et(E+λK)/λ y − etK y = 0.

λ→0 0≤t≤t0

Proof. Consider the space C([0, t0 ], Y) with the supremum norm. Set K(t) = etE/λ Ke−tE/λ . For f ∈ C([0, t0 ], Y), define Bλ f (t) :=

t

K(s/λ)f (s)ds, 0

B0 f (t) := K

t

f (s)ds. 0

Clearly, B0 and Bλ are linear operators on C([0, t0 ], Y) satisfying Bλ ≤ t0 K.

(27)

lim Bλ f = B0 f.

(28)

Moreover λ→0

To prove (28), by (27) it suffices to assume that f ∈ C 1 ([0, t0 ], Y). Now t s t Bλ f (t) = 0 K(s/λ)ds f (t) − 0 0 ds1 K(s1 /λ) f (s)ds t → tK f (t) − 0 sK f (s)ds = B0 f (t). We easily get Bλn ≤

tn0 tn Kn , B0n ≤ 0 Kn . n! n!

(29)

Let y ∈ Y. Set yλ (t) := e−tE/λ et(E+λK)/λ y. Note that yλ (t) = y + Bλ yλ (t), y0 (t) = y + B0 y0 (t). Treating y as an element of C([0, t0 ], Y) – the constant function equal to y we can write ∞ ∞ Bλn y, (1 − B0 )−1 y = B0n y, (1 − Bλ )−1 y = n=0

n=0

where both Neumann series are absolutely convergent. Therefore, in the sense of the convergence in in C([0, t0 ], Y), we get yλ =

∞ n=0

2

Bλn y →

∞ n=0

B0n y = y0 .


85

Theorem 3.6. Let Y be finite dimesional. Then K exists for any K ∈ B(Y) and K =

1ie (E)K1ie (E) = lim t−1 t→∞

ie∈spE

t 0

esE Ke−sE ds,

lim sup e−tE/λ et(E+λK)/λ − etK = 0.

λ→0 0≤t≤t0

Proof. In finite dimension we can replace the strong limit by the norm limit. Moreover, t eit(e1 −e2 ) − 1 . esE Ke−sE ds = 1ie1 (E)K1ie2 (E) t−1 i(e1 − e2 )t 0 ie1 ,ie2 ∈spE

2 Remark 3.1. The following results generalize some aspects of Theorem 3.6 to the case when P is not necessarily finite dimensional. They are proven in [Da3]. We will not need these results. 1) If K exists, then it commutes with etE . 2) If K is a compact operator and Y is a Hilbert space, then K exists and we can replace the strong limit in (26) by the norm limit. 3) If E has a total set of eigenvectors, then K exists as well.

3.4 Second Order Asymptotics of Evolution with the First Order Term In this subsection we consider a somewhat more general situation than in Subsection 3.1. We make the Assumptions 2.1, 2.3 and 2.4, or 2.1*, 2.3* and 2.4 but we do not assume that P is finite dimensional, nor that PQP = 0. Thus we allow for a term of first order in λ in the asymptotics of the reduced dynamics. We again follow [Da3]. ! and PQP ! We assume also that PQP are bounded or w* continuous and that E + λPQP generates a C0 - or C0∗ -group of isometries on RanP. ! and PQP, ! Using the boundedness of off-diagonal elements PQP we see that ! ! PLλ P is the generator of a continuous semigroup. In this subsection, the definition of Kλ (t) slightly changes as compared with (9): λ−2 t e−s(E+λPQP) PQes!PLλ!P QPds. Kλ (t) := 0

Theorem 3.7. Suppose that the following assumptions are true: 1) For all t0 > 0, there exists c such that sup

sup Kλ (t) ≤ c.

|λ| 0, Trρ = 1, and ρ−1 exists). On the space of operators on K we introduce the scalar product given by ρ: (A|B)ρ := Trρ1/2 A∗ ρ1/2 B.

(41)

92


This space equipped with the scalar product (41) will be denoted by Bρ2 (K). Let ∗ρ denote the hermitian conjugation with respect to this scalar product. Thus if M is a map on B(K), then M ∗ρ is defined by (M ∗ρ (A)|B)ρ = (A|M (B))ρ . Explicitly,

M ∗ρ (A) = ρ−1/2 M ∗ (ρ1/2 Aρ1/2 )ρ−1/2 .

Definition 4.1. Let M be the generator of a Markov c.p. semigroup on B(K). We will say that M satisfies the standard Detailed Balance Condition with respect to ρ if there exists a self-adjoint operator Θ on K such that 1 (M − M ∗ρ ) = [Θ, ·]. 2i Theorem 4.1. Let M be the generator of a Markov c.p. semigroup on B(K). 1) Let M satisfy the standard DBC with respect to ρ. Then

(42)

M (A) = i[Θ, A] + Md (A), M ∗ (A) = −i[Θ, A] + ρ1/2 Md (ρ−1/2 Aρ−1/2 )ρ1/2 .

(43)

where Md is a generator of another Markov c.p. semigroup satisfying Md = Md∗ρ and Θ is a self-adjoint operator on K. Moreover, [Θ, ρ] = 0, M ∗ (ρ) = Md∗ (ρ) = 0. 2) Let M be given by (40). If there exists a unitary operator U : H → H such that [Θ, ρ] = 0, [W ∗ W, ρ] = 0, W = ρ−1/2 ⊗U W ρ1/2 , then M satisfies the standard DBC wrt ρ. Proof. 1) By (42), [Θ, ·] = −[Θ, ·]∗ρ = −ρ−1/2 [Θ, ρ1/2 · ρ1/2 ]ρ−1/2 . Using [Θ, 1] = 0, we obtain [Θ, ρ] = 0. Setting Md := 12 (M + M ∗ρ ) we obtain the decomposition (43). Clearly, 0 = M (1) = Md (1). Hence Md is Markov. Next 0 = Md (1) = Md∗ρ (1) gives Md (ρ) = 0. To see 2) we note that if Md = then Md∗ρ (B) = ρ−1/2

1

2 [W

∗

1 ∗ [W W, B]+ − W ∗ B⊗1 W, 2

W, ρ1/2 Bρ1/2 ]+ − W ∗ ρ1/2 Bρ1/2 ⊗ 1 W ρ−1/2

= 12 [W ∗ W, B]+ − (ρ1/2 ⊗1 W ρ1/2 )∗ B⊗1 ρ1/2 ⊗1 W ρ−1/2 . 2 Md is called the dissipative part of the generator M .


93

4.5 Detailed Balance Condition in the Sense of Alicki-Frigerio-Gorini-Kossakowski-Verri In this subsection we recall the definition of Detailed Balance Condition, which can be found in [A, FGKV]. Let us introduce the scalar product (A|B)(ρ) := TrρA∗ B. 2 (K) denote the space of operators on K equipped with this scalar product. Let B(ρ) Let M ∗(ρ) denote the conjugate of M with respect to this scalar product. Explicitly:

M ∗(ρ) (A) = ρ−1 M ∗ (ρA). Definition 4.2. We will say that M satisfies the Detailed Balance Condition with respect to ρ in the sense of AFGKV if there exists a self-adjoint operator Θ such that 1 (M − M ∗(ρ) ) = [Θ, ·]. 2i Note that for DBC in the sense of AFGKV, the analog of Theorem 4.1 1) holds, where we replace the scalar product (·|·)ρ with (·|·)(ρ) . In practical applications, c.p. semigroups usually originate from the weak coupling limit of reduced dynamics, as we describe further on in our lectures. In this case the standard DBC is equivalent to DBC in the sense of AFGKV, which follows from the following theorem: Theorem 4.2. Suppose that M satisfies ρ1/4 M (ρ−1/4 Aρ1/4 )ρ−1/4 = M (A). Then M satisfies the DBC in the sense of (42) iff it satisfies DBC in the sense of AFGKV. Moreover, the decompositions M = i[Θ, ·] + Md obtained in both cases concide. Proof. It is enough to note that the map 2 (K) Bρ2 (K) A → ρ−1/4 Aρ1/4 ∈ B(ρ)

is unitary. 2

5 Small Quantum System Interacting with Reservoir In this section we describe the class of W ∗ -dynamical systems that we consider in our notes. They are meant to describe a small quantum system S interacting with a large reservoir R. Pauli-Fierz systems, considered in [DJ2], are typical examples of such systems.

94


In Subsect. 5.1 we recall basic elements of the theory of W ∗ -algebras (see [BR1, BR2, DJP] for more information). In Subsect. 5.2 we introduce the class of W ∗ -dynamical systems describing S + R in purely algebraic (representationindependent) terms. In Subsect. 5.3 and 5.4 we explain the construction of two representations of our W ∗ -dynamical system: the semistandard and the standard representation. Both representations possess a distinguished unitary implementation of the dynamics. Its generator will be called the semi-Liouvillean in the former case and the Liouvillean in the latter case. The standard representation and the Liouvillean can be defined for an arbitrary W ∗ -algebra (see next subsection, [DJP] and references therein). The semistandard representation and the semi-Liouvillean are concepts whose importance is limited to a system of the form S + R considered in these notes. Their names were coined in [DJ2]. The advantage of the semistandard representation over the standard one is its simplicity, and this is the reason why it appears often in the literature [Da1,LeSp]. The semistandard representation is in particular well adapted to the study of the reduced dynamics. 5.1 W ∗ -Algebras In this subsection we recall the definitions of basic concepts related to the theory of W ∗ -algebras (see [BR1, BR2, DJP]). A W ∗ -dynamical system (M, τ ) is a pair consisting of a W ∗ -algebra M and a 1-parameter (pointwise) σ-weakly continuous group of ∗-automorphisms of M, R t → τ t . A standard representation of a W ∗ -algebra M is a quadruple (π, H, J, H+ ) consisting of a representation π, its Hilbert space H, an antilinear involution J and a self-dual cone H+ satisfying the following conditions: 1) Jπ(M)J = π(M) ; 2) Jπ(A)J = π(A)∗ for A in the center of M; 3) JΨ = Ψ for Ψ ∈ H+ ; 4) π(A)Jπ(A)H+ ⊂ H+ for A ∈ M. J is called the modular conjugation and H+ the modular cone. Every W ∗ -algebra possesses a standard representation, unique up to the unitary equivalence. Suppose that we are given a faithful state ω on M. In the corresponding GNS representation πω : M → B(Hω ), the state ω is given by a cyclic and separating vector Ωω . The Tomita-Takesaki theory yields the modular W ∗ -dynamics t → σωt , the modular conjugation Jω and the modular cone Hω+ := {AJω AΩω : A ∈ M}cl , where cl denotes the closure. The state ω satisfies the −1-KMS condition for the dynamics σω . The quadruple (πω , Hω , Jω , Hω+ ) is a standard representation of M. Until the end of this subsection, we suppose that a standard representation (π, H, J, H+ ) of M is given. Let ω be a state on M. Then there exists a unique vector in the modular cone Ω ∈ H+ representing ω. Ω is cyclic iff Ω is separating iff ω is faithful. Let t → τ t be a W ∗ -dynamics on M. The Liouvillean L of τ is a self-adjoint operator on H uniquely defined by demanding that


π(τ t (A)) = eitL π(A)e−itL ,

95

eitL H+ = H+ , t ∈ R.

(L implements the dynamics in the representation π and preserves the modular cone). It has many useful properties that make it an efficient tool in the study of the ergodic properties of the dynamics τ . In particular, L has no point spectrum iff τ has no normal invariant states, and L has a 1-dimensional kernel iff τ has a single invariant normal state.

5.2 Algebraic Description The Hilbert space of the system S is denoted by K. Throughout the notes we will assume that dim K < ∞. Let the self-adjoint operator K be the Hamiltonian of the small system. The free dynamics of the small system is τSt (B) := eitK Be−itK , B ∈ B(K). Thus the small system is described by the W ∗ -dynamical system (B(K), τS ). The reservoir R is described by a W ∗ -dynamical system (MR , τR ). We assume that it has a unique normal stationary state ωR (not necessarily a KMS state). The generator of τR is denoted by δR (that is τRt = eδR t ). The coupled system S + R is described by the W ∗ -algebra M := B(K) ⊗ MR . The free dynamics is given by the tensor product of the dynamics of its constituents: τ0t (A) := τSt ⊗ τRt (A), A ∈ M. We will denote by δ0 the generator of τ0 . Let V be a self-adjoint element of M. The full dynamics t → τλt := etδλ is defined by δλ := δ0 + iλ[V, ·]. (One can consider also a more general situation, where V is only affilliated to M— see [DJP] for details).

5.3 Semistandard Representation Suppose that MR is given in the standard form on the Hilbert space HR . Let 1R + stand for the identity on HR . We denote by HR , JR , and LR the corresponding modular cone, modular conjugation, and standard Liouvillean. Let ΩR be the (unique) + vector representative in HR of the state ωR . Clearly, ΩR is an eigenvector of LR . |ΩR )(ΩR | denotes projection on ΩR . Let us represent B(K) on K and take the representation of M in the Hilbert space K ⊗ HR . We will call it the semistandard representation and denote by π semi : M → B(K ⊗ HR ). (To justify its name, note that it is standard on its reservoir part, but not standard on the small system part). We will usually drop π semi and treat M as a subalgebra of B(K ⊗ HR ). Let us introduce the so-called free semi-Liouvillean Lsemi = K ⊗ 1 + 1 ⊗ LR . 0

(44)

96


The full semi-Liouvillean is defined as Lsemi = Lsemi + λV. λ 0 It is the generator of the distinguished unitary implementation of the dynamics τλ : semi

τλt (A) = eitLλ

Ae−itLλ

semi

,

A ∈ M,

(45)

with , ·]. δλ = i[Lsemi λ 5.4 Standard Representation Let us recall how one constructs the standard representation for the algebra B(K). Recall that B 2 (K) denotes the space of Hilbert-Schmidt operators on K. Equipped with the inner product (X|B) = Tr(X ∗ B) it is a Hilbert space. Note that B(K) acts naturally on B 2 (K) by the left multiplication. This defines a representation πS : B(K) → B(B 2 (K)). Let JS : B 2 (K) → B 2 (K) be defined by JS (X) = X ∗ , 2 and let B+ (K) be the set of all positive X ∈ B 2 (K). The algebra πS (B(K)) is in the standard form on the Hilbert space B 2 (K), and its modular cone and modular 2 (K) and JS . conjugation are B+ There exists a unique representation π : M → B(B 2 (K) ⊗ HR ) satisfying π(B ⊗ C) = πS (B) ⊗ C.

(46)

The von Neumann algebra π(M) is in standard form on the Hilbert space B 2 (K) ⊗ HR . The modular conjugation is J = JS ⊗ JR . The modular cone can be obtained as cl H+ := {π(A)Jπ(A) (ρ⊗ΩR ) : A ∈ M} , 2 where ρ is an arbitrary nondegenerate element of B+ (K). The Liouvillean of the free dynamics (the free Liouvillean) equals

L0 = [K, · ] ⊗ 1 + 1 ⊗ LR ,

(47)

and the Liouvillean of the full dynamics (the full Liouvillean) equals Lλ = L0 + λ(π(V ) − Jπ(V )J).

(48)

Sometimes we will assume that the reservoir is thermal. By this we mean that ωR is a β-KMS state for the dynamics τR . Set Ψ0 := e−βK/2 ⊗ ΩR . Then the state (Ψ0 |π(·)Ψ0 )/Ψ0 2 is a (τ0 , β)-KMS state. The Araki perturbation theory yields that Ψ0 ∈ Dom(e−β(L0 +λπ(V ))/2 ),


the vector

Ψλ := e−β(L0 +λπ(V ))/2 Ψ0

97

(49)

belongs to H+ ∩ KerLλ , and that (Ψλ |π(·)Ψλ )/Ψλ 2 is a (τλ , β)-KMS state (see [BR2, DJP]). In particular, zero is always an eigenvalue of Lλ . Thus, in the thermal case, (M, τλ ) has at least one stationary state.

6 Two Applications of the Fermi Golden Rule to Open Quantum Systems In this section we keep all the notation and assumtions of the preceding section. We will describe two applications of the Fermi Golden Rule to the W ∗ -dynamical system (M, τλ ) introduced in the previous section. In the first application we compute the LSO for the generator of the dynamics δλ . We will call it the Davies generator and denote by M . In the literature, M appears in the context of the Dynamical Fermi Golden Rule. It is the generator of the semigroup obtained by the weak coupling limit to the reduced dynamics. This result can be used to partly justify the use of completely positive semigroups to describe dynamics of small quantum systems weakly interacting with environment [Da1, LeSp]. In the second application we consider the standard representation of the W ∗ dynamical system in the Hilbert space H with the Liouvillean L. We will compute the LSO for iLλ . We denote it by iΓ . In the literature, iΓ appears in the context of the Spectral Golden Rule. It is used to study the point spectrum of the Liouvillean Lλ . The main goal of this study is a proof of the uniqueness of a stationary state in the thermal case and of the nonexistence of a stationary state in the non-thermal state under generic conditions [DJ1,DJ2,DJP]. (See also [JP1,JP2,BFS2] for related results). In Subsection 6.3, we will describe the result of [DJ3], which gives a relationship between the two kinds of LSO’s in the thermal case. In Subsections 6.4–6.6 we compute both LSO’s explicitly. In the case of the Davies generator, these formulas are essentially contained in the literature, in the case of the LSO for the Liouvillean, they are generalizations of the analoguous formulas from [DJ2]. Both LSO’s can be expressed in a number of distinct forms, each having a different advantage. In particular, as a result of our computations, we describe a simple characterization of the kernel of imaginary part of Γ , which can be used in the proof of the return to equilibrium. This characterization is a generalization of a result from [DJ2]. 6.1 LSO for the Reduced Dynamics It is easy to see that there exists a unique bounded linear map P on M such that for B ⊗ C ∈ M ⊂ B(K ⊗ HR ) P(B ⊗ C) = ωR (C)B ⊗ 1R .

98


P ∈ B(M) is a projection of norm 1. (It is an example of a conditional expectation). We identify B(K) with RanP by Note that δ0

B(K) B → B ⊗ 1R ∈ RanP. RanP

(50)

can be identified with i[K, ·].

We assume that ωR (V ) = 0. That implies P[V, ·]P = 0. Note that Assumptions 2.1*, 2.2, 2.3* and 2.4 are satisfied for the Banach space M, the projection P, the C0∗ -group of isometries etδ0 , and the perturbation i[V, ·]. Remark 6.1. One can ask whether the above defined projection P is given by the formula (5). Note that M is not a reflexive Banach space, so it is even not clear if this formula makes sense. Assume that δR has no eigenvectors apart from scalar operators. Then the set of eigenvalues of δ0 equals {i(k − k ) : k, k ∈ spK}. One can also show that for any e ∈ R, δ0 is globally ergodic at ie ∈ iR (see Appendix) and the corresponding eigenprojection is given by ωR (C) (1k (K)B1k−e (K)) ⊗1R . 1ie (δ0 )(B ⊗ C) = k∈spK

Therefore, in this case the answer to our question is positive and 1ie (δ0 ), P= e∈R

as suggested in Subsection 2.6. We make the following assumption: Assumption 6.1 Assumption 2.5 holds for (P, δ0 , i[V, ·]). This means that there exists 1e ([K, · ])[V, · ](ie + 0 − δ0 )−1 [V, · ]1e ([K, · ]). (51) M := − e∈sp([K,·])

M is the LSO for (P, δ0 , i[V, ·]). It will be called the Davies generator (in the Heisenberg picture). To describe the physical interpretation of M , suppose that we are interested only in the evolution of the observables corresponding to system S (taking, however, into account the influence of R). We also suppose that initially the reservoir is given by the state ωR . Let X be a density matrix on the Hilbert space K, such that the initial state of the system is described by the density matrix X ⊗|ΩR )(ΩR |. Let B ∈ B(K) be an observable for the system S, such that the measurement at the final time t is given by the operator B ⊗ 1R . Then the expectation value of the measurement is given by


TrK

X ⊗ |Ω)(Ω| τλt (B⊗1R ) .

99

(52)

Obviously, (52) tensored with 1R equals TrK XPτλt P(B ⊗ 1R ) . Now under quite general conditions [Da1, Da2, Da3] we have t/λ2

lim e−it[K,·]/λ Pτλ 2

λ→0

P = etM .

(53)

Thus M describes the reduced dynamics renormalized by [K, ·]/λ2 in the limit of the weak coupling, where we rescale the time by λ2 . Let us note the following fact: Theorem 6.1. Suppose Assumption 6.1 holds. Then M is the generator of a Markov c.p. semigroup and for any z ∈ C, M (B) = ezK M (e−zK BezK )e−zK .

(54)

Proof. We know that LSO M commutes with E = i[K, ·]. This is equivalent to ezE M e−zE = M , which means (54). The fact that M is a Lindblad-Kossakowski generator and annihilates 1 will follow immediately from explicit formulas given in Subsection 6.4. If we can prove 53, then an alternative proof is possible: we immediately see that the left hand side of (53) is a Markov c.p. map for any t and λ, hence so is etM . 2 6.2 LSO for the Liouvillean Consider the the Hilbert space B 2 (K) ⊗ HR and the orthogonal projection P := 1B2 (K) ⊗ |ΩR )(ΩR |. We have P L0 = L0 P = [K, ·]P . We identify B 2 (K) with RanP by B 2 (K) B → B ⊗ ΩR ∈ RanP.

(55)

We again assume that ωR (V ) = 0. This implies P π(V )P = P Jπ(V )JP = 0. Note that Assumptions 2.1, 2.2, 2.3 and 2.4 are satisfied for the Hilbert space B 2 (K) ⊗ HR , the projection P , the strongly continuous unitary group eitL0 , and the perturbation i(π(Q) − Jπ(Q)J). Remark 6.2. Assume that LR has no eigenvectors apart from ΩR . Then the set of eigenvalues of δ0 equals {i(k − k ) : k, k ∈ spK} and

100


1e (L0 )B ⊗ Ψ = (ΩR |Ψ )

(1k (K)B1k−e (K)) ⊗ΩR .

k∈spK

Therefore, P =

1ie (iL0 )

e∈R

is the spectral projection on the point spectrum of iL0 , as suggested in Subsection 2.6. Assumption 6.2 Assumption 2.5 for (P, iL0 , i(π(V ) − Jπ(V )J)) is satisfied. This means that there exists iΓ := − 1e ([K, · ])(π(V ) − Jπ(V )J) e∈sp([K,·])

×(ie + 0 − iL0 )−1 (π(V ) − Jπ(V )J)1e ([K, · ]). iΓ is the LSO for P, iL0 , i(π(V ) − Jπ(V )J) . We will call it the LSO for the Liouvillean. The operator Γ appeared in [DJ1], where it was used to give an upper bound on the point spectrum of Lλ for small nonzero λ. Theorem 6.2. Suppose that Assumption 6.2 holds. Then iΓ is the generator of a contractive c.p. semigroup and for any z ∈ C, Γ (B) = ezK Γ (e−zK BezK )e−zK .

(56)

Proof. The proof of (56) is the same as that of (54). etiΓ is contractive by Theorem 2.1. The proof of its complete positivity will be given later on (after (60)). 2

6.3 Relationship Between the Davies Generator and the LSO for the Liouvillean in Thermal Case Obviously, as vector spaces, B(K) and B 2 (K) coincide. We are interested in the relation between iΓ and generator M . We will see that in the thermal case the two operators are similar to one another. The following theorem was proven in [DJ3]: Theorem 6.3. Suppose that ωR is a (τR , β)-KMS state. Assumption 6.1 holds if and only if Assumption 6.2 holds. If these assumptions hold, then for B ∈ B(K), we have M (B) = iΓ (Be−βK/2 )eβK/2 (57) = eβK/4 iΓ (e−βK/4 Be−βK/4 )eβK/4 .


101

Remark 6.3. Let ρ := e−βK and γρ : B(K) → B 2 (K) be the linear invertible map defined by (58) γρ (B) := Bρ1/2 . Then the first identity of Theorem 6.3 can be written as M = iγρ−1 ◦ Γ ◦ γρ . Therefore, both iΓ and M have the same spectrum. Theorem 6.3 follows from the explicit formulas for M and iΓ given in Subsections 6.4–6.6. It is, however, instructive to give an alternative, time dependent proof of Identity (57), which avoids calculating both LSO’s. Strictly speaking, the identity will be proven for the “the dynamical Level Shift Operators” Mdyn and iΓdyn which, however, according to the Dynamical Fermi Golden Rule, under broad conditions, coincide with the usual Level Shift Operators M and iΓ . Theorem 6.4. Suppose that ωR is a (τR , β)-KMS state. Then the following statements are equivalent: 1) there exists an operator Mdyn satisfying t/λ2


λ→0

P = etMdyn .

2) there exists an operator Γdyn satisfying lim e−it[K,·]/λ P e−itLλ /λ P = eitΓdyn . 2

2

λ→0

Moreover,

Mdyn = γρ−1 ◦ iΓdyn ◦ γρ .

Proof. The Araki perturbation theory (see [DJP] and references therein) yields that the vector Ψλ , defined by (49), satisfies Ψλ = Ψ0 + O(λ) and Lλ Ψλ = 0. For X, B ∈ B(K) = B 2 (K), using the identifications (50) and (55), we have TrK X ∗ Pτ0−t τλt (B⊗1R ) = XeβK/2 ⊗ ΩR (e−itL0 eitLλ B⊗1R e−itLλ eitL0 ) e−βK/2 ⊗ΩR O(λ)

= (XeβK/2 ⊗ ΩR | e−itL0 eitLλ B⊗1R e−itLλ Ψλ )

O(λ)

= (XeβK/2 ⊗ ΩR | e−itL0 eitLλ B⊗1R e−βK/2 ⊗ΩR ) = X | (P e−itL0 eitLλ Be−βK/2 ⊗ΩR ) eβK/2

uniformly for t ≥ 0. Hence, since dim K < ∞, 2 2 e−it[K,·]/λ Pτλt (B⊗1R ) = e−it[K,·]/λ P eitLλ (Be−βK/2 ⊗ΩR ) eβK/2 + O(λ) uniformly for t ≥ 0. We conclude that for a given t the limit

102


lim e−it[K,·]/λ P eitLλ /λ P =: T t 2

2

λ→0

exists iff the limit

t/λ2


λ→0

P =: Tt

exists. Moreover, if the limits exist, then Tt = γρ−1 ◦ T t ◦ γρ . In particular, Tt is a semigroup iff T t is a semigroup and their generators (Mdyn and iΓdyn respectively) satisfy (57). 2 It is perhaps interesting that Theorem 6.4 can be immediately generalized to some non-thermal cases. Theorem 6.5. Suppose that instead of assuming that ωR is KMS, we make the following stability assumption: We suppose that ρ is a nondegenerate density matrix on K, and for |λ| ≤ λ0 there exists a normalized vector Ψλ ∈ H such that Ψλ = ρ1/2 ⊗ ΩR + o(λ0 ) and Lλ Ψλ = 0. Then all the statements of Theorem 6.4 remain true, with ρ replacing e−βK . Let us return to the thermal case. It is well known [A, FGKV] that in this case the Davies generator satisfies the Detailed Balance Condition. We will see that this fact is essentially equivalent to Relation (57). Theorem 6.6. Suppose that ωR is a (τR , β)-KMS state and Assumption 6.1 holds. Then the Davies generator M satisfies DBC for e−βK both in the standard sense and in the sense of AFGKV. 2 (K) to B 2 (K). Proof. Recall that the operator γρ defined in (58) is unitary from B(ρ) Recall also that in the thermal case

M = γρ−1 ◦ iΓ ◦ γρ . Hence,

M ∗(ρ) = −γρ−1 ◦ iΓ ∗ ◦ γρ .

Thus, 1 2i (M

− M ∗(ρ) ) = γρ−1 ◦ 12 (Γ + Γ ∗ ) ◦ γρ = γρ−1 ◦ [∆R , ·] ◦ γρ = [∆R , ·],

(where ∆R will be defined in the next subsection). This proves DBC in the sense of AFGKV. By Theorem 6.1 and the fact that ρ is proportional to e−βK , for any z ∈ C we have M (B) = ρz M (ρ−z Bρz )ρ−z . Therefore, by Theorem 4.2, the DBC in the sense of AFGKV is equivalent to the standard DBC. 2


103

6.4 Explicit Formula for the Davies Generator In this subsection we suppose that Assumption 6.1 is true and we describe an explicit formula for the Davies generator M . We introduce the following notation for the set of allowed transition frequencies and the set of allowed transition frequencies from k ∈ spK: F := {k1 − k2 : k1 , k2 ∈ spK} = sp[K, ·], Fk := {k − k1 : k1 ∈ spK}. Let |Ω) denote the map C z → |Ω)z := zΩ ∈ HR . Then 1K ⊗|Ω) ∈ B(K, K ⊗ HR ). Set v := V 1K ⊗|Ω) Note that v belongs to B(K, K ⊗ HR ). We also define v k1 ,k2 := 1k1 (K)⊗1R v 1k2 (K); v k,k−p ; v˜p :=

∆=

k∈spK

∗ k,k−p

(v )

1⊗(p + i0 − LR )−1 v k−p,k

k∈spK p∈Fk

=

(˜ v p )∗ 1⊗(p + i0 − LR )−1 v˜p .

p∈F

The real and the imaginary part of ∆ are given by ∗ k,k−p ∆R := 12 (∆ + ∆∗ ) = (v ) 1⊗P(p − LR )−1 v k−p,k k∈spK p∈Fk

=

(˜ v p )∗ 1⊗P(p − LR )−1 v˜p ;

p∈F

∆I :=

1 2i (∆

− ∆∗ ) = π

(v ∗ )k,k−p 1⊗δ(p − LR )v k−p,k

k∈spK p∈Fk

=π

(˜ v p )∗ 1⊗δ(p − LR )˜ vp ;

p∈F

Note that ∆ ≥ 0. Below we give four explicit formulas for the Davies generator in the Heisenberg picture: I

104


M (B) = i(∆B − B∆∗ ) p ∗ (˜ v ) B⊗δ(p − LR )˜ vp +2π p∈F

=i

(˜ v p )∗ 1⊗(p − i0 − LR )−1 (˜ v p B − B⊗1R v˜p )

p∈F

−i

(B(˜ v p )∗ − (˜ v p )∗ B⊗1R ) 1⊗(p + i0 − LR )−1 v˜p

p∈F

= i[∆R , B] p ∗ (˜ v ) 1⊗δ(p − LR ) (B⊗1R v˜p − v˜p B) +π p∈F

+π

((˜ v p )∗ B⊗1R − B(˜ v p )∗ ) 1⊗δ(p − LR )˜ vp

p∈F

∞

=i

1k (K)(Ω|V 1k−p (K)τ0s (V )Ω)1k (K)Bds

k∈spK p∈Fk 0

−i

0

k∈spK p∈Fk −∞

+2π

B1k (K)(Ω|V 1k−p (K)τ0s (V )Ω)1k (K)ds

∞

k,k ∈spK

−∞

1k (K)(Ω|V 1k−p (K)B1k −p (K)τ0s (V )Ω)1k (K)ds.

p∈Fk ∩Fk

The first expression on the right has the standard form of a Lindblad-Kossakowski generator (39). The second expression can be used in a characterization of the kernel of M . In particular, it implies immediately that 1K ∈ KerM . The third expression shows the splitting of M into a reversible part and an irreversible part. The fourth expression uses uses time-dependent quantities and is analoguous to formulas appearing often in the physics literature. 6.5 Explicit Formulas for LSO for the Liouvillean In this subsection we suppose that Assumption 6.2 is true and we describe an explicit formula for iΓ , the LSO for the Liouvillean. Recall that π denotes the standard representation of M and LR is the Liouvillean of the free reservoir dynamics τR . Let L0R denote the Liouvillean of the modular dynamics for the state ωR . The fact that ωR is stationary for τRt implies that the two Liouvilleans commute: 0

0

eitLR eisLR = eisLR eitLR , t, s ∈ R. The following identities follow from the modular theory and will be useful in our explicit formulas for Γ :


105

Proposition 6.1. The following identities are true for B ∈ B2 (K): π(V ) B⊗ΩR = vB, 0

Jπ(V )J B⊗ΩR = B⊗eLR /2 v. Moreover, if B1 , B2 ∈ B 2 (K) and Φ ∈ HR , then 0

(B1 ⊗ Φ|vB2 ) = (eLR /2 vB1 |B2 ⊗ JR Φ).

(59)

Proof. To prove the second identity we note that J B⊗ΩR = B ∗ ⊗ΩR , Jπ(V )B ∗ ⊗ΩR = eLR /2 B⊗π(V )ΩR . 0

To see (59), we note that it is enough to assume that Φ = A ΩR , where A ∈ π(MR ) and π(MR ) denotes the commutant of π(MR ). Then (B1 ⊗ Φ|vB2 ) = (B1 ⊗ A ΩR |π(V )B2 ⊗ ΩR ) = (π(V )B1 ⊗ ΩR |B2 ⊗ A∗ ΩR ) = (vB1 |B2 ⊗ eLR /2 JR A ΩR ). 0

2 Note that if we compare (59) with the definition of the !-operation (37), and if we make the identification Φ = JR Φ, then we see that (59) can be rewritten as 0

v = eLR /2 v. The LSO for the Liouvillean equals iΓ (B) = i∆B − iB∆∗ p ∗ 0 +2π (˜ v ) B⊗δ(p − LR )eLR /2 v˜p .

(60)

p∈F

Note that the term on the second line of (60) is completely positive. Therefore, (60) is in the Lindblad-Kossakowski form. Hence eitΓ is a c.p. semigroup. This completes the proof of Theorem 6.2. Let us split Γ into its real and imaginary part: Γ R :=

1 1 (Γ + Γ ∗ ), Γ I := (Γ − Γ ∗ ). 2 2i

(Γ ∗ is defined using the natural scalar product in B 2 (K)). Then the real part is given by (61) Γ R (B) = [∆R , B].

106


The imaginary part equals 0 (˜ v p )∗ 1⊗δ(p − LR ) B⊗eLR /2 v˜p − v˜p B p∈F p ∗ 0 (˜ v ) B⊗eLR /2 − B(˜ v p )∗ 1⊗δ(p − LR )˜ vp . +π

ΓI = π

(62)

p∈F

Another useful formula for Γ I represents it as a quadratic form: TrB1 Γ I (B2 ) 0 0 =π Tr(˜ v p B1 − B1 ⊗eLR /2 v˜p )∗ 1⊗δ(p − LR )(˜ v p B2 − B2 ⊗eLR /2 v˜p ). p∈F

(63) To see (63) we note the following identities: (˜ v p )∗ 1⊗δ(p − LR )˜ v p = TrHR 1⊗δ(p − LR )eLR v˜p (˜ v p )∗ , 0

(˜ v p )∗ B⊗δ(p − LR )eLR /2 v˜p = TrHR 1⊗δ(p − LR )eLR /2 v˜p B(˜ v p )∗ , 0

0

which follow from (59). The study of the kernel of Γ I is important in applications based on the Spectral Fermi Golden Rule. The identity (63) is very convenient for this purpose. It was first discovered in the context of Pauli-Fierz systems in [DJ2]. In the thermal case (63) can be transformed into Tre−βK (˜ v p B1 eβK/2 − B1 eβK/2 ⊗1R v˜p )∗ TrB1 Γ I (B2 ) = π p∈F (64) ×1⊗δ(p − LR )(˜ v p B2 eβK/2 − B2 eβK/2 ⊗1R v˜p ). 6.6 Identities Using the Fibered Representation Using the decomposition of the Hilbert space HR into the fibered integral given by the spectral decomposition of LR , we can rewrite (63) in an even more convenient form. To describe the fibered form of (63), we will not strive at the greatest generality. We will make the following assumptions (which are modelled after the version of the Jakˇsić-Pillet gluing condition considered in [DJ2]): Assumption 6.3 There exists a Hilbert space G and a linear isometry U : G ⊗ 0 L2 (R) → HR such that Ran v, Ran eβLR /2 v ⊂ K ⊗ RanU and U ∗ LR U is the operator of the multiplication by the variable in R. We will identify RanU with L2 (R) ⊗ G. Note that Ψ ∈ L2 (R) ⊗ G can be identified with an almost everywhere defined function R p → Ψ (p) ∈ G such that (LR Ψ )(p) = pΨ (p), (see e.g. [DJ2]). We can (at least formally) write L0R as the direct integral:


107

(L0R Ψ )(p) = L0R (p)Ψ (p), where L0R (p) are operators on G. Likewise, v ∈ B(K, K⊗HR ) can be interpreted as an almost everywhere defined function R p → v(p) ∈ B(K, K ⊗ G) such that (LR vΦ)(p) = pv(p)Φ, Φ ∈ K. Assumption 6.4 R p → v(p), L0R (p) are continuous at p ∈ F, so that we can define unambiguously v(p), L0R (p) for those values of p. Under the above two assumptions we can define wp := v˜p (p) p ∈ F. Then we can rewrite the formula (63) as TrB1 Γ I (B2 ) 0 0 =π Tr(wp B1 − B1 ⊗eLR (p)/2 wp )∗ (wp B2 − B2 ⊗eLR (p)/2 wp ).

(65)

p∈F

(65) implies immediately Theorem 6.7. The kernel of Γ I consists of B ∈ B2 (K) such that 0

wp B = B⊗eLR (p)/2 wp , p ∈ F.

Note that Theorem 6.7 implies that generically KerΓ I = {0}. Therefore, for a generic open quantum system, if the Spectral Fermi Golden Rule can be applied, then the Liouvillean Lλ has no point spectrum for small nonzero λ. Therefore, for the same λ, the W ∗ -dynamical system (M, τλ ) has no invariant normal states. Identities (63), (65) and Theorem 6.7 are generalizations of similar statements from [DJ2]. In [DJ2] the reader will find their rigorous application to Pauli-Fierz systems. If ωR is a (τR , β)-KMS state, we can transform (65) as follows: TrB1 Γ I (B2 ) = π Tr e−βK (wp B1 eβK/2 − B1 eβK/2 ⊗1R wp )∗ p∈F (66) ×(wp B2 eβK/2 − B2 eβK/2 ⊗1R wp ). Following [DJ2], define N := {C : wp C = C⊗1R wp , p ∈ F}.

(67)

Repeating the arguments of [DJ2] we get Theorem 6.8.

1) N is a ∗-algebra invariant wrt eitK · e−itK and containing C1.

108


2) The kernel of Γ I consists of e−βK/2 C with C ∈ N . Theorem 6.8 implies that in a thermal case, generically, KerΓ I = {0}. Therefore, if the Spectral Fermi Golden Rule can be applied, for a generic open quantum system, for small nonzero λ, the Liouvillean Lλ has no point spectrum except for a nondegenerate eigenvalue at zero. Therefore, for the same λ, the W ∗ -dynamical system (M, τλ ) has a unique stationary normal state. Again, Identity (66) and Theorem 6.8 are generalizations of similar statements from [DJ2], where they were used to study the return to equilibrium for thermal Pauli-Fierz systems.

7 Fermi Golden Rule for a Composite Reservoir In this section we describe a small quantum system interacting with several reservoirs. We will assume that the reservoirs R1 , . . . , Rn do not interact directly—they interact with one another only through the small system S. We will compute both kinds of the LSO for the composite system. We will see that it is equal to the sum of the LSO’s corresponding to the interaction of S with a single reservoir Ri . Our presentation is divided into 3 subsections. The first uses the framework of Section 2, the second—that of Section 5 and the third—that of Section 6. 7.1 LSO for a Sum of Perturbations Let X be a Banach space. Let P1 , . . . , Pn be projections of norm 1 on X such that Pi Pj = Pi Pj . Let L0 be the generator of a group of isometries such that L0 Pi = Pi L0 , i = 1, . . . , n. Let Qi be operators such that RanPi ⊂ DomQi and Qi Pj = Pj Qi , i = j. Set Q :=

n

Qj ,

P :=

j=1

n

Pj ,

Xj := Ran

j=1

Pi .

i =j

Clearly, Xj is left invariant by L0 , Pj , Qj . Therefore, these operators can be restricted to Xj . We set L0,j := L0 , Pj := Pj = P , Qj := Qj . Xj

Clearly, RanP = RanPj We set E := L0

RanP

Xj

L0

RanP

Xj

= L0,j

Xj

RanPj

.

.

Theorem 7.1. Suppose that Pj Qj Pj = 0, j = 1, . . . , n. Then: 1) PQP = 0, Pj Qj Pj = 0, j = 1, . . . , n.


109

2) Suppose in addition that the LSO’s for (Pi , L0,i , Qi ), denoted Mi , exist. Then the LSO for (P, L0 , Q), denoted M , exists as well and M=

n

Mi .

i=1

# Proof. Set Jj := i =j Pi . 1) It is obvious that Pi Qi Pi = 0 implies Pi Qi Pi = 0. 2) We have M =

n

1ie (E)Qi (ie + 0 − L0 )−1 Qj 1ie (E),

i,j=1 ie∈spE

Mj =

1ie (E)Qj (ie + 0 − L0,j )−1 Qj 1ie (E).

.

ie∈spE

For i = j, PQi (ie + 0 − L0 )−1 Qj P = PQi Jj (ie + 0 − L0 )−1 Qj P = 0, since PQi Jj = PPi Qi Pi Jj = 0. Clearly, PQi (ie + 0 − L0 )−1 Qi P = PQi (ie + 0 − L0,i )−1 Qi P. 2 7.2 Multiple Reservoirs Suppose that (MR1 , τR1 ),. . . , (MRn , τRn ) are W ∗ -dynamical systems with τRt i = etδRi . Let 1Ri denote the identity on HRi . Suppose that MRi have a standard representation in Hilbert spaces HRi with the modular conjugations JRi . Let LRi be the Liouvillean of the dynamics τRi . Let (B(K), τS ) describe the small quantum system, with τSt := eit[K,·] , as in Section 5. Define the free systems (Mi , τ0,i ) where Mi := B(K) ⊗ MRi , Hi := B 2 (K) ⊗ HRi , Ji := JS ⊗ JRi , t τ0,i := τSt ⊗ τRt i = etδ0,λ ,

δ0,i = i[K, ·] + δRi , L0,i = [K, ·] + LRi .

110


Let πi be the standard representation of Mi in Hi and Ji the corresponding conjugations. t := etδλ,i Let Vi ∈ Mi and define the perturbed systems (Mi , τλ,i ) where τλ,i and δλ,i := δ0,i + iλ[Vi , ·], Lλ,i = L0,i + λ(πi (Vi ) − Ji πi (Vi )Ji ). Likewise, consider the composite reservoir R described by the W ∗ -dynamical system (MR , τR ), where MR := MR1 ⊗ · · · ⊗ MRn , HR := HR1 ⊗ · · · ⊗ HRn , JR := JR1 ⊗ · · · ⊗ JRn , τRt := τRt 1 ⊗ · · · ⊗ τRt n = etδR , δR := δR1 + · · · + δRn , LR = LR1 + · · · + LRn . Define the free composite system (M, τ0 ) where M := B(K) ⊗ MR , H := B 2 (K) ⊗ HR , J = JS ⊗ JR , τ0t := τSt ⊗ τRt = etδ0 , δ0 = i[K, ·] + δR , L0 = [K, ·] + LR . Let π be the standard representation of M in H. Set V = V1 + · · · + Vn . The perturbed composite system describing the small system S interacting with the composite reservoir R is (M, τλ ), where τλt := etδλ , δλ := δ0 + iλ[V, ·], Lλ := L0 + λ(π(V ) − Jπ(V )J).

.

7.3 LSO for the Reduced Dynamics in the Case of a Composite Reservoir Suppose that the reservoir dynamics τRi have stationary states ωRi . We introduce a projection of norm one in M, denoted Pi , such that Pi (B ⊗ A1 ⊗, · · · ⊗ Ai ⊗ · · · ⊗ An ) = ωRi (Ai )B ⊗ A1 ⊗ · · · ⊗ 1Ri ⊗ · · · ⊗ An .


111

#n

Set P := i=1 Pi . The projection Pi restricted to Mi (which can be viewed as a subalgebra of M) is denoted by Pi . Explicitly, Pi (B ⊗ Ai ) = ωRi (Ai )B ⊗ 1Ri . Assume that ωRi (Vi ) = 0 for i = 1, . . . , n. Note that we can apply the formalism of Subsection 7.1, where the Banach space is X is M, the projections Pi are Pi , the generator of an isometric dynamics L0 is δ0 and the perturbations Qi are i[Vi , ·]. Clearly, Xi can be identified with Mi and RanP with B(K). We obtain the LSO for (P, δ0 , i[V, ·]), denoted M , and the LSO’s for (Pi , δ0,i , i[Vi , ·]), denoted Mi . By Theorem 7.1, we have M=

n

Mi ,

i=1

7.4 LSO for the Liovillean in the Case of a Composite Reservoir Let ΩRi be the standard vector representative of ωRi . We define the orthogonal projection in B(H) P i := 1B2 (K) ⊗ 1R1 ⊗ · · · ⊗ |ΩRi )(ΩRi | ⊗ · · · ⊗ 1Rn . The projection P i restricted to Hi is denoted by Pi and equals #n

Pi = 1B2 (K) ⊗ |ΩRi )(ΩRi |.

Set P = i=1 P i . We can apply the formalism of Subsection 7.1, where the Banach space is X is H, the projections Pi are P i , the generator of an isometric dynamics L0 is iL0 and the perturbations Qi are i(Vi − Ji Vi Ji ). Clearly, Xi can be identified with Hi and RanP with B 2 (K) (which as a vector space coincides with B(K)). We obtain the LSO for (P, iL0 , i(V − JV J)), denoted iΓ , and the LSO for (Pi , iL0,i , i(Vi − Ji Vi Ji )), denoted iΓi . By Theorem 7.1, we have iΓ =

n

iΓi .

i=1

The following theorem follows from obvious properties of negative operators: Theorem 7.2. Suppose that for some i = j, dim KerΓiI = dim KerΓjI = 1 and KerΓiI = KerΓjI . Then KerΓ = {0}. Corollary 7.1. Suppose that for some i = j, the states ωRi and ωRj are (τRi , βi ) and (τRj , βj )-KMS. Let Ni and Nj be the corresponding ∗-algebras defined as in (67). Suppose that βi = βj and Ni = Nj = C1. Then KerΓ = {0}. If we can apply the Spectral Fermi Golden Rule, then under the assumptions of 7.1, for sufficiently small nonzero λ, Lλ has no point spectrum. Consequently, for the same λ, the system (Mλ , τλ ), has no invariant normal states.

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A Appendix – One-Parameter Semigroups In this section we would like to discuss some concepts related to one-parameter semigroups of operators in Banach spaces, which are used in our lectures. Even though the material that we present is quite standard, we could not find a reference that presents all of it in a convenient way. Most of it can be found in [BR1]. Less pedantic readers may skip this appendix altogether. Let X be a Banach space. Recall that [0, ∞[ t → U (t) ∈ B(X ) is called a 1-parameter semigroup iff U (0) = 1 and U (t1 )U (t2 ) = U (t1 + t2 ). If [0, ∞[ is replaced with R, then we speak about a one-parameter group instead of a oneparameter semigroup. We say that U (t) is a strongly continuous semigroup (or a C0 -semigroup) iff for any Φ ∈ X , t → U (t)Φ is continuous. Every C0 -semigroup possesses its generator, that is the operator A defined as follows: Φ ∈ DomA ⇔ lim t−1 (U (t) − 1)Φ =: AΦ exists. t0

The generator is always closed and densely defined and uniquely determines the semigroup. We write U (t) = etA . Recall also the following well known characterization of contractive semigroups: Theorem A.1. The following conditions are equivalent: 1) etA is contractive for all t ≥ 0. 2) A is densely defined, spA ⊂ {z ∈ C : Rez ≤ 0} and (z − A)−1 ≤ (Rez)−1 for Rez > 0. 3) (i) A is densely defined and for some z+ with Rez+ > 0, z+ ∈ spA, (ii) A is dissipative, that is for any Φ ∈ DomA there exists ξ ∈ X ∗ with (ξ|Φ) = Φ and (ξ|AΦ) ≤ 0. Moreover, if A is bounded, then we can omit (i) in 3). There exists an obvious corollary of the above theorem for groups of isometries: Theorem A.2. The following conditions are equivalent: 1) etA is isometric for all t ∈ R. 2) A is densely defined, spA ⊂ iR and (z − A)−1 ≤ |Rez|−1 for Rez = 0. 3) (i) A is densely defined and for some z± with ±Rez± > 0, z± ∈ spA, (ii) A is conservative, that is for any Φ ∈ DomA there exists ξ ∈ X ∗ with (ξ|Φ) = Φ and Re(ξ|AΦ) = 0. Morover, if A is bounded, then we can omit (i) in (3). Not all semigroups considered in our lectures are C0 -semigroups. An important role in our lectures (and in applications to statistical physics) is played by somewhat less known C0∗ -semigroups. In order to discuss them, first we need to say a few words about dual Banach spaces.


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Let X ∗ denote the Banach space dual to X (the space of continuous linear functionals on X ). We will use the sesquilinear duality between X ∗ and X : the form (ξ|Φ) will be antilinear in ξ ∈ X ∗ and linear in Φ ∈ X . The so-called weak∗ (w∗) topology on X ∗ is defined by the seminorms |(·|Φ)|, where Φ ∈ X . The space of w∗ continuous linear operators on X ∗ will be denoted by Bw∗ (X ∗ ). Note that Bw∗ (X ∗ ) ⊂ B(X ∗ ). If A ∈ B(X ), and A∗ is its adjoint, then A∗ ∈ Bw∗ (X ∗ ). Conversely, if B ∈ Bw∗ (X ∗ ), then there exists a unique A ∈ B(X ), sometimes called the preadjoint of B, such that B = A∗ . Likewise, if A is closed and densely defined on X , then A∗ is w∗ closed and w∗ densely defined on X ∗ . We say that [0, ∞[ t → W (t) ∈ Bw∗ (X ∗ ) is a w∗ continuous semigroup (or a C0∗ -semigroup) iff t W (t)ξ is w∗ continuous for any ξ ∈ X ∗ . Note that if U (t) is a C0 -semigroup, then U (t)∗ is a C0∗ -semigroup. Conversely, if W (t) is a C0∗ -semigroup on X ∗ , then there exists a unique C0 -semigroup U (t) on X such that W (t) = U (t)∗ . Every C0∗ -semigroup W (t) possesses its generator, that is the operator B defined as follows: ξ ∈ DomB ⇔ w ∗ − lim t−1 (W (t) − 1)ξ =: Bξ exists. t0

The generator is always w∗-closed and w∗-densely defined and uniquely determines the semigroup. We write W (t) = etB . We have ∗

(etA )∗ = etA . On a reflexive Banach space, e.g. on a Hilbert space, the concepts of a C0 - and C0∗ -semigroup coincide. Unfortunately, W ∗ -algebras are usually not reflexive. They are, however, dual Banach spaces: they are dual to the space of normal functionals. In the context of W ∗ -algebras the w∗-topology is usually called the σ-weak or ultraweak topology. Groups of automorphisms of W ∗ -algebras are rarely C0 -groups. To see this note that if H is a self-adjoint operator on a Hilbert space H, then t → eitH · e−itH

(68)

is always a C0∗ -group on B(H). It is a C0 -group (and even a norm continuous group) iff H is bounded, which is usually a very severe restriction. In the context of W ∗ -algebras, C0∗ groups are usually called (pointwise) σweakly continuous groups. C0∗ -groups of ∗-automorphisms are often called W ∗ dynamics. So far, all the material that we recalled can be found e.g. in [BR1]. Now we would like to discuss how to define the spectral projection onto a (not necessarily isolated) eigenvalue of a generator of contractive semigroup. We will see that a fully satisfactory answer is available for purely imaginary eigenvalues in the case of a reflexive Banach spaces. For non-reflexive Banach spaces the situation is much more complicated. Our discussion is adapted from [Zs] and partly from [Da3].

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Let A be the generator of a contractive C0 -semigroup on X and e ∈ R. Following [Zs], we say that A is ergodic at ie iff 1ie (A) := lim ξ(ξ + ie − A)−1

(69)

ξ0

exists. Let B be the generator of a contractive C0∗ -semigroup on X ∗ and e ∈ R. Following [Zs], we say that B is globally ergodic at ie iff 1ie (B) := w ∗ − lim ξ(ξ + ie − B)−1

(70)

ξ0

exists and is w∗-continuous. As we will see from the theorem below, (69) and (70) can be called spectral projections onto the eigenvalue ie. Theorem A.3. Let A, B and e ∈ R be as above. 1) If A is ergodic at ie, then 1ie (A) is a projection of norm 1 such that cl

Ran1ie (A) = Ker(A − ie), Ker1ie (A) = (Ran (A − ie)) . 2) On a reflexive Banach space, we have always the ergodic property for all generators of contractive semigroups and all ie ∈ iR. 3) If B is globally ergodic at ie, then 1ie (B) is a w∗-continuous projection of norm 1 such that Ran1ie (B) = Ker(B − ie), Ker1ie (B) = (Ran (A − ie))

w∗cl

.

4) A is ergodic at ie iff A∗ is globally ergodic at −ie and 1ie (A)∗ = 1−ie (A∗ ). 1) and 2) are proven in [Da3] Theorem 5.1 and Corollary 5.2. 3) and 4) can be proven by adapting the arguments of [Zs] Theorem 3.4 and Corollary 3.5. As an ilustration of the above concepts consider the W ∗ -dynamics (68). Clearly, it is a group of isometries and the spectrum of its generator i[H, ·] is contained in iR. If H possesses only point spectrum, then i[H, ·] is globally ergodic for any ie ∈ iR. In fact, we have the following formula for 1ie (i[H, ·])(C) = 1x+e (H)C1x (H). x∈R

Note that i[H, ·] always possesses an eigenvalue 0 and the corresponding eigenvectors are all operators commuting with H. It is never globally ergodic at 0 if H has some continuous spectrum.


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References [AJPP] Aschbacher, W., Jakˇsić, V., Pautrat, Y., Pillet, C.-A.: Introduction to non-equilibrium quantum statistical mechanics. Grenoble lecture notes. [A] Alicki, R.: On the detailed balance condition for non-hamiltonian systems, Rep. Math. Phys. 10 (1976) 249 [AL] Alicki, R., Lendi, K.: Quantum dynamical semigroups and applications, Lecture Notes in Physics no 286, Springer 1991 [BR1] Brattelli, O., Robinson D. W.: Operator Algebras and Quantum Statistical Mechanics, Volume 1. Springer-Verlag, Berlin, second edition 1987. [BR2] Brattelli, O., Robinson D. W.: Operator Algebras and Quantum Statistical Mechanics, Volume 2. Springer-Verlag, Berlin, second edition 1996. [BFS1] Bach, V., Fröhlich, J., Sigal, I.: Quantum electrodynamics of confined nonrelativistic particles, Adv. Math. 137, 299 (1998). [BFS2] Bach, V., Fröhlich, J., Sigal, I.: Return to equilibrium. J. Math. Phys. 41, 3985 (2000). [Da1] Davies, E. B.: Markovian master equations. Commun. Math. Phys. 39, 91 (1974). [Da2] Davies, E. B.: Markovian master equations II. Math. Ann. 219, 147 (1976). [Da3] Davies, E. B.: One parameter semigroups, Academic Press 1980 [DJ1] Dereziński, J., Jakˇsić, V.: Spectral theory of Pauli-Fierz operators. J. Func. Anal. 180, 243 (2001). [DJ2] Dereziński, J., Jakˇsić, V.: Return to equilibrium for Pauli-Fierz systems. Ann. Henri Poincaré 4, 739 (2003). [DJ3] Dereziński, J., Jakˇsić, V.: On the nature of Fermi golden rule for open quantum systems, J. Statist. Phys. 116 (2004), 411 (2004). [DJ4] Dereziński, J., Jakˇsić, V.: In preparation. [Di] Dirac, P.A.M.: The quantum theory of the emission and absorption of radiation. Proc. Royal Soc. London, Series A 114, 243 (1927). [DJP] Dereziński, J., Jakˇsić, V., Pillet, C. A.:Perturbation theory of W ∗ -dynamics, Liouvilleans and KMS-states, to appear in Rev. Math. Phys [FGKV] Frigerio, A., Gorini, V., Kossakowski A., Verri, M.: Quantum detailed balance and KMS condition, Comm. Math. Phys. 57 (1977) 97-110 [DF1] Dereziński, J., Früboes, R.: Level Shift Operator and second order perturbation theory. J. Math. Phys. 46, 033512 (2005). [DF2] Dereziński, J., Früboes, R.: Stationary van Hove limit. J. Math. Phys. 46, 063511 (2005). [Fe] Fermi, E.: Nuclear Physics, University of Chicago Press, Chicago 1950 [GKS] Gorini, V., Kossakowski, A., Sudarshan, E.C.G. Journ. Math. Phys. 17 (1976) 821 [Haa] Haake, F.: Statistical treatment of open systems by generalized master equation. Springer Tracts in Modern Physics 66, Springer-Verlag, Berlin, 1973. [JP1] Jakˇsić, V., Pillet, C.-A.: On a model for quantum friction III. Ergodic properties of the spin-boson system. Commun. Math. Phys. 178, 627 (1996). [JP2] Jakˇsić, V., Pillet, C.-A.: Spectral theory of thermal relaxation. J. Math. Phys. 38, 1757 (1997). [JP3] Jakˇsić, V., Pillet, C.-A.: From resonances to master equations. Ann. Inst. Henri Poincaré 67, 425 (1997). [JP4] Jakˇsić, V., Pillet, C.-A.: Non-equilibrium steady states for finite quantum systems coupled to thermal reservoirs. Commun. Math. Phys. 226, 131 (2002).

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[JP5] Jakˇsić, V., Pillet, C.-A.: Mathematical theory of non-equilibrium quantum statistical mechanics. J. Stat. Phys. 108, 787 (2002). [JP6] Jakˇsić, V., Pillet, C.-A.: In preparation. [Ka] Kato, T.: Perturbation Theory for Linear Operators, second edition, [KTH] Kubo, R., Toda, M., Hashitsume, N.: Statistical Physics II. Nonequilibrium Statistical Mechanics. Springer-Verlag, Berlin, 1985. [L] Lindblad, G.: On the generators of quantum dynamical semigroups, Comm. Math. Phys. 48 (1976) 119-130 [M] Merkli, M.: Positive commutators in non-equilibrium quantum statistical mechanics. Commun. Math. Phys. 223, 327 (2001). [LeSp] Lebowitz, J., Spohn, H.: Irreversible thermodynamics for quantum systems weakly coupled to thermal reservoirs. Adv. Chem. Phys. 39, 109 (1978). [Ma1] Majewski, W. A.: Dynamical semigroups in the algebraic formulation of statistical mechanics, Fortschritte der Physik 32 (1984) 89-133 [Ma2] Majewski, W. A.: Journ. Math. Phys. The detailed balance condition in quantum statistical mechanics 25 (1984) 614 [MaSt] Majewski, W. A., Streater, R. F.: Detailed balance and quantum dynamical maps Journ. Phys. A: Math. Gen. 31 (1998) 7981-7995 [VH1] Van Hove, L.: Quantum-mechanical perturbations giving rise to a statistical transport equation. Physica 21 (1955) 517. [VH2] Van Hove, L.: The approach to equilibrium in quantum statitsics. Physica 23 (1957) 441. [VH3] Van Hove, L.: Master equation and approach to equilibrium for quantum systems. In Fundamental problems in statistical mechanics, compiled by E.G.D. Cohen, NorthHoland, Amsterdam 1962. [RS4] Reed, M., Simon, B.: Methods of Modern Mathematical Physics, IV. Analysis of Operators, London, Academic Press 1978. [Sp] Spohn, H.: Entropy production for quantum dynamical semigroups, Journ. Math. Phys. 19 (1978) 1227 [St] Stinespring, W. F.: Positive functions on C ∗ -algebras, Proc. Am. Math. Soc. 6 (1955) 211-216 [WW] Weisskopf, V., Wigner, E.: Berechnung der natürlichen Linienbreite auf Grund der Dirakschen Lichttheorie, Zeitschrift für Physik 63 (130) 54 [Zs] Zsidó, L.: Spectral and ergodic properties of analytic generators, Journ. Approximation Theory 20 (1977) 77-138

Decoherence as Irreversible Dynamical Process in Open Quantum Systems Philippe Blanchard1 and Robert Olkiewicz2 1

2

1

Physics Faculty and BiBoS, University of Bielefeld, Universitätsstrasse 25, 33615 Bielefeld, Germany e-mail: physik.uni-bielefeld.de Institute of Theoretical Physics, University of Wrocław, pl. M. Borna 9, 50-204 Wrocław, Poland e-mail: [email protected]

Physical and Mathematical Prologue . . . . . . . . . . . . . . . . . . . . . . . . . . . . 118 1.1 1.2 1.3 1.4 1.5

2

The Asymptotic Decomposition of T . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 126 2.1 2.2 2.3 2.4 2.5

3

Infinite Spin Systems . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 138 Continuous Pointer States [10] . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 139 Decoherence-Induced Spin Algebra [6] . . . . . . . . . . . . . . . . . . . . . . . 143 From Quantum to Classical Dynamical Systems [38] . . . . . . . . . . . . 146

Dynamical Semigroups on CCR Algebras . . . . . . . . . . . . . . . . . . . . . . . . 148 4.1 4.2 4.3 4.4 4.5

5

Notation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 126 Dynamics in the Markovian Regime . . . . . . . . . . . . . . . . . . . . . . . . . . 127 The Unitary Decomposition of T2 . . . . . . . . . . . . . . . . . . . . . . . . . . . . 130 The Isometric-Sweeping Decomposition . . . . . . . . . . . . . . . . . . . . . . 133 Remarks . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 135

Review of Decoherence Effects in Infinite Spin Systems . . . . . . . . . . . . 138 3.1 3.2 3.3 3.4

4

Physical Background . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 118 Environmental Decoherence . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 119 Algebraic Framework . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 120 Quantum Dynamical Semigroups . . . . . . . . . . . . . . . . . . . . . . . . . . . . 121 A Model of a Discrete Pointer Basis . . . . . . . . . . . . . . . . . . . . . . . . . . 123

Algebras of Canonical Commutation Relations (CCR) . . . . . . . . . . . 148 Promeasures on Locally Convex Topological Vector Spaces . . . . . . 149 Perturbed Convolution Semigroups of Promeasures . . . . . . . . . . . . . 151 Quantum Dynamical Semigroups on CCR Algebras . . . . . . . . . . . . . 153 Example: Quantum Brownian Motion . . . . . . . . . . . . . . . . . . . . . . . . . 155

Outlook . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 157

References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 158

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Philippe Blanchard and Robert Olkiewicz

1 Physical and Mathematical Prologue 1.1 Physical Background Quantum mechanics, whose basic laws were formulated in the twenties, still remains the most fundamental theory we know. It describes, among other things, behavior of electrons in atoms, molecules and solids with astonishing accuracy. Since its appearance one has seen its remarkable successes and ever increasing range of applicability. There seems to be no limit to the Schrödinger equation and to the power of quantum theory as an incredibly accurate computational tool for physicists and chemists. However, quantum mechanics, when applied to the objects surrounding us, results in contradictions to what is observed. The question why those objects always appear localized and obey the laws of classical physics is in the center of this issue. The most transparent example illustrating that problem is a hypothetical experiment proposed by Schrödinger in 1935 which can be described briefly as follows [53]. A cat is penned up in a steel chamber, along with the following device. In a Geiger counter there is a tiny amount of radioactive substance, so small that perhaps in the course of one hour one of the atoms decays, but also, with equal probability, perhaps none. If it happens, the counter tube discharges and through a relay releases a hammer which shatters a small flask of hydrocyanic acid. If one has left the entire system to itself for one hour, one would say that the cat still lives if meanwhile no atom has decayed. The first atomic decay would have poisoned it.

Hence after one hour the system should be described by a schizophrenic quantum state which is a linear superposition over live and dead states of the cat. It is not a surprise that such an experiment caused some confusion among physicists. The first resolution of that paradox, advocated by Bohr, was to outlaw the use of quantum theory for the objects which are classical. He insisted on considering the interaction between a quantum object and apparatus described in classical terms as an indivisible whole and, consequently, claimed that atomic objects have no specific properties of their own and only factual phenomena exist. This orthodox Copenhagen interpretation places the emergence of a fact at the point where it is first registered by a classical measuring instrument. Such an interpretation had obviously several flaws. Firstly, it would have forced quantum theory to depend on classical physics for its very existence, and, secondly, it would have also meant that neither quantum nor classical theory were universal. Thus it was not convincing for some physicists. They could not accept the fact that quantum mechanics requires us to regard any question concerning the status of the cat as meaningless until we establish an observational relationship with it. For example, in a letter to Schrödinger in 1950 Einstein complained: Most of them simply do not see what sort of risky game they are playing with reality reality as something independent of what is experimentally established. Their interpretation

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is, however, refuted most elegantly by your system of radioactive atom + amplifier + charge of gun powder + cat in a box, in which the ψ-function of the system contains the cat both alive and blown to bits. Nobody really doubts that the presence or absence of the cat is something independent of the act of observation.

Less radical but going into the same direction was Heisenberg’s point of view on the subject. According to him, the physical world can be split into two parts, the observed object and the observing system which should be described in quantum and classical terms, respectively. Although such a recipe was useful, it was ambiguous in principle. Since there is no fundamental reason why the physics involved in measurements should differ from how other physical interactions are described, the very legitimacy of such a conceptual discontinuity and the precise location of its position, the so-called Heisenberg’s cut, was the crux of the issue. In contrast to that of Bohr and Heisenberg, the Dirac-von Neumann approach sought to solve the measurement riddle by invoking an additional axiom, known as the projection postulate. However, the wave function collapse as a dynamical transition from a pure state to a mixed state cannot be achieved by a unitary transformation. Hence, the hypothesis that at some stage during a measurement the Schrödinger evolution must be suspended and replaced by a different physical process whose detailed dynamics remains unspecified has some obvious flaws. Apart from the ad hoc way such a postulate is inserted to the theory, we are not told exactly at what point the collapse occurs or how long it takes [33, 45]. The reality of the reduction of the wave packet was discussed by Omnès who concluded: “Reduction is nothing but a convenient shortcut to avoid keeping track of all measurements by dealing explicitly with histories involving many outside devices, when one needs only to compute some probabilities. It has no physical content.” [44]. 1.2 Environmental Decoherence A different point of view was taken in a program of environment induced decoherence which emphasizes the role of an inevitable dissipative coupling of macrosystems with the surrounding environment. The aim of that program was to describe consequences of such openness of quantum systems to their environments and to study emergence of the effective classicality of some of the quantum states and of the associated observables. In recent years decoherence has received much attention and has been accepted as the mechanism responsible for the appearance of classicality in quantum measurements and the absence in the real world of Schrödinger-cat-like states [5, 29, 35, 47, 67]. It was also shown that decoherence is a universal short time phenomenon independent of the character of the system and its reservoir [15]. Decoherence is a dynamical effect taking place in a bulk of matter. It is most of the time extraordinary efficient and happens so quickly that it was extremely difficult to catch it [16, 34]. For that reason it is also the main obstacle for the experimental implementation of quantum state processing in quantum information theory. Nevertheless, the intuitive idea of environmental decoherence is rather clear: Quantum

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interference effects for macroscopic systems are practically unobservable because superpositions of their quantum states are rapidly destroyed by unavoidable interaction and entanglement with the surrounding environment. More precisely, it accepts the wave function description of such a system but contends that it is practically impossible to distinguish between vast majority of its pure states and the corresponding statistical mixtures. Moreover, the emergent localized wave packets at a macroscopic level obey classical dynamics because their spreading cannot occur since the coupling to the environment dominates the system’s internal quantum dynamics. It was summed up by Zeh who concluded: “All quasi-classical phenomena, even those representing reversible mechanics, are based on de facto irreversible decoherence” [66]. Decoherence therefore provides an answer, at least for all practical purposes, to one of the most difficult problems by which quantum mechanics was plagued for many years by taking advantage of the unavoidable entanglement of the system with its environment. However, in spite of the continuing progress in the theoretical and experimental understanding of this effect, its range of validity and its full meaning still need to be revealed [46, 50]. 1.3 Algebraic Framework Everybody agrees that concepts of classical and quantum physics are opposite in many aspects. Therefore, in order to discuss the emergence of classical behavior of quantum systems we need a single theory which allows a coherent description of quantum physics, classical mechanics and electrodynamics in the same mathematical language. A convenient framework for such a unified description is the formalism of algebraic quantum theory [3]. A recent presentation of this approach is given in [31]. It is a representation theory of the basic kinematical symmetry group and the associated canonical commutation or anticommutation relations. Its usefulness stems from the fact that it is valid for microscopic, mesoscopic and macroscopic systems with both finitely and infinitely many degrees of freedom. They may be purely quantal, purely classical or mixed (quantal with some classical properties). In this approach description of any individual physical system can be given in terms of an abstract unital C ∗ -algebra A [32]. A C ∗ -algebra is a topological algebra with an extraordinary property that its topology (the so-called norm topology) is determined algebraically and so does not depend on any experimental context [49]. It is believed that all intrinsic properties of a physical system can be represented by self-adjoint elements of A. A state of a system is represented by a positive linear functional ω on A such that ω(1) = 1, where 1 stands for the unit element in A. The set of all states we shall denote by S. A state ω is called faithful if ω(A∗ A) = 0 implies that A = 0. Algebraic quantum mechanics provides also mathematical tools for entering the traditional framework based on Hilbert space theory. For any faithful state ω ∈ S the so-called GNS representation (according to Gelfand, Naimark and Segal [13]) allows the construction of a Hilbert space Hω and a faithful representation πω : A → B(Hω ), the algebra of all bounded linear operators acting on Hω . In general, C ∗ -algebras admit an uncountable number of unitary inequivalent GNS


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representations, most of which presumably have no physical interpretation. Hence, in order to enter the traditional framework one has to select a subset Sa of admissible states, which through the GNS construction would lead to physically meaningful structures. The von Neumann algebra M = πω (A) , the bicommutant of πω (A), contains all physical observables of the system as its Hermitian operators or, more generally, self-adjoint operators affiliated to M. Generalizing the notion of a density matrix representing mixture of states in the traditional framework of quantum mechanics we say that density matrices (statistical states) of the system are represented by positive normal and normalized functionals on M. The set of density matrices we denote by D. Hence φ ∈ D iff φ(A) ≥ 0 whenever A ≥ 0, φ(1) = 1 and φ is continuous in the σ-weak topology on M. The linear space generated by D is a Banach space called the predual space of M and denoted by M∗ . The connection between a Hermitian operator A representing an observable and experimentally measured values of this observable, when the system is described by a density matrix φ, is obtained in following way. Suppose λdE(λ) is the spectral decomposition of A. The probability that the measured value is in an interval [a, b] is given by φ(E[a, b]), and so the expectation value of A in the state φ equals to < A > = λdφ(E(λ)). Let us observe that dφ(E(λ)) is a probability measure on σ(A), the spectrum of A. Genuine quantum systems are represented by factors, i.e. von Neumann algebras with a trivial center Z(M) = C · 1, whereas classical systems are described by commutative algebras. The triviality of the center expresses the fact that for any two orthogonal pure states their superpositions are physically distinguishable from the corresponding statistical mixtures [9]. Since a classical observable by definition commutes with all other observables so it belongs to the center of algebra M. Hence, the appearance of classical properties of a quantum system has to result in the emergence of an algebra with a nontrivial center, while transition from a factor to commutative algebra corresponds to the passage from purely quantum to classical description of the system. Since automorphic evolutions preserve the center of any algebra so this program may be accomplished only if we admit the loss of quantum coherence, i.e. that quantum systems are open and interact with their environment. 1.4 Quantum Dynamical Semigroups Generally, an open quantum system S can be described as a subsystem of the joint system S + E, where E denotes its environment. Guided by discussion in the previous subsection we associate with the system S + E a von Neumann algebra N acting in a Hilbert space HSE , and with S a von Neumann algebra M ⊂ B(HS ). Since S ⊂ S + E so there exists an injective normal ∗ -homomorphism i : M → N such that i(1) = 1. Hence the image i(M) is a von Neumann subalgebra in N . The joint system is assumed to be closed and so evolves in a reversible way. Physical examples indicate that a conservative dynamical system can be described, under quite general circumstances, by a triple (N , ψ, αt ), t ∈ R, where ψ is a faithful normal and semifinite weight on N and αt is a σ-weakly continuous one parameter group of ∗ -automorphisms of N such that ψ ◦ αt (A) = ψ(A) for all t ∈ R and all positive

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A ∈ N . Moreover, we assume that the weight φ on M given by φ = ψ ◦ i is also semifinite. We recall that a weight on a von Neumann algebra generalizes the notion of a state in the same way as the replacement of a compact space with a probability measure by a locally compact space with a σ-finite measure, for a broad discussion of weights see, for example, [58]. Dynamics of the system S is the reduced evolution obtained by tracing out the environmental degrees of freedom. Suppose that E : N → M is a ψcompatible conditional expectation (a normal projection of norm one which satisfies E ◦ i = id and ψ ◦ i ◦ E = ψ) of N onto M. Such a projection always exists if σtψ (i(M)) = i(M), where σtψ is the modular group of automorhisms corresponding to the weight ψ [58]. Then the evolution of the system S is given by Tt = E ◦ αt ◦ i, for t ≥ 0. Generalizing a bit the result of Emch and Varilly [22] one can show the following. Theorem 1. t → Tt is a σ-weakly continuous family of completely positive normal and norm contractive linear operators on M such that for any t ≥ 0 the following properties hold: (i) Tt (1) = 1, (ii) φ ◦ Tt (A) = φ(A) for all positive A ∈ M, (iii) Tt ◦ σsφ = σsφ ◦ Tt for all s ∈ R. We now say that the reduced dynamics (M, φ, Tt ) is Markovian if Tt ◦ Ts = Tt+s for all t, s ≥ 0. It is worth noting that operators Tt being defined as the composition of an automorphism with a conditional expectation satisfy in general a complicated integro-differential equation. However, for a large class of physical models one can derive, using certain limiting procedures, an approximated Markovian evolution Tt = etL , whose generator L is given by the so-called master equation [2, 17, 47]. In such a case we shall speak of quantum dynamical semigroups. Since operators Tt are normal so there exists a semigroup T∗ = (Tt∗ )t≥0 on the predual space M∗ also called a quantum dynamical semigroup. For a general discussion of these concepts see Rebolledo’s contribution in vol. II of this proceedings. In physical models one takes usually HSE = HS ⊗ HE , N = M ⊗ ME and i(A) = A ⊗ 1, A ∈ M. The conditional expectation E : N → M depends on a reference state ωE of the environment E and is given by φ(E(B)) = (φ ⊗ ωE )(B), B ∈ N , for all states φ ∈ D. The joint system evolves unitarily with the Hamiltonian H (a self-adjoint operator on HSE ) consisting of three parts H = HS ⊗ 1 + 1 ⊗ H E + H I ,

(1)

where HS describes the free evolution of the system, HE the free evolution of the environment, and HI describes the interaction between S and E. The reduced dynamics of the system is then given by Tt (A) = E(eitH (A ⊗ 1)e−itH ).

(2)

In the representation free framework of C ∗ -algebras we say that T = (Tt )t≥0 is a quantum dynamical semigroup on A if t → Tt is a C0 -semigroup of completely


123

positive and norm contractive linear operators on A such that Tt (1) = 1 for all t ≥ 0. It is worth noting that in a number of cases the assumption of the strong continuity of the semigroup T is too restrictive. Thus we also consider a weaker type of continuity and shall say that T is ω-continuous, ω ∈ S, if for all A ∈ A the mapping t → πω (Tt A) is continuous in the σ-weak topology on πω (A). 1.5 A Model of a Discrete Pointer Basis Before turning to a general description of decoherence let us first consider a well known physical example of environmentally induced pointer states. An analysis from the point of view of physics of mutually exclusive quantum states, the socalled privileged basis, was given in [68]. Suppose that • M = B(HS ), ME = B(HE ), where both HS and HE are separable, A ⊗ B, • HI = ∞ •A = n=1 λn Pn , λ ∈ R, minn =m |λn − λm | = δ > 0 and Pn are mutually orthogonal one-dimensional projections summing up to the identity operator, ∗ has an absolutely continuous spectrum, • B = B ∞ • HS = n=1 γn Pn , γn ∈ R, • [HE , B] = 0 (we say that two self-adjoint operators commute when their spectral measures commute), • ωE is an arbitrary statistical state of the environment represented by a density matrix ρ, i.e. a positive trace class operator with Trρ = 1. It is clear that A is self-adjoint and so is HI . Because all three terms in equation (1) commute so H is essentially self-adjoint on an appropriate domain and generates a one parameter unitary group eitH = eitHS ⊗1 eit1⊗HE eitHI . Let E be the conditional expectation from B(HS ) ⊗ B(HE ) onto B(HS ) with respect to the reference state ωE . Then, for any X ∈ B(HS ), Tt (X) = E[eitH (X ⊗ 1)e−itH ] = eitHS E[eitHI (X ⊗ 1)e−itHI ]e−itHS . Because eitHI =

∞

Pn ⊗ eitλn B

n=1

so Tt (X) =

∞

χn,m (t)eit(γn −γm ) Pn XPm ,

n,m=1

where χn,m (t) =

eit(λn −λm )s dTr(ρF (s)),

and dF (s) is the spectral measure of B. Since this measure is absolutely continuous so dTr(ρF (s)) is a probability measure absolutely continuous with respect to

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the Lebesgue measure. Hence, by the Riemann-Lebesgue lemma, χn,m ∈ C0 (R). Because minn =m |λn − λm | = δ > 0 so for any > 0 there exists t0 > 0 such that |χn,m (t)| < for all n = m and all t > t0 . The triple (B(HS ), Tr, Tt ), where Tr denotes the standard trace on B(HS ), satisfies all properties listed in Theorem 1 and hence represents the reduced dynamics of the system. Let us notice that in general the family of maps (Tt )t≥0 is not a semigroup. A Markov approximation when applied to this case would result in a special form of the correlation function χn,m (t), namely χn,m (t) = e−|λn −λm |t . Let ∞

Pˆ (B(HS )) : =

Pn B(HS )Pn ≡ l∞ (N).

n=1

We show now that all expectation values of any observable X ∈ B(HS ) such that Pˆ (X) = 0 decrease to zero uniformly on bounded sets. Suppose that X = (id − Pˆ )X, and X∞ ≤ 1. Then for any ρS ∈ D, |TrρS Tt (X)| ≤ Tt∗ ρS − Pˆ (Tt∗ ρS )1 X∞ ≤ Tt∗ ρS − Pˆ (Tt∗ ρS )1 , where · 1 is the trace norm and ∞

Tt∗ ρS =

χn,m (t)eit(γn −γm ) Pm ρS Pn .

n,m=1

Hence |TrρS Tt (X)| ≤

Pm ρS Pn χn,m (t)eit(γn −γm ) 1 .

n =m

Suppose first that ρS is a pure state associated with a unit vector from a dense subspace M of HS given by finite linear combinations of vectors |en > such that N P = |en >< en |, i.e. ρs = |f >< f |, where |f > = k=1 zk |ek > and nN 2 |z | = 1. Then k k=1 ρs =

N

z k zl |el >< ek |

k,l=1

and so |TrρS Tt (X)| ≤

N

z n zm χn,m (t)eit(γn −γm ) |em >< en | + h.c. 1

1=n<m

=

N 1=n<m

|zn ||zm ||χn,m (t)|Tr(Pn + Pm ) ≤

N

(|zn |2 + |zm |2 )|χn,m (t)|,

1=n<m

where h.c. stands for the Hermitian conjugate. Suppose that > 0 is given. Let us take t0 > 0 such that for all t > t0 , |χn,m (t)| < N −1 for all n = m. Then


|TrρS Tt (X)| ≤

125

N · (N − 1) |zn |2 = . N −1 n=1

If ρS is an arbitrary pure state, i.e ρS = |v >< v| with a unit vector v ∈ HS , then for any unit vector w ∈ HS $ |v >< v| − |w >< w| 1 ≤ 2 1 − | < v, w > |2 , see for example [62], and so for any > 0 there exists a unit vector f ∈ M such that ρS − |f >< f | 1 < . Hence (id − Pˆ )Tt∗ ρS 1 ≤ (id − Pˆ )Tt∗ (ρS − |f >< f |)1 +(id − Pˆ )Tt∗ (|f >< f |)1 < 3 for all t > t0 . Finally, suppose that ρS is an arbitrary statistical state. Then ∞ orthogonal one-dimensional projecρS = n=1 an Qn , where Qn are mutually ∞ tions summing up to the identity operator, and n=1 an = 1. Let N ∈ N be such N that ρS − ρ˜S 1 < , where ρ˜S = n=1 an Qn . By the previous step, for each (n) n ∈ {1, 2, ..., N } we can find t0 such that Tt∗ Qn − Pˆ (Tt∗ Qn )1 < for all (n) (n) t > t0 . Let t0 = max1≤n≤N t0 . Then for all t > t0 Tt∗ ρ˜S − Pˆ (Tt∗ ρ˜S )1 ≤

N

an Tt∗ Qn − Pˆ (Tt∗ Qn )1 < ,

n=1

and so Tt∗ ρS − Pˆ (Tt∗ ρS )1 < 3. This implies that lim Tt∗ ρS − Pˆ (Tt∗ ρS )1 = 0,

t→∞

and hence lim |TrρS Tt (X)| = 0,

t→∞

uniformly in X provided they belong to the unit ball. It means that for any experimental setup there exists a decoherence time td (usually very short) after which the expectation value of any observable X such that Pˆ (X) = 0 is beyond the experimental resolution. On the other hand, if Pˆ (X) = X, then Tt X = X for all t ≥ 0. Because any observable X ∈ B(HS ) can be written as X = Pˆ (X) + (id − Pˆ )(X) so we conclude that lim Tt (X) = Pˆ (X) t→∞

in the σ-weak topology. From the above example we can learn that there exists a decomposition of the von Neumann algebra M = B(HS ) of the system onto two parts M = M1 ⊕ M2 such that M1 = Pˆ (B(HS )) is a commutative von Neumann algebra with a trivial evolution on it, and M2 = (id − Pˆ )(B(HS )) is a Banach subspace whose

126


observables cannot be detected in practice. All projections Pn = |en >< en | belong to the algebra M1 and so do not evolve in time. However, any superpositions of the states |en > deteriorate to classical probability distributions over pure states Pn . Therefore such states have been termed classical quantum states [8]. In the next section we show that such a splitting is typical for the reduced dynamics of a quantum open system.

2 The Asymptotic Decomposition of T 2.1 Notation Since we have a considerable amount of mathematics to discuss in this section it is perhaps useful to describe briefly the general strategy. Guided by the above example our main objective here is to establish a decomposition M = M1 ⊕M2 , which we shall call the isometric-sweeping decomposition, under the most possible general assumptions (Section 2.2). To this end we, firstly, implement the dynamics in the associated Hilbert space, where the unitary-completely nonunitary decomposition holds (Section 2.3), next we extend this decomposition to the predual space, and finally that result will be transformed by duality to the algebra M (Section 2.4). We start with introducing the following notation. Let M be a von Neumann algebra with a distinguished normal semifinite and faithful weight φ. The predual space of M we shall denote by M∗ with the duality between M∗ and M given by ψ(x), ψ ∈ M∗ , x ∈ M. For any subset N ⊂ M we shall denote by Nh (respectively N+ ) the set of all Hermitian (respectively positive) operators from N . The same will apply for sets in M. We shall use the standard notation for objects associated with φ in the Tomita-Takesaki theory (because the weight φ is fixed we omit the subscript φ in notation) such as N = {x ∈ M : φ(x∗ x) < ∞}, M = span{y ∗ x : x, y ∈ N } = span{x ∈ M+ : φ(x) < ∞}, Λ the canonical injection of N into its Hilbert space completion H with the scalar product given by < Λ(x), Λ(y) > = φ(y ∗ x), x, y ∈ N , π the canonical representation of M in H being an isometry and a σ-weak homeomorphism of M onto π(M), ∆ the modular operator in H arising from the left Hilbert algebra U = Λ(N ∩ N ∗ ), J the corresponding isometric involution in H, and (σt )t∈R the group of modular automorphisms on M associated with φ. By S (respectively F ) we shall denote the corresponding sharp (respectively flat) operators in H, i.e. for any ξ ∈ DS , S(ξ) = ξ , and for any η ∈ DF , F (η) = η . By the same symbol π we shall denote the canonical faithful representation of U in B(H) given by π(ξ)η = ξη, ξ, η ∈ U. Thus, for any x ∈ N ∩ N ∗ , π(Λ(x)) = π(x). Definitions of all these concepts can be found for example in [56, 57]. The operator norm in M we shall denote by · ∞ , the norm in M∗ by · 1 , and the norm in H induced by the scalar product by · 2 . The operator norm in


127

B(H) will be denoted by · op . Thus π(x)op = x∞ for all x ∈ M. Because in the following we use operators acting in all spaces M, M∗ , and H so in order to avoid confusion we shall mark operators acting in M∗ with the subscript 1, and in H with the subscript 2. The closure of M in the operator norm we shall denote by C. Since M is a ∗ -algebra so C is a σ-weakly dense C ∗ -subalgebra in M. The classes of right (left) bounded elements in H we shall denote by U and U respectively, i.e. U = {η ∈ DF : ∃c > 0 π(ξ)η2 ≤ cξ2 ∀ξ ∈ U}, U = {ξ ∈ DS : ∃c > 0 π (η)ξ2 ≤ cη2 ∀η ∈ U }, where π (η)ξ = π(ξ)η, ξ ∈ U. Because algebra U is achieved so U = U . Finally, the injection of M into M∗ , x → φx , given by φx (u) =

n

< Jπ(u)∗ JΛ(yi ), Λ(zi ) >,

(3)

i=1

where x = i zi∗ yi , zi , yi ∈ N , and u ∈ M, we shall denote by Φ. As was shown in [63] φx is well defined, i.e. independent of the representation of x, and Φ is an injective linear positive map onto a norm dense subspace in M∗ . In the following we use also another expressions for φx given in [60]: φx (z ∗ y) = < Jπ(x)∗ JΛ(y), Λ(z) >, φx (y) = < Λ(y), JΛ(x) >, φx (y) = φy (x),

y, z ∈ N,

y ∈ N,

y ∈ M.

(4) (5) (6)

The closure of M in the norm xL = max{x∞ , φx 1 } we shall denote by L. As was shown in [60] Φ extends to an injection from L into M∗ . 2.2 Dynamics in the Markovian Regime Since the generalization to the time continuous case is straightforward we restrict our considerations to the discrete time case, i.e. we consider a semigroup (T n )n≥0 . Suppose that a bounded linear operator T : M → M satisfies the following assumptions: A1) T is two-positive, A2) T is normal with the predual T∗1 : M∗ → M∗ , A3) T (1) ≤ 1, where 1 is the identity operator in M, A4) φ ◦ T ≤ φ, i.e. φ(T x) ≤ φ(x) for all x ∈ M+ , A5) T ◦ σt = σt ◦ T ∀t ∈ R, A6) T∗1 preserves the space Φ(M ), i.e. T∗1 : Φ(M ) → Φ(M ). Let us comment on the above conditions. By Theorem 1, the first five of the above assumptions only generalize properties of the reduced dynamics. The last assumption is a technical one. It is a consequence of arbitrariness of the weight φ, and is superfluous in the case when φ is a tracial weight as we will see in Section 2.5.

128


Suppose that T satisfies A1-A6. Then, by A1 and A3, T satisfies the Schwarz inequality T (x)∗ T (x) ≤ T (x∗ x), and so is contractive in the operator norm. By the Schwarz inequality and A4, T : N → N . The map T2 Λ(x) = Λ(T x), x ∈ N , is contractive in · 2 , and so extends to the whole space H. This extension we denote also by T2 . By A4, T : M → M , and so the map T1 : Φ(M ) → Φ(M ) given by T1 (φx ) = φT x , x ∈ M , is well defined. Theorem 2. T1 extends to a linear two-positive and contractive operator on M∗ (denoted also by T1 ). Proof. Step 1. First we show that for any x ∈ M , T1 φx 1 ≤ 2φx 1 . If x ∈ Mh , then T x ∈ Mh , and so φT x 1 = inf{φ(h) + φ(k) : h − k = T x, h, k ∈ M+ } ≤ inf{φ(T y) + φ(T z) : y − z = x, y, z ∈ M+ } ≤ inf{φ(y) + φ(z) : y − z = x, y, z ∈ M+ } = φx 1 . The formula for the norm of φT x follows from the Remark on page 165 in [63]. Hence, using the Hermitian decomposition and the property φx∗ 1 = φx 1 , we arrive at φT x 1 ≤ 2φx 1 , for all x ∈ M . The bounded extension of T1 onto M1 we denote also by T1 . ˜ ≥ 0, Step 2. We show that Φ is completely positive. Suppose x ˜ ∈ M ⊗ Mn×n and x x) where Mn×n is the algebra of n × n matrices. A functional (φxij )i,j = Φ ⊗ id(˜ is positive on M ⊗ Mn×n if and only if for any y1 , ..., yn ∈ N there is n

φxij (yj∗ yi ) ≥ 0.

i,j=1

x) is positive so Let ξ˜ = (JΛ(y1 ), ..., JΛ(yn )) ∈ H ⊗ Cn . Because π ⊗ id(˜ ˜ ξ˜ > = < π ⊗id(˜ x)ξ,

n i,j=1

< Jπ(xij )∗ JΛ(yi ), Λ(yj ) > =

n

φxij (yj∗ yi ) ≥ 0.

i,j=1

Step 3. Because Φ is completely positive so T1 is two-positive. Hence the dual operator T1∗ : M → M is also bounded and two-positive. By step 1, T1 ψ1 ≤ ψ1 for all ψ ∈ M∗+ . Hence ψ(1) − ψ(T1∗ 1) ≥ 0, and so T1∗ 1 ≤ 1. Thus T1∗ satisfies the Schwarz inequality and so is contractive in the operator norm. Hence T1 ψ1 ≤ ψ1 for all ψ ∈ M∗ . 2 Let us next consider the dual operator T1∗ : M → M. Suppose that x ∈ M . Then, for any y ∈ M , φy (T1∗ x) = φT y (x) = φx (T y) = (T∗1 φx )(y). By Proposition 7 in [60], we infer that T1∗ x ∈ L and φT1∗ x = T∗1 φx . By assumption A6, T1∗ x ∈ M . If x ∈ M+ , then


129

$ $ φ(T1∗ x) = < Jπ(1)∗ JΛ( T1∗ x), Λ( T1∗ x) > = φT1∗ x (1) T1∗

= φT1∗ x 1 = T∗1 φx 1 ≤ φx 1 = φ(x),

and so φ ◦ ≤ φ. In particular, T1∗ : M → M and the map (T1∗ )1 (φx ) = φT1∗ x , x ∈ M , is well defined and extends to a bounded operator on M∗ . Let x ∈ M and y ∈ M. Then (T1∗ )1 (φx )(y) = φT1∗ x (y) = φx (T y) = (T∗1 φx )(y). Because Φ(M ) is norm dense in M∗ so (T1∗ )1 = T∗1 . This identification allows us to denote the operator T1∗ on M by T∗ . Using the same argument as for the operator T we obtain that operator T∗2 : Λ(N ) → Λ(N ), T∗2 Λ(x) = Λ(T∗ x), extends to a contraction on H which we denote also by T∗2 . Theorem 3. T2∗ = T∗2 , where T2∗ is the adjoint operator of T2 . Proof. Step 1. Suppose that x, y ∈ M . Then (T∗1 φx )(y) = φx (T y) = < T2 Λ(y), JΛ(x) > . On the other hand (T∗1 φx )(y) = φT∗ x (y) = < Λ(y), JT∗2 Λ(x) > . Because Λ(M ) is dense in H so JT∗2 J = T2∗ , and hence (T∗2 )∗ = JT2 J. Step 2. T2 : D(∆1/2 ) → D(∆1/2 ) and T2 ◦ ∆1/2 = ∆1/2 ◦ T2 |D(∆1/2 ) . Suppose x ∈ N ∩ N ∗ . Then π(∆it Λ(x)) = π(σt x). Hence ∆it Λ(x) ∈ U and ∆it Λ(x) = Λ(σt x). Thus, by assumption A5, T2 ∆it Λ(x) = Λ(T σt x) = Λ(σt T x) = ∆it T2 Λ(x). Because ∆it and T2 are contractions and U is dense in H so T2 ∆it = ∆it T2 . Let A = ln ∆ and let A = λdE(λ) be its spectral decomposition. Then T2 E(B) = E(B)T2 for any Borel set B ⊂ R. Because ∆1/2 = eλ/2 dE(λ), the assertion follows. Step 3. Suppose again that x ∈ N ∩ N ∗ . Then (T2 S)Λ(x) = (ST2 )Λ(x). Because S = J∆1/2 and D(∆1/2 ) = DS so (T2 J∆1/2 )Λ(x) = (J∆1/2 T2 )Λ(x) = (JT2 ∆1/2 )Λ(x). Because ∆1/2 Λ(x) = JΛ(x∗ ), the set ∆1/2 U is dense in H. Thus T2 J = JT2 and T∗2 J = JT∗2 . By step 1, T∗2 = T2∗ which completes the proof. 2 Summing up this subsection: In each space M, M∗ and H there is a pair of contractive (in the corresponding norms) operators T, T∗ : M → M

two-positive and normal,

T1 , T∗1 : M∗ → M∗

two-positive,

T2 , T∗2 : H → H,

(7) (8) (9)

such that T is dual to T∗1 , T∗ is dual to T1 , and T2 and T∗2 are adjoint in H. Moreover, both T and T∗ leave the space M invariant, and φ ◦ T ≤ φ,

φ ◦ T∗ ≤ φ.

(10)

130


2.3 The Unitary Decomposition of T2 m m Suppose S2,m = T∗2 T2 , m ∈ N, and let K m = {ξ ∈ H : S2,m ξ = ξ}. It is clear that K m is a closed linear subspace in H. If ξ ∈ K m and m ≥ 2, then

ξ2 = S2,m ξ2 ≤ T2m−1 ξ2 ≤ ξ2 . Hence T2m−1 ξ2 = ξ2 . Because S2,(m−1) ξ − ξ22 = S2,(m−1) ξ22 − 2T2m−1 ξ22 + ξ22 ≤ 0 so S2,(m−1) ξ = ξ. Thus (K m ) is a decreasing sequence of closed subspaces in H %∞ ∞ and we define K = m=1 K m . Let P2,m and P2 be the orthogonal projections in H onto K m and K ∞ respectively. It is well known, see for example [36], that for any ξ ∈ H, n−1 1 k P2,m ξ = lim S2,m ξ, n→∞ n k=0

and the limit exists in the norm in H. From step 3 in the proof of Theorem 3 we obtain that P2,m ◦ J = J ◦ P2,m , and P2 ◦ J = J ◦ P2 . Theorem 4. Suppose Sm = T∗m T m . Then, for any x ∈ M , the mean average limit converges σ-strongly∗ to a two-positive and contractive in the operator norm projection Pm : M → M , n−1 1 k Sm x. n→∞ n

Pm x = lim

k=0

Moreover, φ(Pm x) ≤ φ(x) for all x ∈ M+ . Proof. Let us define xn

n−1 1 k = Sm x, n k=0

ξn

n−1 1 k = Λ(xn ) = S2,m Λ(x). n k=0

Then xn ∈ M and ξn ∈ U. Let ξ = limn→∞ ξn = P2,m Λ(x). k k Λ(x)) = S2,m (Λ(x∗ )) so ξn converges in H. Step 1. ξ, ξ ∈ U. Because S(S2,m Since S is closed, ξ ∈ DS and ξn → ξ . Hence π(ξ) is affiliated to π(M). Suppose that η ∈ U . Then π (η)ξn 2 = π(ξn )η2 ≤ π(ξn )op η2 . However, π(ξn )op = xn ∞ ≤ x∞ . Hence π (η)ξn 2 ≤ x∞ η2 . Because ξn → ξ and π (η) is bounded so also π (η)ξ2 ≤ x∞ η2 . Thus π(ξ) is bounded which implies that ξ ∈ U. Replacing x by x∗ one may check in the same way that ξ ∈ U. Step 2. Let y = Λ−1 (ξ). Then xn → y in the σ-strong∗ topology. Since π : M →


131

π(M) is a homeomorphism with respect to the σ-strong∗ topology so it is sufficient to consider operators π(xn ) and π(y). Suppose that η ∈ U . Then π(xn )η − π(y)η2 = π (η)(ξn − ξ)2 → 0. Because π(xn )op ≤ x∞ and U is dense in H so π(xn ) → π(y) strongly. Since ξn → ξ ∈ U and π(xn )∗ η = ξn η, π(y)∗ η = ξ η for all η ∈ H, so π(xn ) → π(y) strongly∗ . In particular, π(y)op ≤ x∞ . Since σ-strong∗ and strong∗ topologies coincides on bounded sets, the assertion follows. n−1 k Step 3. y ∈ M . Suppose that z ∈ M and let zn = n1 Sm z. Then k=0

|φz (y)| = | < Λ(y), JΛ(z) > | = | < P2,m Λ(x), JΛ(z) > | = | < Λ(x), JP2,m Λ(z) > | = lim | < Λ(x), JΛ(zn ) > | = lim |φzn (x)| n→∞

n→∞

= lim |φx (zn )| ≤ φx 1 z∞ . n→∞

Hence, by Corollary 17 in [60], y ∈ L. Because x = x1 − x2 + i(x3 − x4 ), where xj ∈ M+ , so yj := Λ−1 (P2,m xj ) ∈ L+ , and (xj )n → yj σ-strongly. Since the weight φ is σ-weakly lower continuous, φ(yj ) ≤ lim inf φ((xj )n ). However, by formula (10), n−1 1 k φ(Sm xj ) ≤ φ(xj ). φ((xj )n ) = n k=0

Hence yj ∈ M+ and so, by linearity, y ∈ M . Step 4. Finally, let us define a map Pm : M → M , by Pm x = Λ−1 (P2,m Λ(x)). Then Pm is a positive and contractive in the operator norm projection such that Pm x = limn→∞ xn in the σ-strong∗ topology. Moreover, φ(Pm x) ≤ φ(x) for all ˜ = M ⊗ M2×2 x ∈ M+ . Thus only two-positivity remained to be shown. Let M ˜ and let φ = φ ⊗ Tr, where Tr is the standard trace on M2×2 , the algebra of 2 × 2 matrices. Replacing T and T∗ by T˜ = T ⊗ id and T˜∗ = T∗ ⊗ id, and m ˜m T2 is contractive in the corresponding Hilbert space and noting that S˜2,m = T˜∗2 m ˜m ˜ ˜ ˜ = M ⊗ M2×2 , we conclude that Pm ⊗ id is posiSm = T∗ T is positive on M tive, and so Pm is two-positive. 2 Suppose now that x, y ∈ M . Then φPm x (y) = < Λ(y), JP2,m Λ(x) > = < Λ(Pm y), JΛ(x) > = φx (Pm y) (11) because P2,m commutes with J. Using the above property we define a contractive projection P1,m on M∗ as follows. Let P1,m φx = φPm x , x ∈ M . Then P1,m φx 1 =

sup y∈M,y∞ ≤1

|φPm x (y)| =

sup y∈M,y∞ ≤1

|φx (Pm y)| ≤ φx 1 .

Because Φ(M ) is norm dense in M∗ so P1,m extends to a two-positive contractive ∗ : M → M be the dual projection on M∗ which we denote also by P1,m . Let P1,m

132


∗ projection. By formula (11), P1,m |M = Pm . Hence there exists a unique extension of Pm to a two-positive normal and contractive in the operator norm projection on M which we denote also by Pm . Using the properties of projections P2,m and the fact that P2 ξ = limm→∞ P2,m ξ one may show in the same way as above the existence of a two-positive and contractive (in the corresponding norms) projections P1 : M∗ → M∗ , and its dual P : M → M associated with the orthogonal projection P2 in H. Two-positivity follows actually from the fact that for all x ∈ M , Pm (x) → P (x) in the σ-strong∗ topology, and so 2 i,j=1

yj∗ P (x∗j xi )yi = lim ( m→∞

2

yj∗ Pm (x∗j xi )yi ) ≤ 0

i,j=1

for any xi , yi ∈ M , i = 1, 2. It is also clear that P : M → M and φ ◦ P ≤ φ. For x ∈ M , P x is given by P x = Λ−1 (P2 Λ(x)). m P2 , m ∈ N. Clearly, R2,m is a contraction Suppose now that R2,m = P2 T2m T∗2 in H, and let Km be its fixed point space, i.e. Km = {ξ ∈ H : R2,m ξ = ξ}. Then Km+1 ⊂ Km ⊂ K ∞ . Let K =

∞ %

Km .

m=1 for T2 . ∞

Proposition 5. K is a unitary space Proof. Suppose ξ ∈ K. Because ξ ∈ K so T2m ξ2 = ξ2 for all m ∈ N. m P2 ξ2 = ξ2 . However, P2 ξ = ξ and T∗2 = T2∗ which Because ξ ∈ Km so T∗2 ∗m implies that T2 ξ2 = ξ2 for all m ∈ N. Conversely, suppose that for all m m m T2 ξ = T2m T∗2 ξ = ξ, m ∈ N there is T2m ξ2 = T2∗m ξ2 = ξ2 . Then T∗2 and so P2 ξ = ξ which implies that R2,m ξ = ξ. Hence ξ ∈ K. 2 Let Q2,m and Q2 be the orthogonal projections of H onto Km and K respectively. Let Rm = P T m T∗m P . Since operators Rm : M → M possess the same properties as Sm , so by repeating the arguments of Theorem 4 and the discussion after it we arrive at the following result which we state without a proof. Theorem 6. There are two-positive and contractive (in the corresponding norms) projections Q1 : M∗ → M∗ and its dual Q : M → M, and an orthogonal projection Q2 from H onto K such that ∀x ∈ M,

(12)

∀x ∈ N ∩ N ∗ ,

(13)

φ ◦ Q ≤ φ.

(14)

Q1 Φ(x) = Φ(Qx) Q2 Λ(x) = Λ(Qx) Q: M →M

and

Proposition 7. Q(1) ≤ 1. Q(1) = 1 if and only if the projection Q is φcompatible. Proof. Assume that Q(1) = 1. Then, for any x ∈ M+ , φ(Qx) = φQx (1) = (Q1 φx )(1) = φx (Q(1)) = φx (1) = φ(x).


133

Moreover, φ|Q(M) is semifinite. Conversely, suppose that φ(Qx) = φ(x) for all x ∈ M+ . Then φx (Q(1)) = φx (1) for all x ∈ M . Since Φ(M ) is norm dense in M∗ , the assertion follows. The inequality Q(1) ≤ 1 follows from formula (14). 2 2.4 The Isometric-Sweeping Decomposition We start with the following observation. Proposition 8. QT = T Q, QT∗ = T∗ Q, Q1 T1 = T1 Q1 ,

Q1 T∗1 = T∗1 Q1 .

Proof. By duality, it is sufficient to check only the first line. But this follows from the property Q2 T2 = T2 Q2 (since K is the unitary space for T2 ), formula (13), the fact that all three operators Q, T and T∗ are normal maps, and M is σ-weakly dense in M. 2 We are now in a position to formulate our main results. Theorem 9. M∗ = M∗1 ⊕ M∗2 , where M∗1 and M∗2 are norm closed T∗1 and T1 -invariant ∗ -subspaces. The restriction of T1 to M∗1 is an invertible isometry and T∗1 |M∗1 is its inverse. For any ψ ∈ M∗2 and all x ∈ C there is n lim (T1n ψ)(x) = lim (T∗1 ψ)(x) = 0.

n→∞

n→∞

(15)

n If {T∗1 } is relatively compact in the strong operator topology, then n lim T∗1 ψ1 = 0

n→∞

(16)

for all ψ ∈ M∗2 . n ψ)(e) → Remark. If ψ ∈ M∗2 , then for any φ-finite projection e ∈ M we have (T∗1 0, which justifies the name of sweeping. M∗1 is called the isometric part. Proof. Let M∗1 be the image of projection Q1 and let M∗2 = {ψ − Q1 ψ : ψ ∈ M∗ }. The first part of the theorem is clear. If x ∈ M and Qx = x, then Λ(T∗ T x) = T∗2 T2 Λ(x) = Λ(x) = Λ(T T∗ x). Hence T∗ T x = T T∗ x = x, and so T∗1 T1 φx = T1 T∗1 φx = φx . Because the space {φx : Qx = x} is norm dense in M∗1 so T∗1 |M∗1 T1 |M∗1 = T1 |M∗1 T∗1 |M∗1 = id|M∗1 . Since both T1 and T∗1 are contractive, they are isomet⊥ ric operators on M∗1 . Suppose now that x, z ∈ M . Then, Q⊥ 2 Λ(x) ∈ K , the completely nonunitary subspace for T2 , and so (T1n (φx − Q1 φx ))(z) = (T1n φx−Qx )(z) = < Λ(z), JΛ(T n (x − Qx)) > = < Λ(z), JT2n Q⊥ 2 Λ(x) > → 0

134


when n → ∞. The case of T∗1 may be handled in the same way. Since the space {φx − Q1 φx } is norm dense in M∗2 , and M is norm dense in C, the formula (15) n } is relatively compact in the strong operator follows. Finally, suppose that {T∗1 n ψ}∞ topology. Then, for any ψ ∈ M∗2 , the set {T∗1 0 is relatively compact in the norm topology in M∗ . Let ψ0 be a strong accumulation point of this set. Then there exists a subsequence (mn ) of natural numbers such that mn lim T∗1 ψ − ψ0 1 = 0.

n→∞

mn ψ)(x) → ψ0 (x). By formula (15), ψ0 (x) = 0. HowHence, for any x ∈ M , (T∗1 mn ψ1 → 0. ever, ψ0 is normal and M is σ-weakly dense in M so ψ0 = 0. Thus T∗1 Since T∗1 is norm contractive, the formula (16) follows, and the proof is complete. 2

By duality, one can obtain a similar decomposition of the algebra M. Theorem 10. M = M1 ⊕ M2 , where M1 is a σ-weakly closed ∗ -subalgebra and M2 is a σ-weakly closed linear ∗ -subspace in M. Both M1 and M2 are T and T∗ -invariant. The restriction of T to M1 is a ∗ -automorphism, whereas lim ψ(T n x) = 0

n→∞

(17)

n } is relatively for all ψ ∈ M∗ and all x ∈ M2 ∩ C. If the predual semigroup {T∗1 compact in the strong operator topology, then

lim ψ(T n x) = 0

n→∞

(18)

for all x ∈ M2 , uniformly on bounded sets in M2 . If M1 = 0, then the projection from M onto M1 is a conditional expectation, and it is a φ-compatible conditional expectation whenever 1 ∈ M1 . Proof. Let M1 = {Qx : x ∈ M} and let M2 = {x − Qx : x ∈ M}. Because projection Q is two-positive normal and commutes with both T and T∗ so the decomposition of M follows. To proceed further we first show that M1 = {Qx : x ∈ M } is a ∗ -algebra. By linearity, it is sufficient to check that x∗ x ∈ M1 whenever x ∈ M1 . Suppose that x ∈ M1 . Then Q(x) = x and Q(x∗ ) = x∗ . By Proposition 7 and two-positivity, projection Q satisfies the Schwarz inequality. Hence Q(x∗ x) ≥ Q(x∗ )Q(x) = x∗ x, and so φ(Q(x∗ x)) ≥ φ(x∗ x). On the other hand φ(Q(x∗ x)) ≤ φ(x∗ x). Thus φ(Q(x∗ x) − x∗ x) = 0 and so, by faithfulness of φ, Q(x∗ x) = x∗ x. Hence x∗ x ∈ M1 which implies that M1 is a ∗ -algebra. Since M1 is a σ-weak closure of of M1 , it is also a ∗ -algebra. Because T (x∗ x) ≥ (T x)∗ T x so, for any x ∈ M1 , 0 ≤ φ(T (x∗ x)) − φ((T x)∗ T x) ≤ Λ(x)22 − T2 Λ(x)22 = 0. Hence, by faithfulness of φ, T (x∗ x) = (T x)∗ T x. This implies that for any ψ ∈ M∗+ , the positive form b on M given by b(x, y) = ψ(T (x∗ y) − T (x∗ )T (y)),


135

vanishes on M1 . Because ψ was arbitrary we conclude that T (xy) = T (x)T (y) for all x, y ∈ M1 . However, σ-weak continuity of T implies that T (xy) = T (x)T (y) for all x, y ∈ M1 . If x ∈ M1 , then Q(x∗ x) = x∗ x, and so T∗ T (x∗ x) = T T∗ (x∗ x) = x∗ x. Again, by σ-weak continuity of T and T∗ , this equality holds for all x ∈ M1 . Thus T |M1 is a ∗ -automorphism. If y ∈ M2 ∩C, then formula (15) n ) is relatively compact in the strong operator yields (17). Finally, suppose that (T∗1 topology. Then, by formula (16), for any y ∈ M2 with y∞ ≤ 1, and all ψ ∈ M∗ there is n lim |ψ(T n y)| = lim |ψ(T n (id − Q)y)| = lim |(T∗1 (id − Q1 )ψ)(y)|

n→∞

n→∞

n→∞

n ≤ lim T∗1 (id − Q1 )ψ1 = 0 n→∞

since (id − Q1 )ψ ∈ M∗2 . If M∗1 = 0, the Q is a norm one projection, and so it is a conditional expectation onto the algebra M1 . If 1 ∈ M1 , then M1 is a von Neumann algebra, i.e. M1 = M1 , and, by Proposition 7, Q is a φ-compatible conditional expectation onto M1 . 2 It is worth noting that this result is optimal in the following sense. There exists a σ-weakly continuous semigroup of operators on B(HS ) satisfying A1-A6 and such that M1 = 0, M2 = B(HS ), ψ(Tt x) → 0 for all ψ ∈ Tr(HS ) and all x ∈ K(HS ), and ψ(Tt 1) = 1 for all t ≥ 0 [7]. Here Tr(HS ) is the Banach space of trace class operators, the predual space to B(HS ), and K(HS ) stands for the C ∗ -algebra of compact operators. 2.5 Remarks Assumptions A1-A6 are necessary if one wants to consider arbitrary von Neumann algebras, especially those of type III. In special cases they may be simplified. Proposition 11. Suppose M is a semifinite von Neumann algebra, i.e. of type I or II, with a faithful normal and semifinite trace τ . Suppose further that operator T : M → M satisfies assumptions A1-A4 with φ = τ . Then A5 and A6 follows. Proof. Since φ = τ , σt = id. Hence only assumption A6 needs to be shown. By A4, T x1 = τ (T x) ≤ τ (x) = x1 , if x ∈ M+ . Hence T is bounded in the norm · 1 and so extends to a bounded operator T1 on M∗ = L1 (M). Let T1∗ : M → M be the dual operator. Clearly, T1∗ is also two-positive. Moreover, for any ψ ∈ L1+ (M), ψ(T1∗ 1) = (T1 ψ)(1) = T1 ψ1 ≤ ψ1 = ψ(1), which implies that T1∗ (1) ≤ 1. Hence T1∗ satisfies the Schwarz inequality and so is contractive in the operator norm. Thus T1 is contractive in the · 1 norm. Suppose now that x ∈ M+ . Then, for any y ∈ M, Φ(x)(y) = < Jπ(y)∗ JΛ(x1/2 ), Λ(x1/2 ) > = τ (xy) ≡ τx (y).

136


So, by linearity, Φ(x) = τx for all x ∈ M . By Proposition 1 in [65], τ (T1∗ x) ≤ τ (x), for all x ∈ M+ , and so T1∗ : M → M . Because Φ(T1∗ x) = T∗1 Φ(x), for all x ∈ M , so T∗1 : Φ(M ) → Φ(M ). 2 The above decomposition M = M1 ⊕ M2 (called the isometric-sweeping decomposition) is obviously related to the asymptotic properties of the semigroup (T n ). Such properties for positive or completely positive semigroups having a faithful normal stationary state (or a faithful family of subinvariant normal states) have been studied by many authors. For example, in [24] and [40] the problem of the approach to equilibrium was addressed. See also the contribution of Fagnola and Rebolledo in this volume. In [26, 30, 37, 64, 65] the existence of the mean ergodic projection on a von Neumann algebra M was considered. Such a projection being a conditional expectation onto the fixed point subalgebra MT provides another decomposition, namely M = MT ⊕ N , with the obvious inclusion MT ⊂ M1 . However, the evolution restricted to MT is trivial, while on M1 it is given by a group of automorphisms. Moreover, the restriction of the dynamics to N cannot be controlled in general. For a partial result in this direction see [25]. From this point of view the isometric-sweeping decomposition for states (see Theorem 9) is closer to the so-called Jacobs-deLeeuw-Glicksberg splitting onto the so-called reversible and flight parts which holds whenever the semigroup is relatively compact in the weak operator topology, see for example [36]. However, in such a case there is no clear physical interpretation of the flight vectors which are characterized by the property that 0 is a weak accumulation point of their trajectory. It should be also pointed out that the isometric-sweeping decomposition may exist, even when the JacobsdeLeeuw-Glicksberg splitting fails to hold [43]. This is due to the fact that our assumption A4 about the existence of a subinvariant faithful normal weight, contrary to the existence of a subinvariant faithful normal state, has no direct topological consequences for the semigroup (T n ) or its predual. However, in a special case of M = B(HS ), M∗ = Tr(HS ) and φ = Tr, if the Jacobs-deLeeuw-Glicksberg splitting exists, then it coincides with the isometric-sweeping decomposition. To this end, let us define Tr(HS )r = Lin{ψ ∈ Tr(HS ) : T∗1 ψ = eiα ψ for some α ∈ R} and n Tr(HS )0 = {ψ ∈ Tr(HS ) : 0 is a weak limit point of {T∗1 ψ}},

where T∗1 is the predual operator of T , see assumption A2. The Jacobs-deLeeuwGlicksberg theorem states that if T∗1 is relatively compact in the weak operator topology, then Tr(HS ) = Tr(HS )r ⊕ Tr(HS )0 . Theorem 12. Suppose M = B(HS ) and assumptions A1-A4 hold with φ = Tr. If T∗1 is relatively compact in the weak operator topology, then Tr(HS )1 = Tr(HS )r and Tr(HS )2 = Tr(HS )0 .


137

Proof. By Proposition 11, all assumptions A1-A6 are satisfied and so the isometricsweeping decomposition takes place. To prove the theorem we proceed by steps. Step1. Tr(HS )r ⊂ Tr(HS )1 . Suppose T∗1 ψ = eiα ψ, ψ ∈ Tr(HS ). Then also T∗2 ψ = eiα ψ, where T∗2 : HS(HS ) → HS(HS ), and HS(HS ) stands for the Hilbert space of Hilbert-Schmidt operators acting on HS . Hence ∗ ∗ ∗ ψ22 = ψ22 − < e−iα ψ, T∗2 ψ >HS − < T∗2 ψ, e−iα ψ >HS e−iα ψ − T∗2 ∗ + T∗2 ψ22 ≤ 0 ∗ and so T∗2 ψ = e−iα ψ. Therefore, by Proposition 5, ψ ∈ K and hence ψ ∈ Tr(HS )1 . Step 2. By the very construction, Tr(HS )1 ⊥Tr(HS )2 in the following sense: Tr(ψ1 ψ2 ) = 0 for all ψ1 ∈ Tr(HS )1 and all ψ2 ∈ Tr(HS )2 . We show that Tr(HS )r ⊥Tr(HS )0 also. Since T2 and T∗2 are contractions in HS(HS ), so both n } are wo-relatively compact in B(HS(HS )). Let T2 (T2∗ ) denote {T2n } and {T∗2 n }) in B(HS(HS )) and the closure in the weak operator topology of {T2n }({T∗2 ∗ ˜ 2 ) be the unit in the kernel of T2 (T ), respectively. Since (T2 )∗ = T ∗ so Q2 (Q 2 2 ˜ 2 = Q∗ . However, the reversible parts of T2 and T∗2 in HS(HS ) coincide, hence Q 2 ˜ 2 = imQ∗ . Because Q2 = Q2 , Q∗2 = Q∗ , so Q∗ Q2 = Q2 and imQ2 = imQ 2 2 2 2 2 ∗ ∗ Q2 Q2 = Q2 . Therefore (Q2 − Q∗2 )2 = 0 which implies that Q2 = Q∗2 . Thus, for any x ∈ HS(HS )r and y ∈ HS(HS )0 we have

< x, y >HS = < Q2 x, (id − Q2 )y >HS = 0 However, Tr(HS )r ⊂ HS(HS )r and Tr(HS )0 ⊂ HS(HS )0 , hence the assertion follows. Moreover, if ψ ∈ Tr(HS ) and ψ⊥Tr(HS )r , then ψ ∈ Tr(HS )0 . To prove this suppose that ψ = ψ1 + ψ2 , where ψ1 ∈ Tr(HS )r and ψ2 ∈ Tr(HS )0 . By the assumption, TrψTr(HS )r = 0. Because ψ1∗ ∈ Tr(HS )r , where ψ ∗ stands for Hermitian conjugate, and Trψ2 ψ1∗ = 0, so Trψ1 ψ1∗ = 0. Hence ψ1 = 0. n ψ}n≥0 is relatively compact for any ψ ∈ Tr(HS ) in Step 3. A set Kψ = {T∗1 ˇ the weak topology on Tr(HS ). Suppose that ψ ≥ 0. By the Eberlein-Smulian theorem Kψ is weakly sequentially compact. Let {ψm } be an arbitrary sequence in Kψ . Then there exists a subsequence {ψmn } such that w-lim ψmn = ψ0 , where ψ0 ∈ Tr(HS )+ . However, ψmn ∈ Tr(HS )+ so, by Corollary 5.11 in [59], limn→∞ ψmn − ψ0 1 = 0. This implies that Kψ is sequentially compact, and so it is relatively compact in the trace norm topology. Suppose now that ψ ∈ Tr(HS ). Then ψ = ψ1 − ψ2 + iψ3 − iψ4 , where all ψj ∈ Tr(HS )+ . Each set Kj = n ψj }n≥0 is relatively compact. Because the function f (ψ1 , ψ2 , ψ3 , ψ4 ) = {T∗1 ψ1 − ψ2 + iψ3 − iψ4 , ψj ∈ Tr(HS )+ , is norm continuous so the set f (×Kj ) n ψ ∈ f (×Kj ), which implies is compact in Tr(HS ). However, for all n ≥ 0, T∗1 n that Kψ is compact. Hence, the semigroup (T∗1 ) is relatively compact in the strong operator topology. n ψ1 = 0. Because Step 4. By Lemma 4.2 in [42], for any ψTr(HS )0 , limn→∞ T∗1 ψ ∈ Tr(HS )2 ⇒ TrψTr(HS )1 = 0 and, by step 1, Tr(HS )r ⊂ Tr(HS )1 so ψ ∈ Tr(HS )2 ⇒ TrψTr(HS )r = 0 ⇒ ψ ∈ Tr(HS )0 .

138


The last implication follows from step 2. Hence Tr(HS )2 ⊂ Tr(HS )0 . Suppose / Tr(HS )2 . now that Tr(HS )2 = Tr(HS )0 . We take ψ ∈ Tr(HS )0 such that ψ ∈ Let ψ = ψ1 + ψ2 be its isometric-sweeping decomposition, i.e. ψ1 ∈ Tr(HS )1 and ψ2 ∈ Tr(HS )2 with ψ1 = 0. Then ψ1 = ψ − ψ2 ∈ Tr(HS )0 and n n ψ1 1 = 0. On the other hand, by Theorem 9, T∗1 ψ1 1 = so limn→∞ T∗1 ψ1 1 > 0, the contradiction. Therefore Tr(HS )2 = Tr(HS )0 . Thus equality Tr(HS )r = Tr(HS )1 also holds. 2 In the next section we illustrate these general results by physically motivated examples.

3 Review of Decoherence Effects in Infinite Spin Systems 3.1 Infinite Spin Systems The ideal infinite quantum spin system S consists of an array of noninteracting spin1 2 particles fixed at positions n = 1, 2, ... and exposed to a magnetic field. The algebra M of its bounded observables is given by the σ-weak closure of π0 (⊗∞ 1 M2×2 ), where π0 is a (faithful) GNS representation with respect to a tracial state tr on the Glimm algebra ⊗∞ 1 M2×2 , and M2×2 is the algebra generated by Pauli matrices. It is worth pointing out that such a tracial state corresponds to the infinite temperature case. Let us also point out that M is not a ”big” matrix algebra. It is a continuous algebra (factor of type II1 ) in which there are no pure normal states. In fact, any projection e ∈ M contains a nontrivial subprojection f ∈ M. It is worth noting that the absence of minimal projections is a new feature which may be present only in systems in the thermodynamic limit. Since the algebra M is a finite factor so the theorem about the isometric-sweeping decomposition can be strengthen in the following way. Theorem 13. Suppose that a σ-weakly continuous semigroup (Tt )t≥0 , Tt : M → M, satisfies: A1) Tt are two-positive, A3) Tt (1) ≤ 1, A4) tr ◦ Tt ≤ tr, see Section 2.2. Then M = M1 ⊕ M2 , where (i) M1 is a von Neumann subalgebra of M and the evolution Tt when restricted to M1 is reversible, given by a one parameter group of ∗ -automorphisms of M1 . (ii) M2 is a linear space (closed in the norm topology) such that for any observable B = B ∗ ∈ M2 and any statistical state ρ ∈ M∗ of the system there is lim Tt Bρ = 0,

t→∞

(19)

where Aρ = tr(ρA) stands for the expectation value of an observable A in the state ρ. Proof. Using the same argument as in the proof of Proposition 11 one can show that


139

all Tt can be extended to contractive operators (Tt )1 on M∗ = L1 (M). Their dual operators (Tt )∗1 : M → M also satisfy A1, A3 and A4. Because M ⊂ L1 (M) so for any A, B ∈ M, tr[((Tt )∗1 )∗1 A]B = trA[(Tt )∗1 B] = tr(Tt A)B. Since M is dense in L1 (M) in the · 1 -norm so ((Tt )∗1 )∗1 = Tt . Hence Tt are normal operators. By Proposition 11, operators Tt satisfy all assumptions A1-A6 from Section 2.2, and so the isometric-sweeping decomposition follows. Finally, we prove the equation (19). Suppose that ψ ∈ L2 (M) ⊂ L1 (M), where L2 (M) denotes the Hilbert space of square summable with respect to the trace tr operators [54]. From the very definition of the sweeping part it follows that for any B ∈ M2 , lim tr(ψTt B) = 0.

t→∞

Because for any φ ∈ L1 (M) and any > 0 there exists ψ ∈ L2 (M) such that φ − ψ1 < so |tr(φTt B)| ≤ B + |tr(ψTt B)|. Hence limt→∞ |tr(φTt B)| ≤ B. Since was arbitrary, the proof is complete. 2 The above result means that any observable A of the system may be written as a sum A = A1 + A2 , Ai ∈ Mi , i = 1, 2, and all expectation values of the second term A2 are beyond experimental resolution after the decoherence time. Therefore, if decoherence is efficient then almost instantaneously what we can observe are observables contained in the subalgebra M1 . In other words we apply Borel’s 0th axiom: Events with very small probability never occur. Hence all possible outcomes of the process of decoherence can be directly expressed by the description of this subalgebra and its reversible time evolution. 3.2 Continuous Pointer States [10] Suppose that the infinite spin system S described by the algebra M (see the previous subsection) interacts with its environment E. The reservoir is chosen to consists of noninteracting phonons of an infinitely extended one dimensional harmonic crystal 1 . The Hilbert space H representing pure states of at the inverse temperature β = kT a single phonon is (in the momentum representation) H = L2 (R, dk). A phonon energy operator is given by the dispersion relation ω(k) = |k| ( = 1, c = 1). It follows that the Hilbert space of the reservoir is F ⊗ F, where F is the symmetric Fock space over H. A phonon field φ(f ) = √12 (a∗ (f ) + a(f )), where a∗ (f ) and a(f ) are given by the Araki-Woods representation [4]: a∗ (f ) = a∗F ((1 + ρ)1/2 f ) ⊗ I + I ⊗ aF (ρ1/2 f ),

(20)

a(f ) = aF ((1 + ρ)1/2 f ) ⊗ I + I ⊗ a∗F (ρ1/2 f ).

(21)

140


Here a∗F (aF ) denotes respectively creation (annihilation) operators in the Fock space, and ρ is the thermal equilibrium distribution related to the phonons energy according to the Planck law ρ(k) =

1 . eβω(k) − 1

Since the phonons are noninteracting, their dynamics is completely determined by operator HE = H0 ⊗ I − I ⊗ H0 , where H0 = dΓ (ω) = the energy ω(k)a∗F (k)aF (k)dk describes the dynamics of the reservoir at zero temperature. The reference state of the reservoir is taken to be a gauge-invariant quasi-free thermal state given by ∗ ρ(k)g(k)f (k)dk. ωE (a (f )a(g)) = Clearly, ωE is invariant with respect to the free dynamics of the environment. The joint system S + E evolves unitarily with the Hamiltonian H consisting of three parts (22) H = H S ⊗ 1 + 1 ⊗ H E + HI . We assume that HS = 0 and that the coupling between the system and the environment is linear, i.e. HI = λQ ⊗ φ(g), where &∞ ' 1 3 , (23) σ Q = π0 2n n n=1 σn3 is the third Pauli matrix in the n-th site, and λ > 0 is a coupling constant. The factor 21n in equation (23) reflects the property that interaction between spin particles and the reservoir decreases as n → ∞. Its form was chosen to simplify further calculations. The test function g(k) = |k|1/2 χ(k), where χ(k) is an even and real valued function such that: (i) χ is differentiable with bounded derivative, C , C > 0, > 0, (ii) for large |k|, |χ(k)| ≤ k2+ and χ(0) = 1. The behavior of the test function g at the origin and the asymptotic bound (ii) are taken to ensure that H is essentially self-adjoint. Properties (i) and (ii) will also secure that the two-point thermal correlation function of the field operator is integrable. The reduced dynamics of an observable X ∈ M is given by Tt (X) = Π ωE (eitH (X ⊗ I)e−itH ),

(24)

where Π ωE is a conditional expectation (the dual operation to the partial trace) with respect to the reference state ωE of the reservoir. Because the thermal correlation function φt (g)φ(g) = ωE (eitHE φ(g)e−itHE φ(g)) = ωE (φ(eitω g)φ(g))


141

is integrable, we use the so-called singular coupling limit [2, 48] which states that Tt = etL is a quantum Markov semigroup with the generator L given by a master equation in the standard (Gorini-Kossakowski-Sudershan-Lindblad) form L(X) = ib[X, Q2 ] + λa(QXQ −

1 2 {Q , X}). 2

(25)

Parameters a > 0 and b ∈ R are determined by ∞ < φt (g)φ(g) > dt =

a + ib. 2

(26)

0

Direct calculations show that √ < φt (g)φ(g) > = 2πF(f1 )(t) +

√ √ 2π 2π F(f2 )(t) + F(f3 )(t), 2 2

where f1 (k) =

|k|χ2 (k) , eβ|k| − 1

f2 (k) = |k|χ2 (k),

f3 (k) = kχ2 (k),

and F stands for the Fourier transform. Hence, by the inverse Fourier formula, one has 2π , (27) a = 2πf1 (0) + πf2 (0) = β and

√ ∞ ∞ d 2π 2 F (χ )(t) dt = − χ2 (k)dk. b = 2 dt 0

(28)

0

The master equation (25) consists of two terms. The first one is a Hamiltonian term HS = bQ2 , and the second is a dissipative operator LD (X) =

1 2πλ (QXQ − {Q2 , X}). β 2

(29)

Because these two parts commute, it follows from the Trotter-Kato product formula that Tt (X) = eitHS (etLD X)e−itHS . (30) We now describe the effect of dissipation. Because M is a limit (in the σ-weak tLD preserves each local topology) of local algebras M2n ×2n = ⊗∞ 1 M2×2 , and e algebra so we may assume that X = (xij ) ∈ M2n ×2n . Then LD (X)ij = − i, j ∈ {1, ..., 2n }, and so

πλ (j − i)2 · n−1 xij , β 4

(31)

142


(j − i)2 etLD (X)ij = xij exp −γt n−1 , 4

(32)

where γ = πkλT . It follows from equation (32) that the loss of coherence is faster for coefficients which are more distant to the diagonal, and it increases with reservoir temperature similarly as in the model of a harmonic oscillator linearly coupled to an infinite bath of harmonic oscillators [61]. Suppose A is a von Neumann algebra generated by π0 (σn3 ), n ∈ N. Then A is a maximal commutative subalgebra in M, and let P : M → A be the normal norm one projection onto the von Neumann subalgebra A [55]. Since [HS , π0 (σn3 )] = 0, it follows from equations (30) and (32) that all observables from A are Tt -invariant. Theorem 14. For any statistical state ρ of the spin system and any spin observable X (33) lim Tt (X)ρ = P (X)ρ , t→∞

Proof. Because the semigroup (Tt )t≥0 satisfies all assumptions of Theorem 13 so the isometric-sweeping decomposition follows. Hence it is enough to show that A = / A, i.e. M1 . The inclusion A ⊂ M1 is obvious. Suppose that X ∈ M1 and X ∈ P (X) = X. Let Y = X − P (X). Then Y ∈ M1 and Y = 0. We may assume that Y 2 =, 1, where · 2 is the norm in the Hilbert space L2 (M). Let us take a sequence (An ), where An ∈ M2n ×2n ⊂ M, such that An → X in L2 (M). Then Bn = An −P (An ) ∈ M2n ×2n and Bn → Y . Hence, there exists n0 ∈ N such that Y − Bn0 2 < 14 . Because Tt Bn0 2 → 0, when t → ∞, so there exists t0 > 0 such that Tt0 Bn0 2 < 14 . Thus 1 = Tt0 Y 2 ≤ Tt0 (Y − Bn0 )2 + Tt0 Bn0 2
0 is a coupling constant, and an ∼ ( p1 )n for some p ≥ 2. Again, since the coefficients an are summable, the spin part of the coupling operator Q is bounded. We assume that g(k) = |k|1/2 χ(k), where χ(k) satisfies the same assumptions as in the previous subsection. The reduced dynamics of the system is given by equation (24) which in the Markovian approximation leads to the following formula for the corresponding generator L(A) = i[HS − bQ2 , A] + LD (A), where LD (A) =

1 2πλ (QAQ − {Q2 , A}), β 2

(37)

(38)

∞ and b = 0 χ2 (k)dk > 0. The first part in equation (37) is the commutator with a new collective Hamiltonian HC = HS − bQ2 , while the second term is a dissipative operator. The collective Hamiltonian & ' & ∞ ' ∞ 3 1 1 (39) H(n)σn − π0 b J(n + m)σn σm , HC = −π0 gµB n=1

n,m=1

where J(n) = an , is nothing else but the Hamiltonian of the Ising model with an infinite range interaction. However, the potentials H(n) and J(n) are not translationally invariant. Theorem 15. For the semigroup Tt = etL the isometric-sweeping decomposition holds with M1 = C · 1S . Proof. We proceeds by steps.

144


Step 1. It is clear from the form of the generator L, see equation (37), that it generates a semigroup Tt which satisfies all assumptions of Theorem 13. Hence the isometric-sweeping decomposition follows. Step 2. The subalgebra M1 is defined by the property Tt∗ Tt x = Tt Tt∗ x = x for all t ≥ 0. Hence ∞ ( l ker(LD ◦ δH ) ⊂ M1 , C l=0

where δHC (·) = i[HC , ·]. We prove now the reverse inclusion. Suppose that x ∈ M1 . Then, by differentiating the equation Tt∗ Tt x = x at time t = 0, we get M1 ⊂ kerLD . Assume that n−1 ( l kerLD ◦ δH M1 ⊂ C l=0

for some n ≥ 1. Because dn+1 ∗ T Tt x|t=0 = 0 dtn+1 t so

+

dn+1 ∗ T Tt x|t=0 = (−δHC + LD )n+1 (x) dtn+1 t

n n+1 (−δHC + LD )n+1−m ◦ (δHC + LD )m (x) + (δHC + LD )n+1 (x) m m=1 n+1 n+1 n n = (−1)n+1 δH (x) + (−1)n LD ◦ δH (x) + δH (x) + LD ◦ δH (x) C C C C n n+1 m (x) (−δHC + LD )n+1−m ◦ δH + C m m=1

n+1 n+1 n n = (−1)n+1 δH (x) + (−1)n LD ◦ δH (x) + δH (x) + LD ◦ δH (x) C C C C n n n+1 n+1 n+1 n (x) + (x) + (−1)n+1−m δH (−1)n−m LD ◦ δH C C m m m=1 m=1 n+1 (x) = δH C

n+1

m=0

+ {1 + (−1) [ n

n+1

m=0

n+1 m

n+1 m

(−1)n+1−m

n (x) (−1)m − (−1)n+1 ]}LD ◦ δH C

n (x) = 0. = 2LD ◦ δH S

Hence, by induction, M1 ⊂

∞ ( l=0

l kerLD ◦ δH . C


145

Step 3. Let C1 (respectively C3 ) be a C ∗ -subalgebra in the Glimm algebra generated by {σ1i1 ...σnin }, where ik = 0, 1 (ik = 0, 3 respectively), and n ∈ N. Then both π0 (C1 ) and π0 (C3 ) , where π0 (C1 ) denotes the bicommutant of the algebra π0 (C1 ), are maximal Abelian self-adjoint algebras (m.a.s.a in short) in M such that π0 (C1 ) ∩ π0 (C3 ) = C · 1S . The choice of coefficients (H(n)) and (an ) guarantees that L∞ (Q) = π0 (C1 ) and L∞ (HS ) = π0 (C3 ) , where L∞ (Q) is the von Neumann algebra generated by operator Q. Hence L∞ (Q) ∩ L∞ (HS ) = C · 1S . Step 4. We show now that if [Q, [Q, x]] = 0 for some x ∈ M, then x ∈ L∞ (Q). Let us define the derivation δx (·) = i[·, x]. If [Q, [Q, x]] = 0, then [Q, x] ∈ L∞ (Q) since, by step 3, L∞ (Q) is a m.a.s.a. Suppose that W is a polynomial. Then δx (W (Q)) = i[Q, x]W (Q) ∈ L∞ (Q). This implies that δx (L∞ (Q)) ⊂ L∞ (Q) since δx is continuous in the weak operator topology. Because L∞ (Q) is commutative so δx |L∞ (Q) = 0, and hence [Q, x] = 0. Because L∞ (Q) is a m.a.s.a so x ∈ L∞ (Q). Step 5. Next we show that kerLD ∩ L∞ (HC ) = C · 1S . Here L∞ (HC ) stands for the commutant in M of the algebra L∞ (HC ). Suppose that x ∈ kerLD ∩L∞ (HC ) . Then [Q, [Q, x]] = 0 and [HC , x] = 0. By step 4, x ∈ L∞ (Q) which implies that [HS , x] = [HC + bQ2 , x] = 0. Hence x ∈ L∞ (HS ). Because, by step 3, L∞ (Q) ∩ L∞ (HS ) = C · 1S so x = z1S , where z ∈ C. Step 6. By step 2, δHC (M1 ) ⊂ M1 . Hence, the derivation δ1 := δHC |M1 is well defined and bounded. Thus δ1 (·) = i[H1 , ·], where H1 = H1∗ ∈ M1 [52]. By step 2 again, H1 ∈ kerLD . On the other hand [HC , H1 ] = −iδ1 (H1 ) = [H1 , H1 ] = 0. Hence H1 ∈ L∞ (HC ) and so, by step 5, H1 is proportional to the identity operator. Suppose now that x ∈ M1 . Then [HC , x] = −iδ1 (x) = 0, and so x ∈ L∞ (HC ) . Because x ∈ kerLD so, by step 5, x is proportional to the identity operator. Hence M1 = C · 1S . 2 It follows that the system is ergodic, i.e. all expectation values of an observable Tt (A), where A = π0 (σ1i1 ...σnin ), tend to zero when t → ∞, if at least one ik = 0. We use now this dynamical destruction of all coherent terms for reducing the number of degrees of freedom. Corollary 16. Suppose that the first site does not interact with the reservoir, i.e. we put in equation (36) a1 = 0. Then M1 = M2×2 and for any A ∈ M1 Tt (A) = eith1 σ Ae−ith1 σ , 3

3

(40)

where h1 = H(1). Proof. Suppose that in equation (36) the coefficient a1 = 0. The corresponding semigroup we shall denote by Tt1 . Let A be a subalgebra in M generated by {π0 (σ1k ) : k = 0, 1, 2, 3}. Suppose that x ∈ M. Then

146


x =

3

π0 (σ1k )xk ,

k=0

where operators xk belong to A , the commutant in M of algebra A. Let St be a semigroup on M with a generator L0 given by the following Markov master equation L0 (A) = i[HS0 − bQ2 , A] + LD (A), where LD is defined in equation (38), and & HS0

= π0

−gµB

∞

' H(n)σn3

.

n=2

Note that the summation index ranges from 2 to infinity. Then Tt1 (x) =

3

π0 (Ut∗ σ1k Ut )St (xk ),

k=0

where Ut = e−ith1 σ1 . Since operators π0 (Ut∗ σ1k Ut ), k = 0, 1, 2, 3, are orthogonal in L2 (M) so 3 Tt1 (x)2L2 = St (xk )2L2 . 3

k=0

Let us notice that the semigroup St restricted to the commutant A has the same properties as the semigroup Tt . Hence, if any of xk is not proportional to the identity operator, then, by the above theorem, St (xk )L2 < xk L2 for all t > 0. Thus Tt1 (x)L2 < xL2 , too, which implies that such an operator cannot belong to M1 . Hence, if x ∈ M1 , then xk = zk 1S , zk ∈ C, for all k = 0, 1, 2, 3, and so x ∈ A. It follows that M1 = A = M2×2 , and the dynamics on it is given by unitary operators Ut . 2 This result shows that the infinite quantum spin system, subjected to a specific interaction with the phonon field, after the decoherence time may be effectively described as a quantum system with only one degree of freedom. In other words, the environment forces the spin particles to behave in a collective way what allows introduction of three collective observables which satisfy the standard commutation relations of spin momenta. Generalization to a finite number of degrees of freedom is straightforward: If it happens that a1 = a2 = ... = an = 0, then M1 = M2n ×2n . 3.4 From Quantum to Classical Dynamical Systems [38] The origin of deterministic laws that govern the classical domain of our everyday experience has also attracted much attention in recent years. In particular, the emergence of classical mechanics described by differential, and hence local, equations


147

of motion from the evolution of delocalized quantum states was at the center of this issue. For example, the question in which asymptotic regime non-relativistic quantum mechanics reduces to its ancestor, i.e. Hamiltonian mechanics, was addressed in [27]. It was shown there that for very many bosons with weak two-body interactions there is a class of states for which time evolution of expectation values of certain operators in these states is approximately described by a non-linear Hartree equation. The problem under what circumstances such an equation reduces to the Newtonian mechanics of point particles was also discussed in that paper. A different point of view was taken in a seminal paper by Gell-Mann and Hartle [28]. They gave a thorough analysis of the role of decoherence in the derivation of phenomenological classical equations of motion. Various forms of decoherence (weak, strong) and realistic mechanisms for the emergence of various degrees of classicality were also presented. In the same spirit it was shown in [38] that an infinite quantum system subjected to a specific interaction with another quantum system may be effectively described as a simple classical dynamical system. More precisely, the effective observables of the system were parameterized by a single collective variable which underwent a continuous periodic evolution. We shall say that decoherence induces classical behavior of the quantum system if M1 is commutative and its evolution is given by a continuous flow on the configuration space of the algebra M1 . In that example M1 was the same as in Section 3.2, i.e. M1 = L∞ (C, dµ), where C is the Cantor set. However, contrary to the continuous pointer case, the evolution was given by a one parameter periodic group of automorphisms αt . Let us describe briefly this evolution. Suppose that S 1 = {eia , a ∈ R} and let λ : C → S 1 be given by ' & ∞ in λ(i1 , i2 , ...) = exp 2πi , 2n+1 n=1 ˆ of the corresponding algebras where ij ∈ {0, 2}. It induces an isomorphism λ ˆ : L∞ (S 1 , da) → L∞ (C, dµ), λ where da denotes the normalized Lebesgue measure on the Borel σ-algebra of the ˆ t of the algebra L∞ (S 1 , da), α ˆt = circle S 1 . Then the group of automorphism α −1 ˆ ˆ λ ◦ αt ◦ λ, is induced by a continuous flow on the underlying configuration space eia → ei(a+2πt) , i.e. a uniform rotation of the circle. An even more transparent example of an environment induced classical dynamical system was presented in [39]. A quantum dynamical semigroup (Tt )t≥0 of a quantum system represented by a factor of type II∞ such that (M1 , Tt |M1 ) was isomorphic with a classical system (L∞ (R3 , dx), gt ), where gt was a uniform motion, i.e. with a constant velocity, in R3 was constructed there. It should be noted, however, that such a factor has no direct physical interpretation. In order to deal with realistic infinite quantum systems like Bose gases one has to consider abstract C ∗ -algebras of canonical commutation relations (CCR) and their temperature representations which lead to type III factors. The discussion of irreversible dynamics of such algebras is less advanced and concentrated mainly on the so-called quasifree dynamical semigroups [1, 21, 23], see also [18, 19], where a general form of

148


quasi-free dynamical semigroups was given. In the next section we address a question how one can construct a class of quasi-free dynamical semigroups on the CCR algebras which would combine deterministic and stochastic evolutions on the one particle space.

4 Dynamical Semigroups on CCR Algebras 4.1 Algebras of Canonical Commutation Relations (CCR) The aim of this subsection is to set up a formalism in which we can discuss systematically the canonical commutation relations for a system with finite or infinite number of degrees of freedom. A comprehensive discussion of this subject can be found in [14]. Suppose S is a real linear space equipped with a nondegenerate symplectic bilinear form σ : S ×S → R. Moreover, we assume the existence of a linear operator J on S with the following properties σ(Jf, g) = −σ(f, Jg),

J 2 = −id.

With the help of J and σ one can introduce a complex pre-Hilbert space with the scalar multiplication and the scalar product defined by (λ1 + iλ2 )f = λ1 f + λ2 Jf,

λi ∈ R,

< f, g > = σ(f, Jg) + iσ(f, g), where f, g ∈ S. Its norm completion will be denoted by H. On S there is usually defined its own topology τ , which is stronger than the norm topology and which makes S a real locally convex topological vector space, for the definition see the next subsection. The case in which S is infinite dimensional is typical for field theories and many-body problems, whereas finite dimensional S corresponds to quantum mechanics of finite number of particles. Let ∆(S) be the space of formal linear combinations finite ∆(S) = { zk W (fk )}, where zk ∈ C, fk ∈ S, and W (fk ) being abstract symbols called the Weyl operators. Clearly ∆(S) is a complex linear space. The product of two Weyl operators is defined as W (f )W (g) = e−iσ(f, g)/2 W (f + g), while the ∗ -operation as W (f )∗ = W (−f ), and they are next extended to ∆(S) by linearity (anti-linearity) respectively. The completion ∆∗ 1 (S) of ∆(S) with respect |zk |, is a Banach -algebra. We now define a to the norm zk W (fk )1 = new norm on ∆1 (S) by R = sup π(R), π

R ∈ ∆1 (S),


149

where the supremum is taken over all nondegenerate representations π of ∆1 (S) for which π(W (λf )), f ∈ S, is continuous in λ ∈ R with respect to the σ-weak topology on B(Hπ ). The completion of ∆(S) with respect to this norm is a C ∗ -algebra, say W(S), which we refer to as the C ∗ -algebra of the canonical commutation relations [20]. It is worth noting that such an algebra is simple. 4.2 Promeasures on Locally Convex Topological Vector Spaces Suppose E is a locally convex topological vector space over R, i.e. such that its topology is defined by a family of seminorms separating points. It is clear that the topology of a locally convex space is always Hausdorff. By E we denote the topological dual, and by E ∗ the algebraic dual of the space E. Let I be the set of all closed linear subspaces V in E such that dim(E/V ) < ∞, and let pV : E → E/V be the canonical projection. We say that V ≤ W , V, W ∈ I, if W ⊂ V . For any V ≤ W we define a surjective linear map pV W : E/W → E/V by pV W (pW f ) = pV f , f ∈ E. Then (E/V, pV W , I) is a projective net of finite dimensional locally convex (and hence locally compact) topological vector spaces. The projective limit of this net is canonically isomorphic to the topological space E ∗ equipped with the σ(E ∗ , E )-topology. Let M (E/V ) denote the set of all complex measures on E/V with finite variations. M (E/V ), when equipped with the natural sum and multiplication by scalars, the multiplication given by convolution ∗, and the norm µV = |µV |(E/V ), is a Banach algebra. As a Banach space M (E/V ) is the dual space to C0 (M/V ), the Banach space of continuous functions on E/V vanishing at infinity and equipped with the sup-norm. By definition, see [12], a promeasure on E is an arbitrary projective net (µV , (pV W )∗ , I), where µV is a positive finite measure on E/V , (pV W )∗ : M (E/W ) → M (E/V ) is the induced algebraic homomorphism, and (pV W )∗ (µW ) = µV for all V ≤ W . It is worth noting that in general the projective limit lim← µV may not exist on E ∗ . However, if dimE < ∞, then any promeasure on E can be identified with a measure in an obvious way. To simplify notation we shall denote a promeasure by (µV )V ∈I or just by µ, if there is no risk of confusion. Since for all V ≤ W , µV (E/V ) = (pV W )∗ µW (E/V ) = µW (p−1 V W (E/V )) = µW (E/W ), we conclude that µV1 = µV2 for all V1 , V2 ∈ I. This common value uniquely associated with the promeasure µ = (µV )V ∈I , is called its total mass and will be denoted by µ. If the total mass is equal to one, we shall say that (µV )V ∈I is a probability promeasure on E. Suppose now that (µV )V ∈I and (νV )V ∈I are promeasures on E. Because (pV W )∗ (µW ∗ νW ) = (pV W )∗ (µW ) ∗ (pV W )∗ (νW ) = µV ∗ νV so µ ∗ ν = (µV ∗ νV )V ∈I is again a promeasure on E, which we shall call the convolution of promeasures (µV )V ∈I and (νV )V ∈I . It is clear that convolution of probability promeasures is also a probability promeasure. If T : E → E is R-linear and continuous, then for any V ∈ I also T −1 (V ) ∈ I and so the linear operator

150


TV : E/T −1 (V ) → E/V,

TV (pT −1 (V ) f ) = pV (T f ),

f ∈ E, is well defined. Moreover, it is injective. Let (TV )∗ : M (E/T −1 (V )) → M (E/V ) be the induced homomorphism of measure algebras. Proposition 17. Suppose (µV )V ∈I is a promeasure on E. Then ν = (νV )V ∈I , where νV = (TV )∗ (µT −1 (V ) ), is also a promeasure on E, which we shall denote by T∗ (µ). Moreover, T∗ (µ) = µ. Proof. If V ≤ W , then (pV W )∗ νW = (pV W )∗ (TW )∗ (µT −1 (W ) ) = (pV W ◦ TW )∗ (µT −1 (W ) ). Because pV W ◦ TW = TV ◦ pT −1 (V )T −1 (W ) so (pV W ◦ TW )∗ (µT −1 (W ) ) = (TV )∗ (pT −1 (V )T −1 (W ) )∗ (µT −1 (W ) ) = (TV )∗ (µT −1 (V ) ) = νV . By definition, T∗ (µ) = νV for any V ∈ I. Hence T∗ (µ) = µT −1 (V ) (TV−1 (E/V )) = µT −1 (V ) = µ, which completes the proof. 2 Suppose now that x ∈ E . If µ = (µV )V ∈I is a promeasure on E, then µx = (x )∗ (µ) is a finite measure on R. Hence

∞

F(µ)(x ) =

eit µx (dt), −∞

is a function on E which we shall call the Fourier transform of the promeasure µ. It is a positive definite function which is continuous on every finite dimensional subspace of E [12]. Let us recall that E as the topological dual space is equipped with the σ(E , E)-topology. Proposition 18. If µ = (µV )V ∈I and ν = (νV )V ∈I are promeasures on E, then for all x ∈ E , F(µ ∗ ν)(x ) = F(µ)(x ) · F(ν)(x ). Proof.

∞

F(µ ∗ ν)(x ) = −∞

∞

∞

=

∞

e (x )∗ (µ ∗ ν)(dt) = it

eit (µx ∗ νx )(dt) −∞

ei(t+s) µx (dt)νx (ds) = F(µ)(x ) · F(ν)(x ).

2

−∞ −∞

Proposition 19. If T : E → E is R-linear and continuous, then for any promeasure µ on E, F(T∗ (µ)) = F(µ) ◦ T , where T : E → E is the dual operator. Proof. Let x ∈ E . Then


F(T∗ (µ))(x ) =

∞

eit (x )∗ (T∗ µ)(dt) =

−∞

∞ =

∞

151

eit (x ◦ T )∗ (µ)(dt)

−∞

eit (T (x ))∗ (µ)(dt) = F(µ)(T (x )).

2

−∞

Combining Propositions 18 and 19 we obtain the following: F(µ ∗ (T∗ ν)) = F(µ) · (F(ν) ◦ T ).

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4.3 Perturbed Convolution Semigroups of Promeasures Suppose that (St )t≥0 is a semigroup of R-linear and continuous contractions in E, i.e. S0 = id and St ◦ Ss = St+s for all s, t ≥ 0. Let µt = (µV (t))V ∈I , t ≥ 0, be a family of probability promeasures on E. We shall say that µt is an St -perturbed convolution semigroup if µ0 = δ0 , where δ0 denotes the Dirac point measure with support in the zero vector of E, and for all s, t ≥ 0, µt ∗ [(St )∗ µs ] = µs+t ,

(42)

i.e. for all V ∈ I the following equality holds µV (t) ∗ [(St,V )∗ µS −1 (V ) (s)] = µV (s + t). t

(43)

Let r, s, t ≥ 0. The following calculations µt+s ∗ [(St+s )∗ µr ] = [µt ∗ (St )∗ µs ] ∗ [(St )∗ (Ss )∗ µr ] = µt ∗ [(St )∗ (µs ∗ (Ss )∗ µr )] = µt ∗ [(St )∗ µs+r ], show that this notion is well defined. Construction of perturbed semigroups is similar to that of typical convolution semigroups. For example, we prove the following. Theorem 20. Let ν be a probability promeasure on E. Suppose that the function t → (St,V )∗ νS −1 (V ) ∈ M (E/V ) is weakly∗ -measurable for all V ∈ I. Then there t exists a Poisson St -perturbed convolution semigroup µt of probability promeasures on E. Proof. We proceed by steps. Step 1. Because the function t → (St,V )∗ νS −1 (V ) is weakly∗ -measurable and t (St,V )∗ νS −1 (V ) = 1 for all t ≥ 0, so there exists a measure νV (t) ∈ M (E/V ) t such that for any f ∈ C0 (E/V ), t νV (t)(f ) =

(Ss,V )∗ νSs−1 (V ) (f )ds. 0

152


We show that νt = (νV (t))V ∈I is a promeasure on E. Let V ≤ W . Then, for any t ≥ 0, t t (pV W )∗ νW (t) = (pV W )∗ [ (Ss,W )∗ νSs−1 (W ) ds] = (pV W ◦ Ss,W )∗ νSs−1 (W ) ds 0

0

t

t (Ss,V ◦ pSs−1 (V )Ss−1 (W ) )∗ νSs−1 (W ) ds =

= 0

(Ss,V )∗ νSs−1 (V ) ds = νV (t). 0

Step 2. If ν is a promeasure on E, then µ = (µV )V ∈I given by µV = eνV is also a promeasure on E. By definition, νV ∗ νV + ... 2!

µV = δ0 + νV +

Because νV ∗ νV = νV 2 so the series is norm convergent in M (E/V ). Suppose that V ≤ W . Because (pV W )∗ is norm continuous so (pV W )∗ µW = lim (pV W )∗ n→∞

n (νW )k

= µV .

k!

k=0

Step 3. For a probability promeasure ν on E we define −at

µt = e

t exp[a

(Ss )∗ νds], 0

where a > 0. By steps 1 and 2, µt is a probability promeasure on E such that µ0 = δ0 . We show that (µt )t≥0 is an St -perturbed convolution semigroup. Let V ∈ I. Then µV (t) ∗ [(St,V )∗ µS −1 (V ) (s)] = e−a(t+s) exp[a(νV (t) + (St,V )∗ νS −1 (V ) (s))] t

−a(t+s)

= e

t

t s exp[a( (Sr,V )∗ νSr−1 (V ) dr + (St,V )∗ (Sr,S −1 (V ) )∗ νSr−1 (S −1 V ) dr)]. t

0

t

0

Because St,V ◦ Sr,S −1 (V ) = Sr+t,V so t

µV (t) ∗ [(St,V )∗ µS −1 (V ) (s)] t

−a(t+s)

= e

t s exp[a( (Sr,V )∗ νSr−1 (V ) dr + (St+r,V )∗ νS −1 (V ) dr)] t+r

0

0

Decoherence as Irreversible Dynamical Process in Open Quantum Systems −a(t+s)

e

153

t+s exp[a( (Sr,V )∗ νSr−1 (V ) dr)] = µV (t + s). 0

Guided by the theory of stochastic processes we shall call such a semigroup the Poisson St -perturbed convolution semigroup. 2 Let (µt )t≥0 be an St -perturbed convolution semigroup. If Γt = F(µt ), then by formula (41), (44) Γt+s (x ) = Γt (x ) · Γs (St x ), for all x ∈ E . We use this property in the next subsection to construct a quantum dynamical semigroup on the CCR algebra W. 4.4 Quantum Dynamical Semigroups on CCR Algebras In order to construct a quantum dynamical semigroup on W = W(S) we combine a deterministic evolution given by a semigroup of injective algebraic homomorphisms of W and a stochastic evolution represented by a perturbed convolution semigroup of probability promeasures. Let (St )t≥0 be a semigroup of R-linear and continuous operators on (S, τ ) such that σ(St f, St g) = σ(f, g) for all f, g ∈ S and all t ≥ 0. It was shown in [41] that with such a semigroup one can associate a semigroup of algebraic and unital ∗ -homomorphisms αt : W → W being the extension of the map αt (W (f )) = W (St f ), f ∈ S. It is worth pointing out that since W is simple so all αt are injective. It is obvious that such a semigroup generalizes the notion of automorphic evolution. Since all αt are injective and map unitary operators from W into unitary operators we shall say that (α)t≥0 represents a deterministic evolution of the system. Now let E = S , where S is the topological dual space to (S, τ ). S with the σ(S , S)-topology is a locally convex topological vector space over R such that S = S. Since the topology τ is stronger than the norm topology so the following inclusion S ⊂ H ⊂ S holds. Let (St )t≥0 , St : S → S , be the dual semigroup. By definition, St are R-linear and continuous operators on S such that (St ) = St . Theorem 21. Suppose that (µt )t≥0 is an St -perturbed convolution semigroup of probability promeasures on S . Then there exists a unique quantum dynamical semigroup (Tt )t≥0 , Tt : W → W, such that Tt W (f ) = F(µt )(f )W (St f ),

(45)

for all f ∈ S. If the following conditions a) limt→0+ σ(St f, g) = σ(f, g) for all f, g ∈ S, b) limt→0+ ω(W (St f − f )) = 1, f ∈ S, for some state ω ∈ S, c) limt→0+ µV (t) = δ0 ∈ M (E/V ) in the vague topology for all V ∈ I, hold, then the semigroup (Tt )t≥0 is ω-continuous. Proof. Let Tt0 W (f ) = Γt (f )W (f ), where Γ (f ) = F(µt )(f ), and f ∈ S. We show that operator Tt0 can be extended to a completely positive norm contractive

154


and unital operator on W. By linearity, Tt0 : ∆(S) → ∆(S). The space S when equipped with the discrete topology is an Abelian group whose dual group (the group of characters) Sˆ is a commutative compact group. The pairing between S and ˆ With a character fˆ one can associate a ∗ Sˆ we denote by (f, fˆ), f ∈ S and fˆ ∈ S. automorphism βfˆ of ∆(S) defined by βfˆW (f ) = (f, fˆ)W (f ), and then extended by linearity to ∆(S). Since Γt is a positive definite function on the group S and ˆt on Sˆ such Γt (0) = 1 so for any t ≥ 0 there exists a probability Borel measure µ that (f, fˆ)ˆ µt (dfˆ), Γt (f ) = ˆ S

see for example [51]. Hence, for any x ∈ ∆(S), 0 βfˆ(x)ˆ µt (dfˆ). Tt (x) =

(46)

ˆ S

Because βfˆ(x) = x so Tt0 (x) ≤ x, and Tt0 can be extended to a contractive operator on the algebra W. It is also clear that Tt0 (1) = 1. Since the formula (46) holds for any A ∈ W, so for all A1 , ..., An and B1 , ..., Bn from W we get n

n

Bj∗ (Tt0 (A∗j Ai ))Bi =

i,j=1

Bj∗ [ βfˆ(Aj )∗ βfˆ(Ai )ˆ µt (dfˆ)]Bi

i,j=1

=

ˆ S

n n ( βfˆ(Aj )Bj )∗ ( βfˆ(Ai )Bi )ˆ µt (dfˆ) ≥ 0. ˆ S

j=1

i=1

Thus Tt0 is completely positive for all t ≥ 0. Let us now define Tt : W → W, Tt = αt ◦ Tt0 , t ≥ 0. By definition, Tt is a norm contractive completely positive and unital operator on W. Let us check that (Tt )t≥0 is a semigroup. Clearly, it is enough to show the semigroup property on Weyl operators. Suppose that s, t ≥ 0 and f ∈ S. Then (Ts ◦ Tt )W (f ) = (αs ◦ Ts0 )(αt ◦ Tt0 )W (f ) = (αs ◦ Ts0 )(Γt (f )W (St f )) = Γt (f )Γs (St f )W (Ss+t f ). St -perturbed

Because (µt )t≥0 is an convolution semigroup on S so, by formula (44), Γt (f )Γs (St f ) = Γs+t (f ). Hence (Ts ◦ Tt )W (f ) = Ts+t W (f ). Finally, we show that the mapping t → πω (Tt A), A ∈ W, where πω is the GNS representation associated with the state ω, is σ-strongly continuous. Because operators Tt are contractive it is enough to check that for any f ∈ S, lim πω (Tt W (f )) = πω (W (f ))

t→0+

in the strong topology. Suppose that g ∈ S. Then, by assumptions, a) and b)


155

(πω (W (St f )) − πω (W (f )))πω (W (g))Ω2 = 2 − 2Re < πω (W (St f ))πω (W (g))Ω, πω (W (f ))πω (W (g))Ω > = 2 − 2Re[eiσ(St f,g) e−iσ(f,g) eiσ(St f,f )/2 ω(W (St f − f ))], tends to zero when t → 0+ . Let)V ⊂ S , V ∈ I, and let V 0 be the subspace of S orthogonal to V . Because S = V ∈I V 0 , so for any f ∈ S there exists V ∈ Isuch that f ∈ V 0 . However, for any g ∈ V 0 , eif (g) µV (t)(df ). F(µt )(g) = S /V

Let us notice that since g ∈ V 0 , the action f (g), f ∈ S /V , is well defined. By assumption c) limt→0+ Γt (f ) = 1. Hence for any g ∈ S, lim (πω (Tt W (f )) − πω (W (f )))πω (W (g))Ω2 = 0,

t→0+

and so the semigroup (Tt )t≥0 is ω-continuous. 2 By means of St -perturbed convolution semigroups of probability promeasures on S one can construct a general class of quantum dynamical semigroups on the CCR algebras. In the next subsection we present a simple example, known to physicists as the quantum Brownian motion in the large mass limit, which illustrates the above framework. 4.5 Example: Quantum Brownian Motion Let us consider a quantum particle in R3 . For such a quantum system S = R6 ≡ R3 × R3 . The CCR algebra W = W(S) is generated by Weyl operators W (a, b), a, b ∈ R3 . A remarkable theorem due to Stone and von Neumann shows that there is essentially only one faithful representation π of W, the so-called Schrödinger representation in the Hilbert space L2 (R3 , dx) of square integrable functions: π(W (a, b)) =

3

eiaj bj /2 Uj (aj )Vj (bj ),

(47)

j=1

where a = (a1 , a2 , a3 ), b = (b1 , b2 , b3 ), and the unitary operators Uj and Vj are given by (48) Uj (aj )ψ(x1 , x2 , x3 ) = eiaj xj ψ(x1 , x2 , x3 ), Vj (bj )ψ(x1 , x2 , x3 ) = ψ(x1 − δ1j bj , x2 − δ2j bj , x3 − δ3j bj ).

(49)

The generators of the one parameter groups of unitary operators Uj (Vj ) we denote pj ) respectively. Dynamical de-quantization of such a system means that due by x ˆj (ˆ

156


to the interaction with an environment the effective (or decoherence free) observables of the system form a commutative algebra of functions on the configuration space R3 . Guided by the discussion of the previous subsection we construct a quantum dynamical semigroup on W using a convolution semigroup of probability measures on S = S . To this end suppose that the deterministic evolution of the system is trivial, i.e.that St = id for all t ≥ 0. Suppose further that (µt )t≥0 are probability = tm, distributions of a Gaussian process Xt on S with the mean vector m(t) m = (m1 , ..., m6 ), and the covariance matrix K(s, t) = min(s, t) · K, where K = [Kjk ] is a positive definite matrix in R6 . Then the Fourier transform of µt , the so-called characteristic function of the process Xt is given by 1 < K(t, t)x, x >] 2 ⎡ ⎤ 6 6 t = exp ⎣it xj mj − Kjk xj xk ⎦ , 2 j=1

Γt (x) = exp[i < x, m(t) > −

(50)

j,k=1

where for simplicity we replaced a vector (a, b) by x ∈ R6 . If the process Xt takes values in {0} × R3 , i.e. Kjk = 0 whenever j ≤ 3 or k ≤ 3, and m = (0, 0, 0, m1 , m2 , m3 ), then ⎤ ⎡ 3 3 t 0 (51) bj mj − Kjk bj bk ⎦ , Γt (a, b) = exp ⎣it 2 j=1 j,k=1

0 where the matrix K 0 : R3 → R3 is defined by Kjk = K(j+3)(k+3) . It follows from equation (51) that the unitary operators W (a, 0) are Tt -invariant while the other operators tend to zero when t → ∞. Hence, for any A ∈ W

lim Tt (A) = P (A),

t→∞

(52)

in the norm topology, where P : W → C is a projection onto a commutative subalgebra generated by the unitary operators W (a, 0), a ∈ R3 . More precisely µH (dχ)τχ (W (a, b)), (53) P (W (a, b)) = R3

where µH is a normalized Haar measure on the Bohr compactification R3 of R3 , and τχ is an automorphism of W given by τχ (W (a, b)) = χ(b)W (a, b). Because

µH (dχ)χ(b) = 0 R3

(54)


157

if b = 0 so P (W (a, b)) = 0 whenever b = 0. Hence the isometric-sweeping decomposition is given by A = P (A) + (id − P )(A), A ∈ W. Because the algebra C is isomorphic to the C ∗ -algebra of quasi-periodic functions on R3 so the semigroup (Tt )t≥0 indeed leads to the dynamical de-quantization of the system. Finally, we derive the formula for the generator L of the semigroup (Tt )t≥0 in the Schrödinger representation π. Since (55) Tt π(W (a, b)) = Γt (a, b)π(W (a, b)), where Γt (a, b) is given by equation (51), and [ˆ xj , π(W (a, b))] = bj π(W (a, b)) so Lπ(W (a, b)) = i

3 j=1

mj [ˆ xj , π(W (a, b))] −

3 1 0 Kjk [ˆ xj , [ˆ xk , π(W (a, b))]]. 2 j,k=1

0 is diagonal, then L is the If mj = 0 for all j ∈ {1, 2, 3} and if the matrix Kjk generator of the quantum Brownian motion in the large mass limit [11, 69].

5 Outlook The example presented in the previous subsection is rather simple. To construct the semigroup of quantum Brownian motion one assumes that the system has a finite number of degrees of freedom and that the corresponding convolution semigroup is that of a Gaussian process. It is obvious, however, that it is a very specific case. Possible generalizations include for example application of arbitrary infinitely divisible processes like the α-stable and Poisson processes. The main advantage, however, of the proposed framework is based on the possibility of construction quantum dynamical semigroups of systems in the thermodynamic limit. CCR algebras with infinite dimensional spaces S and their temperature representations describe Bose gases. It is believed that such systems strongly interact with their environment and so they show up efficient decoherence phenomena. For example decoherence due to environmental coupling should be transparent when a Bose-Einstein condensate is present in the trap. Many features of Bose-Einstein condensates are well described by the mean-field theory. In the mean-field picture all atoms of the condensate have the same macroscopic function satisfying the GrossPitajevski equation. This equation is so successful because short-range correlations between the bosons induced by the interatomic potential may be neglected. However, such a system cannot be isolated in practice. Even at low temperatures the interaction between atoms of the condensate and those outside the trap leads to ejection of atoms from the condensate suggesting rich microscopic dynamic not captured by the mean-field theory. Therefore, a new rigorous model of interacting continuous quantum systems is necessary for the description of such phenomena. We hope that the proposed framework of irreversible dynamics of infinite quantum systems will play an essential role in future investigations of this subject.

158


Acknowledgements One of the authors (R. O.) has been supported by the Polish Ministry of Scientific Research and Information Technology under the grant No PBZ-MIN-008/P03/2003. We both thank the Referee for his valuable comments and remarks.

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Notes on the Qualitative Behaviour of Quantum Markov Semigroups∗ Franco Fagnola1 and Rolando Rebolledo2 1

2

1

Politecnico di Milano, Dipartmento di Matematica “F. Brioschi” Piazza Leonardo da Vinci 32, 20133 Milano, Italy e-mail: [email protected] Facultad de Matemáticas, Universidad Católica de Chile Casilla 306 Santiago 22, Chile e-mail: [email protected]

Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 162 1.1

Preliminaries . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 164

2

Ergodic Theorems . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 165

3

The Minimal Quantum Dynamical Semigroup . . . . . . . . . . . . . . . . . . . . 167

4

The Existence of Stationary States . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 172 4.1 4.2 4.3 4.4 4.5 4.6

5

Faithful Stationary States and Irreducibility . . . . . . . . . . . . . . . . . . . . . . 184 5.1 5.2 5.3

6

The Support of an Invariant State . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 184 Subharmonic Projections. The Case M = L(h) . . . . . . . . . . . . . . . . . 186 Examples . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 188

The Convergence Towards the Equilibrium . . . . . . . . . . . . . . . . . . . . . . . 189 6.1 6.2

7

A General Result . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 172 Conditions on the Generator . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 174 Examples . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 178 A Multimode Dicke Laser Model . . . . . . . . . . . . . . . . . . . . . . . . . . . . 178 A Quantum Model of Absorption and Stimulated Emission . . . . . . . 182 The Jaynes-Cummings Model . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 183

Main Results . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 190 Examples . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 192

Recurrence and Transience of Quantum Markov Semigroups . . . . . . 194 7.1

Potential . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 194

∗ Partially supported by FONDECYT grant 1030552 and CONICYT/ECOS exchange program

162

Franco Fagnola and Rolando Rebolledo

7.2 7.3

Defining Recurrence and Transience . . . . . . . . . . . . . . . . . . . . . . . . . . 198 The Behavior of a d-Harmonic Oscillator . . . . . . . . . . . . . . . . . . . . . . 201

References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 203

1 Introduction Within these notes we provide a survey of results connected with the large time behavior of Quantum Markov Semigroups. More precisely, given a QMS T = (Tt )t≥0 we explore below a number of conditions on its generator L to have the following list of properties of the semigroup: – – – –

Existence of stationary states; Existence of a faithful stationary state; Convergence towards the equilibrium; Recurrence and Transience.

It is worth noticing several peculiarities of this mathematical study. To have a notion of semigroup broad enough to include both, quantum dynamics (“Master Equations”) as well as the classical Markov structure, one sacrifices strong topological properties. This leads to difficult problems like that of characterizing the semigroup from its generator, a problem which has been solved for an important class of Quantum Markov semigroups (see [43], [20], [21], [39]) but which is far from being closed. As we will see below, in most cases the generator of such a semigroup is given as a densely defined sesquilinear form on a Hilbert space. This forces to construct the Quantum Markov semigroup following the procedure used in Classical Probability to built up the minimal semigroup (see, for instance, [16]). In this case, the preservation of the identity, which is equivalent to the characterization of the domain of the generator, is often a non trivial problem. Tools for solving this problem have been developed by Chebotarev and Fagnola in [14] (see also [26], [15]). As a compensation of weak topological properties, a strong algebraic condition is assumed, namely the property of complete positivity. This notion is the key feature which allowed the development of the current theory of Quantum Markov Semigroups. Let be given a von Neumann algebra M of operators over a complex separable Hilbert space h, endowed with a trace tr(·). We follow the previous text [52] to introduce a Quantum Markov Semigroup as a w∗ -continuous semigroup T = (Tt )t∈R+ of normal completely positive linear maps on M satisfying that T0 (·) is the identity map of M and such that Tt (1) = 1, for all t ≥ 0, where 1 denotes the unit operator in M. In general these semigroups are termed as Quantum Dynamical Semigroups too, however, we will reserve that name for the most general category of semigroups including both Markov and sub-Markov semigroups for which the weaker condition Tt (1) ≤ 1 holds. The infinitesimal generator of T is the operator L(·) with domain D(L) which is the vector space of all elements a ∈ M such that the w∗ –limit of t−1 (Tt (a) − a) exists. For a ∈ D(L(·)), L(a) is defined as the limit above.

Notes on the Qualitative Behaviour of Quantum Markov Semigroups

163

We recall here for easy reference the following well-known examples. Example 1.1. The dynamics of closed systems is defined via a group of linear unitary transformations Ut : h → h, (t ∈ R), with a generator H which is self-adjoint. Indeed, it suffices to consider the von Neumann algebra M = L(h) of all bounded linear operators acting on h, the quantum Markov semigroup being defined as Tt (a) = Ut∗ aUt = eitH ae−itH , for all t ≥ 0. If H is bounded, the quantum Markov semigroup is uniformly strongly continuous, that is lim sup Tt (a) − a = 0. t→0 a≤1

In this case the infinitesimal generator is L(a) = i[H, a], (a ∈ M).

Example 1.2. A slight modification of the above example consists in taking a general strongly continuous semigroup (Pt )t∈R+ R+ acting on a complex separable Hilbert space h, with generator G. Define Tt (a) = Pt∗ aPt , for all t ≥ 0, a ∈ L(h). If G is bounded, the generator is L(a) = G∗ a + aG, (a ∈ L(h)). If G is unbounded, the above expression needs to be interpreted as a sesquilinear form: −(a)(v, L u) = Gv, au + v, aGu, for all u, v in the domain D(G) of G, a ∈ M. Definition 1.1. A state ω on the given von . Neumann . algebra M is normal it is σ– weakly continuous, or equivalently if ω( .α aα ) = α ω(aα ) for any increasing net (aα )α of positive elements in M, where α is the symbol for the least upper bound of a net. ω is faithful if ω(a) > 0 for all non-zero positive element a ∈ M. Given a quantum Markov semigroup T in M, a state ω is invariant with respect to the semigroup if ω(Tt (a)) = ω(a), for any a ∈ M, t ≥ 0. A von Neumann algebra M is σ-finite if and only if there exists a normal faithful state on M (see [11], Proposition 2.5.6). In particular, any von Neumann algebra on a separable Hilbert space is σ-finite. Within this framework we will be placed throughout this paper.

164


The notes are organized as follows: first we introduce some preliminary notations and concepts. We then analyze ergodic type theorems. Next, we establish a criterion on the existence of stationary states, depending on conditions on the generator of the semigroup. We continue analyzing faithfulness of stationary states and giving a result on the convergence towards the equilibrium of the QMS, the analysis of recurrence and transience being the final lecture. We have made an effort to keep the text as simple as possible, sacrificing in many cases the proof of statements requiring more sophisticated concepts which the interested reader can follow in the references. Namely, this is the case for a number of results whose proof is based on dilations of QMS by means of quantum cocycles, so called quantum dilations of Markov semigroups. This subject uses in force the results of the chapter on quantum stochastic differential equations written by Franco Fagnola. Along the last five years we have been invited to lecture on the subject of these notes several times, so that besides the papers containing the original results of our joint work, the reader is addressed to the previous surveys [33], [34] to complement the current text with additional examples and the use of quantum dilations to study the convergence towards the equilibrium of QMS with unbounded generators.

1.1 Preliminaries We start by fixing notations which will be used throughout the remains of the current article. We write h a complex separable Hilbert space, endowed with a scalar product ·, · antilinear in the first variable, linear in the second. L(h) denotes the von Neumann algebra of all the bounded linear operators in h. The w∗ or σ–weak topology of L(h) is the weaker topology for which all maps x → tr(ρx) are continuous, where ρ ∈ I1 (h) and tr(·) denotes the trace. The predual space of a von Neumann algebra M, which is the Banach space of all σ-weakly continuous linear functionals on M, is denoted A∗ , in particular, L(h)∗ = I1 (h), the space of trace-class operators. Any quantum Markov semigroup T on M induces a predual semigroup T∗ on A∗ defined by (1) T∗t (ω)(a) = ω (Tt (a)) , for all ω ∈ A∗ , a ∈ M, t ≥ 0. The cone of positive elements in the algebra M is denoted M+ . The space of normal states is S = {ω ∈ A+ ∗ : ω(1) = 1}, where 1 denotes the identity in M. A function t : D(t)×D(t) → C, where D(t) is a subspace of h, is a sesquilinear form over a Hilbert space h if t(v, u) is antilinear in v and linear in u. The set of all sesquilinear forms over h is denoted F(h). The form is said to be densely defined if its domain D(t) is dense, symmetric if t(v, u) = t(u, v), for all u, v ∈ D(t), and positive if t(u, u) ≥ 0, for all u ∈ D(t). We follow Bratteli and Robinson [12] to recall some useful properties of forms. A quadratic form u → t(u, u) is associated to each sesquilinear form t. This quadratic form determines t by polarization. A positive quadratic form is said to be closed whenever the conditions


165

1. un ∈ D(t), 2. un − u → 0, imply that u ∈ D(t) and t(un − u, un − u) → 0. Moreover, the quadratic form u → t(u, u) is densely defined, positive and closed if and only if there exists a unique positive selfadjoint operator T such that D(t) = D(T 1/2 ) and t(v, u) = T 1/2 v, T 1/2 u, for all u, v ∈ D(t). In that case it holds in particular that t(v, u) = v, T u, for any u ∈ D(T ), v ∈ D(t).

2 Ergodic Theorems We start analyzing the simpler of our problems which is the convergence of Cesàro means of a given quantum Markov semigroup. Indeed this problem is simpler due to the following well known fact. Proposition 2.1. The unit ball of L(h) is w∗ -compact. Proof. Indeed this follows from Alaoglu-Bourbaki theorem and the fact that L(h) is the topological dual of the Banach space I1 (h) endowed with the norm T → tr(|T |) (see [11], Proposition 2.4.3, p.68). Thus, given a ∈ M, the ball Ba = {x ∈ L(h) : x ≤ a} is w∗ -compact. Moreover, given any quantum Markov semigroup T , the orbit of a ∈ M is T (a) = {Tt (a) ∈ M : t ≥ 0} . We call co(T (a)) the convex hull of the orbit and we denote co(T (a)) its w∗ closure. As a result we have Corollary 2.1. Given any quantum Markov semigroup on M, and any a ∈ M, the set co(T (a)) is compact in the w∗ -topology. Proof. Indeed, since Tt (a) ≤ a we have that co(T (a)) ⊆ Ba , is a closed subset of a compact set. Here however, we are looking for more applicable results, thus, the use of sequences (or, say, criteria for sequential w∗ -compactness) will be sufficient for our purposes. Proposition 2.2. For any a ∈ M the w∗ -limit of any sequence tn 1 Ts (a)ds; n ≥ 0 , tn 0 with tn → ∞, is Tt -invariant, for all t ≥ 0.

166


Proof. Call b one of these limit points, i.e. b = w∗ − lim n

1 tn

tn

Ts (a)ds.

0

Then 1 tn Ts+r (a)ds n tn 0 1 tn +r ∗ Ts (a)ds = w − lim n tn r tn tn +r r 1 ∗ Ts (a)ds + Ts (a)ds − Ts (a)ds = w − lim n tn tn 0 0 1 tn = w∗ − lim Ts (a)ds. n tn 0

Tr (b) = w∗ − lim

Now, we would like to say a word about the convergence of states, which requires some additional notions. Definition 2.1. A sequence of states (ωn )n is said to converge narrowly to ω ∈ S if it converges in the weak topology of the Banach space A∗ i.e. lim ωn (x) = ω(x)

n→∞

for all x ∈ M. A sequence of states (ωn )n is tight if for any > 0 there exists a finite rank projection p ∈ M and n0 ∈ N such that ωn (p) ≥ 1 − , for all n ≥ n0 . Theorem 2.1. Any tight sequence of states on L(h) admits a narrowly convergent subsequence. The reader is referred to [19] Lemma 4.3 p.291 or [49] Theorem 2 p.27 (see also [44] Appendix 1.4) for the proof. A detailed exposition of this kind of results is contained in [17]. Corollary 2.2. Suppose that M = L(h). If for each state ω the family 1 t

t

T∗s (ω)ds,

t>0

0

is tight, then each sequential limit point of the family is invariant under T∗ .


167

The proof of this corollary is completely similar to Corollary 2.2 and it is omitted. We denote F (T )the set of fixed points of T in M. A straightforward generalization of Proposition 2.2, shows that any limit point of the family of Cesàro means of the orbit T (a) (indeed any limit point of co(T (a))) belongs to F (T ), for any a ∈ M. To prove the convergence of the whole family it suffices to prove that co(T (a)) ∩ F (T ) is reduced to a single point. If the existence of a faithful, normal, stationary state ω is assumed, then F (T ) becomes a von Neumann subalgebra of M. Moreover, this subalgebra is globally invariant under the modular automorphism σtω introduced in the theory of Tomita and Takesaki (see [11, 12], [38]), since σtω (·) and Tt (·) commute. Therefore, there exists a faithful normal conditional expectation E F (T ) which satisfies CE1 E F (T ) : M → F (T ) is linear, w∗ –continuous, completely positive, CE2 E F (T ) (1) = 1, CE3 ω ◦ E F (T ) = ω, and E F (T ) (aE F (T ) (b)) = E F (T ) (a)E F (T ) (b), for all a, b ∈ M. The above characterization contains the Ergodic Theorem for QMS. Indeed E F (T ) is unique since, given any other map E which satisfies CE1, CE2, CE3, it follows that E F (T ) = E ◦ E F (T ) = E F (T ) ◦ E = E. More precisely, Theorem 2.2. If ω is a faithful, normal state which is invariant under T , then there exists a unique normal conditional expectation E F (T ) onto F (T ). In addition, E F (T ) ◦ Tt (·) = E F (T ) (·) for all t ≥ 0; for any element a ∈ M, E F (T ) (a) belongs to the w∗ –closure co(T (a)) of the convex hull of the orbit T (a) = (Tt (a))t≥0 . Moreover, invariant states under the action of the predual semigroup (T∗t )t≥0 , are elements of the form ϕ ◦ E F (T ) of the predual M∗ , where ϕ runs over all states defined on the algebra F (T ). Since the paper of S.Ch.Moy [45], several authors have studied the construction of conditional expectations in a non-commutative framework, in particular Umegaki [58], Takesaki [57], Accardi and Cechini [1] (see eg. the survey included in the work of Petz [48]). As we have pointed out along this section, the concept of a conditional expectation is crucially related to the existence of invariant states and Cesàro (or Abel) limits.

3 The Minimal Quantum Dynamical Semigroup Throughout this chapter, which is merely expository, we consider the von Neumann algebra M = L(h) and we rephrase, for easier reference the crucial result which allows to construct a quantum dynamical semigroup starting from a generator given as a sesquilinear form. For further details on this matter we refer to [26], section 3.3, see also [15]. Let G and L , ( ≥ 1) be operators in h which satisfy the following hypothesis:

168


– (H-min) G is the infinitesimal generator of a strongly continuous contraction semigroup in h, D(G) is contained in D(L ), for all ≥ 1, and, for all u, v ∈ D(G), we have Gv, u +

∞

L v, L u + v, Gu = 0.

=1

Under the above assumption (H-min), for each x ∈ L(h) let −(x) L ∈ F(h) be the sesquilinear form with domain D(G) × D(G) defined by −(x)(v, L u) = Gv, xu +

∞

L v, xL u + v, xGu.

(2)

=1

It is well-known (see e.g. [20] Sect.3, [26] Sect. 3.3) that, given a domain D ⊆ D(G), which is a core for G, it is possible to built up a quantum dynamical semigroup, called the minimal QDS, satisfying the equation: t v, Tt (x)u = v, xu + −(T L s (x))(v, u)ds, (3) 0

for u, v ∈ D. This equation, however, in spite of the hypothesis (H-min) and the fact that D is a core for G, does not necessarily determine a unique semigroup. The minimal QDS is characterized by the following property: for any w∗ -continuous family (Tt )t≥0 of positive maps on L(h) satisfying (3) we have Tt(min) (x) ≤ Tt (x) for all positive x ∈ L(h) and all t ≥ 0 (see e.g. [26] Th. 3.21). (min) denote the predual semigroup on I1 (h) with infinitesimal generator Let T∗ (min) (min) L∗ . It is worth noticing here that T∗ is a weakly continuous semigroup on the Banach space I1 (h), hence it is strongly continuous. The linear span V of elements (min) of I1 (h) of the form |uv| is contained in the domain of L∗ . Thus we can write the equation (3) as follows t (min) tr(L∗ (|uv|)Ts (x))ds. tr(|uv|Tt (x)) = tr(|uv|x) + 0

This equation reveals that the solution to (3) is unique whenever the linear manifold (min) (V) is big enough. Indeed, the following characterization holds. L∗ Proposition 3.1. Under the assumption (H-min) the following conditions are equivalent: (min)

(i) the minimal QDS is Markov (i.e. Tt (1) = 1), (min) (ii) (Tt )t≥0 is the unique w∗ -continuous family of positive contractive maps on L(h) satisfying (3) for all positive x ∈ L(h) and all t ≥ 0, (min) (iii) the domain V is a core for L∗ ,


169

(iv) for all λ > 0, the unique solution x to −(x) L = λx, in the form sense, is x = 0. The equivalence of (i) and (iii) (resp. (i) and (ii)) have been proved in [20] Th. 3.2 and also in [26] Prop. 3.31 (resp. [26] Th. 3.21). For the sake of completeness we sketch this proof below. Proof. For any u, v ∈ V, x ∈ L(h), the equation (3) can be written as (min)

tr(xT∗t

(|uv|)) = tr(x|uv|) +

t/ 0 v, −(T L s(min) (x))u ds. 0

So that, 0 1 1 t/ (min) tr(x T∗t (|uv|) − |uv| ) = [ Gv, Ts(min) (x) u t t 0 ∞ / 0 L v, Ts(min) (x) L u + =1

0 / + v, Ts(min) (x) Gu ]ds. The functions of s appearing in the right-hand side of the previous equation are all continuous and (H-min) implies that / 0 L v, Ts(min) (x) L u ≤ L v L u , for all ≥ 1. Moreover, ∞

L v L u ≤

&∞

=1

'1/2 & 2

L v

=1

∞

'1/2 2

L u

=1

= (−2Rev, Gv)1/2 (−2Reu, Gu)1/2 , so that the series of the left-hand side converges and the function s →

∞ /

0 L v, Ts(min) (x) L u ,

=1

is continuous by Lebesgue’s theorem on dominated convergence. So that, 1 (min) lim tr(x T∗t (|uv|) − |uv| ) = v, −(x)u. L t→0 t (min)

Therefore, since the weak and the strong generators of T∗ coincide, the rang-one operator |uv| belongs to the domain of L∗ for all u, v ∈ D(G) and L∗ (|uv|) = |Guv| +

∞ =1

|L uL v| + |uGv|.

(4)

170


We now go into the proof of the equivalence of all conditions (i) to (iv). Notice that, under the hypothesis (H-min), one has v, −(1)u L = 0 for all u, v ∈ D, so that the constant family of operators t → 1 solves the equation (3). Therefore, (i) follows immediately from (ii). On the other hand, if (i) holds, let T be another contractive quantum dynamical semigroup solving (3). Then, for any x ∈ L(h) such that 0 ≤ x ≤ 1 and all t ≥ 0 we have, (min)

Tt

(x) ≤ Tt (x) = Tt (1) − Tt (1 − x) ≤ 1 − Tt (1 − x) (min)

≤ 1 − Tt =

(min) Tt

(1 − x)

(x) .

Since each operator y in L(h) can be written as a linear combination of four such (min) (y) = Tt (y) for any y ∈ L(h) and (i) is operators x before, it follows that Tt equivalent to (ii). Since V is trace-norm dense in the Banach space of trace-class operators, V is a core for L∗ if and only if the ortogonal complement of the linear manifold (λI − L∗ )(V) in L(h) is trivial for some λ > 0 (see e.g. [24], Prop. 3.1). Suppose (iv), then if x is an element of the above orthogonal complement, it holds tr((λI − L∗ )(|uv|)x) = 0, that is, −(x) L = λx in the form sense. So that x = 0 by (iv) and V is a core for L∗ , that is (iv) implies (iii). Reciprocally assume (iii) to be true. If there exists a solution x = 0 of −(x) L = λx for a λ > 0, then (λI − L∗ )(V) is not trivial, so that V is not a core for the predual generator, contradicting (iii). Thus, (iii) and (iv) are equivalent. For every ρ ∈ V, we have tr(L∗ (ρ)) = 0. Under condition (iii) the above identity holds for any ρ in the domain of L∗ and d (min) (min) tr(T∗t (ρ)) = tr(L∗ (T∗t (ρ))) = 0, dt (min)

thus, tr(T∗t (ρ)) = tr(ρ), for all t ≥ 0 and every trace class operator ρ because V is dense with respect to the trace norm. Thus, T (min) is Markov. That is, (iii) implies (i). The proof that (i) implies (iv) is more technically involved and the interested reader is referred to [26], Prop.3.30 to conclude. However, just to give a flavor of the main idea used in this part of the proof, suppose that L(x) is a bounded operator. If (iv) does not hold, there exists λ > 0 and x ∈ B(HS ) such that L(x) = λx. In this case Tt (x) = exp(λt)x. Notice that −2 x 1 ≤ (x + x∗ ) ≤ 2 x 1,

(5)

−2 x 1 ≤ i(x − x∗ ) ≤ 2 x 1.

(6)


171

If we apply Tt (·) to (5) and use the fact that the semigroup is Markov, we obtain −2 x 1 ≤ eλt (x + x∗ ) ≤ 2 x 1, for all t ≥ 0. This is a contradiction, so that necessarily x + x∗ = 0, working similarly with (6) yields the conclusion that x = 0 and (iv) holds. Assume that the minimal QDS is Markov and call (Pt )t∈R+ R+ the semigroup of contractions generated by G, then the equation (3) may be written in an equivalent form as t L Pt−s v, Tt (x)L Pt−s uds, (7) v, Tt (x)u = Pt v, xPt u + ≥1

0

Moreover, the solution to (7) is obtained as the supremum of an approximating sequence (T (n) )n∈N defined recursively as follows on positive elements x ∈ L(h): (0)

Tt

(x) = Pt∗ xPt

(n+1) u, Tt (x)u

(8)

= Pt u, xPt u (9) t (n) L Pt−s u, Tt (x)L Pt−s uds, (u ∈ D(G)). + ≥1

0

For any positive element x ∈ L(h) the above sequence is increasing with n. This (n) allows to define Tt (x) = supn Tt (x). T is the Minimal Quantum Markov semigroup, (see for instance [26]). The previous discussion has shown the importance of getting a minimal quantum dynamical semigroup which preserves the identity, that is, a quantum Markov semigroup. Recently A.M. Chebotarev and the first author have obtained easier criteria to verify the Markov property. For instance, the following result ( [14] Th. 4.4 p.394) which will be good enough to be applied in our framework. Proposition 3.2. Under the hypothesis (H-min) suppose that there exists a selfadjoint operator C in h with the following properties: (a) the domain of G is contained in the domain of C 1/2 and is a core for C 1/2 , (b) the linear manifold L (D(G2 )) is contained in the domain of C 1/2 , (c) there exists a self-adjoint operator Φ, with D(G) ⊆ D(Φ1/2 ) and D(C) ⊆ D(Φ), such that, for all u ∈ D(G), we have −2Reu, Gu = L u2 = Φ1/2 u2 ,

(d) for all u ∈ D(C ) we have Φ u ≤ C 1/2 u, (e) for all u ∈ D(G2 ) the following inequality holds 1/2

2ReC

1/2

1/2

u, C

1/2

Gu +

∞

C 1/2 L u2 ≤ bC 1/2 u2

=1

where b is a positive constant depending only on G, L , C.

(10)

172


Then the minimal QDS is Markov. As shown in [26] the domain of G2 can be replaced by a linear manifold D which is dense in h, is a core for C 1/2 , is invariant under the operators Pt of the contraction semigroup generated by G, and enjoys the properties: R(λ; G)(D) ⊆ D(C 1/2 ),

L (R(λ; G)(D)) ⊆ D(C 1/2 )

where R(λ; G) (λ > 0) are the resolvent operators. Moreover the inequality (10) must be satisfied for all u ∈ R(λ; G)(D). We finish this section giving a useful criterion to characterize the domain of the generator, assuming two hypothesis: (H-min) of section 3 and (H-Markov) that the minimal QDS is Markov. We recall that, as in section 3, D is a core for G. Moreover, V the linear manifold generated by the rank-one operators |uv|, where u, v ∈ D, is a core for L∗ . Lemma 3.1. Under the above hypotheses the domain of L is given by all the elements X ∈ B(h) for which the application (v, u) → −(X)(v, L u) is norm– continuous in the product Hilbert space. Proof. We remark that X ∈ D(L) if and only if the linear form ρ → tr(L∗ (ρ)X), defined on D(L∗ ), is continuous for the norm · 1 of I1 (h), since L = (L∗ )∗ . So that the essential of the proof consists in establishing the equivalence of the above property with the continuity of (v, u) → −(X)(v, L u) as stated. Moreover, the reader will agree that the latter is a necessary condition for X being an element of D(L), so that it remains to prove the sufficiency. Indeed, if L(X) is bounded then it is represented by Y = L(X) ∈ L(h). Then for any ρ ∈ V, the computation of tr(()L∗ (ρ)X) yields |tr(L∗ (ρ)X)| = |tr(ρY )| ≤ ρ1 Y . The proof is then completed by a standard argument based on the core property of V.

4 The Existence of Stationary States This section is aimed at finding a criterion for the existence of stationary states for a quantum Markov semigroup whose generator is unbounded and known as a sesquilinear form. We will be concerned with the case M = L(h) again. 4.1 A General Result We begin by introducing a notation for truncated operators in L(h).


173

Definition 4.1. For each self-adjoint operator Y , bounded from below, we denote by Y ∧ r the truncated operator Y ∧ r = Y Er + rEr⊥

(11)

where Er denotes the spectral projection of Y associated with the interval ]−∞, r]. We are now in a position to prove our first result on the existence of normal stationary states. Theorem 4.1. Let T be a quantum Markov semigroup. Suppose that there exist two self-adjoint operators X and Y with X positive and Y bounded from below and with finite dimensional spectral projections associated with bounded intervals such that t u, Ts (Y ∧ r)uds ≤ u, Xu (12) 0

for all t, r ≥ 0 and all u ∈ D(X). Then the QMS T has a normal stationary state. Proof. Let −b (with b > 0) be a lower bound for Y . Note that, for each r ≥ 0 we have Y ∧ r ≥ −bEr + rEr⊥ = −(b + r)Er + r1 so that (12) yields

t

−(b + r)

u, Ts (Er )uds + rtu2 ≤ u, Xu 0

for all u ∈ D(X). Normalize u and denote by |uu| the pure state with unit vector u. Dividing by t(b + r), for all t, r > 0 we have then 1 t

t

tr(T∗s (|uu|)Er )ds ≥ 0

It follows that the family of states 1 t T∗s (|uu|) ds, t 0

u, Xu r − . b + r t(b + r)

t>0

is tight. The conclusion follows then from Theorem 2.1 and Corollary 2.2. Remark. It is worth noticing that we wrote the inequality (12) truncated (integral on [0, t], and Y ∧ r) to cope with two difficulties: the divergence of the integral and the unboundedness of Y . Defining appropriately the supremum of a family of self-adjoint operators and then the potential U for positive self-adjoint operators, the formula (12) can be written as U(Y ) ≤ X.

174


This also throws light on the classical potential-theoretic meaning of our condition which is currently under investigation. In the applications, however, the inequality (12) is hard to verify since very frequently the QMS is not explicitly given. Therefore we shall look for conditions involving the infinitesimal generator. To this end we introduce now the class of QMS with possibly unbounded generators that concerns our research. This is sufficiently general to cover a wide class of applications. 4.2 Conditions on the Generator Here we use the notations and hypotheses of the previous chapter yielding to the construction of the minimal quantum dynamical semigroup associated to a given form-generator. Definition 4.2. Given two selfadjoint operators X, Y , with X positive and Y bounded from below, we write −(X) L ≤ −Y on D, whenever Gu, Xu +

∞

X 1/2 L u, X 1/2 L u + Xu, Gu ≤ −u, Y u,

(13)

=1

for all u in a linear manifold D dense in h, contained in the domains of G, X and Y , which is a core for X and G, such that L (D) ⊆ D(X 1/2 ), ( ≥ 1). Theorem 4.2. Assume that the hypothesis (H-min) of the previous chapter holds and that the minimal QDS associated with G, (L )≥1 is Markov. Suppose that there exist two self-adjoint operators X and Y , with X positive and Y bounded from below and with finite dimensional spectral projections associated with bounded intervals, such that (i) −(X) L ≤ −Y on D; (ii) G is relatively bounded with respect to X; (iii)L (n + X)−1 (D) ⊆ D(X 1/2 ), (n, ≥ 1). Then the minimal quantum dynamical semigroup associated with G, (L )≥1 has a stationary state. It is worth noticing that the above sufficient conditions always hold for a finite dimensional space h. Indeed, by the hypothesis (H-min), it suffices to take X = 1, Y = 0 and D = h. We begin the proof by building up approximations T (n) of T (min) . Lemma 4.1. Under the hypotheses of Theorem 4.2, for all integer n ≥ 1 the opera(n) tors G(n) and L with domain D defined by G(n) = nG(n + X)−1 ,

(n)

L

= nL (n + X)−1 ,


admit a unique bounded extension. The operator on L(h) defined by (n)∗ (n) L xL + xG(n) L(n) (x) = G(n)∗ x +

175

(14)

(n ≥ 1) generates a uniformly continuous quantum dynamical semigroup T (n) . (n)

Proof. First notice that G(n) and the L ’s are bounded. Indeed, by the hypothesis (ii), the resolvent (n + X)−1 maps h into the domain of the operators G and L , (n) therefore, G(n) and L are everywhere defined. Moreover, since G is relatively bounded with respect to X, there exist two constants c1 , c2 > 0 such that, for each u ∈ h we have nG(n + X)−1 u ≤ c1 nX(n + X)−1 u + c2 n(n + X)−1 u. By well known properties of the Yosida approximation the right hand side is bounded by (nc1 + c2 )u. On the other hand, by (H-min), for each u ∈ h we also have ∞

nL (n + X)−1 u2 = −2Ren(n + X)−1 u, G(n) u ≤ 2(nc1 + c2 )u2 .

=1 (n)

Thus the L ’s are bounded. Moreover, replacing u, v in condition (H-min) by n(n + X)−1 u, u ∈ h, leads to u, L(n) (1)u = 2Reu, G(n) u +

∞

(n)

L u2 = 0.

=1

∞ (n)∗ (n) It follows that the sum =1 L L converges strongly. Therefore by Lindblad’s theorem, the equation (14) defines the generator of a uniformly continuous quantum Markov semigroup. We recall the following well-known result on the convergence of semigroups Proposition 4.1. Let A, A(n) ( n ≥ 1) be infinitesimal generators of strongly con(n) tinuous contraction semigroups (Tt )t≥0 , (Tt )t≥0 on a Banach space and let D0 be a core for A. Suppose that each element x of D0 belongs to the domain of A(n) for n big enough and the sequence (A(n) x)n≥1 converges strongly to Ax. Then the (n) operators Tt converge strongly to Tt uniformly for t in bounded intervals. We refer to [41] Th. 1.5 p.429, Th. 2.16 p. 504 for the proof. We shall need also the following elementary lemma. (n)

Lemma 4.2. Let (r )≥1 , (s )≥1 ( n ≥ 1) be square-summable sequences of pos(n) itive real numbers. Suppose that, for every ≥ 1, s is an infinitesimum as n tends to infinity and that there exists a positive constant c such that

176


(n)

2

s

≤c

≥1

for every n ≥ 1. Then lim

n→∞

(n)

r s

= 0.

≥1

Proof. Suppose that our conclusion is false. Then, by extracting a subsequence (in n) if necessary, we find an ε > 0 such that, for every n, (n) r s > ε. (15) ≥1

The sequences s(n) may be understood as vectors in l2 (N) uniformly bounded in norm by c. Therefore we can extract a subsequence (nm )m≥1 such that (s(nm ) )m≥1 (n) converges weakly as m tends to infinity. Since s is an infinitesimum as n tends to infinity for each ≥ 1, it follows that the weak limit must be the vector 0. This contradicts (15). (n)

Lemma 4.3. Let G(n) , L the operators on h defined in Lemma 4.1. Then, under the hypotheses of Theorem 4.2, for all u ∈ D(X), we have (n)

lim G(n) u = Gu,

lim L u = L u.

n→∞

n→∞

(n)

Moreover the operators T∗t on I1 (h) converge strongly, as n tends to infinity, to T∗t , uniformly for t in bounded intervals. Proof. For all u ∈ D(X), we have " " " " " (n) " "G u − Gu" = "G(n(n + X)−1 − 1)u" " " " " ≤ c1 "(n(n + X)−1 − 1)Xu" + c2 "(n(n + X)−1 − 1)u" . Therefore the sequence G(n) u n≥1 converges strongly to Gu as n tends to infinity by well-known properties of Yosida approximations. Moreover, by (H-min), for u ∈ D(X), we have also ∞ " "2 " (n) " "L u − L u" = −2Re (n(n + X)−1 − 1)u, G(n(n + X)−1 − 1)u . =1

(n) This shows the convergence of sequences L u For all u, v ∈ D(X) we have (n)

(min)

L∗ (|uv|) − L∗

(16) n≥1

to L u for all ≥ 1.

(|uv|) = |(G(n) − G)uv| + |u(G(n) − G)v| ∞ (n) + |(L − L )uv| =1

+

∞ =1

(n)

|u(L

− L )v|.

Notes on the Qualitative Behaviour of Quantum Markov Semigroups (n)

(min)

Therefore the trace norm of L∗ (|uv|) − L∗

177

(|uv|) can be estimated by

v · (G(n) − G)u + u · (G(n) − G)v ∞ ∞ (n) (n) + L u · (L − L )v + L v · (L − L )u. =1

=1

Clearly the first two terms vanish as n tends to infinity. Moreover, by the inequality (16), since the operators X(n + X)−1 are contractive, we have ∞ " "2 " (n) " "L u − L u" ≤ 2(n + X)−1 Xu · (G(n) − G)u =1

" " " " ≤ 2u c1 "(n(n + X)−1− 1)Xu" + c2 "(n(n + X)−1− 1)u" " " " " = 2u c1 "(X(n + X)−1 )Xu" + c2 "(X(n + X)−1 )u" ≤ 2u (c1 Xu + c2 u) . (n)

An application of Lemma 4.2 shows then that the trace norm of L∗ (|uv|) − (min) L∗ (|uv|) converges to 0 as n tends to infinity. Since the minimal QDS associated with G, (L )≥1 is Markov and D(X) is a core for G (it contains D), the linear manifold generated by |uv| with u ∈ D(X) (min) is a core for L∗ . The conclusion follows then from Proposition 4.1. Lemma 4.4. Let Y ∧ r the operator defined by (11) and let X (n) = nX(n + X)−1 , (n) (n ≥ 1). Define Yr = n2 (n+X)−1 (Y ∧r)(n+X)−1 . Then, under the hypotheses of Theorem 4.2, the operator t (n) X − Ts(n) (Yr(n) )ds, 0

is positive for each t ≥ 0. Proof. Notice that Yr ≤ Y . Therefore, by the hypothesis (i) of Theorem 4.2, we have the inequality Gu, Xu +

∞ X 1/2 L u, X 1/2 L u + Xu, Gu ≤ −u, (Y ∧ r)u,

(17)

=1

for all u ∈ D. The domain D being a core for X and G being relatively bounded with respect to X, for every u ∈ D(X) we can find a sequence (un )n≥1 in D such that (Xun )n≥1 converges to Xu and (Gun )n≥1 converges to Gu. Then the convergence of (L un )n≥1 to L u (for all ≥ 1) follows readily from the hypothesis (H-min). Moreover, for every n, m ≥ 1, the inequality (17) yields ∞

X 1/2 L (un − um )2 ≤ −2ReG(un − um ), X(un − um )

=1

− (un − um ), (Y ∧ r)(un − um ).

178


Therefore, replacing u by un , and letting n tend to infinity we show that (17) holds for all u ∈ D(X). Since n(n + X)−1 is a contraction and Yr ≤ Y , under the hypotheses of Theorem 4.2, for all u ∈ h we have u, L(n) (X (n) )u ≤ 2ReG(n) u, X (n) u +

∞

(n)

(n)

X 1/2 L u, X 1/2 L u

=1

≤ −n(n + X)−1 u, Yr n(n + X)−1 u = −u, Yr(n) u. (n)

It follows then L(n) (X (n) ) ≤ −Yr . Now, notice that t d (n) (n) (n) (n) (n) Ts (Yr )ds X − Tt (X ) − dt 0 (n) L(n) (X (n) ) + Yr(n) = −Tt ≥ 0. Therefore,

t

X (n) −

(n)

Ts(n) (Yr(n) )ds ≥ Tt

(X (n) ) ≥ 0

0

for all t ≥ 0. Proof. (of Theorem 4.2). By Lemma 4.4 for each u ∈ D(X), t, r ≥ 0 and n ≥ 1, we have t

(n)

tr(T∗s (|uu|)Yr(n) )ds ≤ u, X (n) u. 0 (n) (Yr )n≥1

converges strongly to Y ∧ r. Thus, by Lemma 4.3, we can The sequence let n tend to infinity to obtain t tr(T∗s (|uu|)(Y ∧ r))ds ≤ u, Xu. 0

This inequality coincides with (12). Therefore Theorem 4.2 follows from Theorem 4.1.

4.3 Examples 4.4 A Multimode Dicke Laser Model We follow Alli and Sewell [4] where a model is proposed for a Dicke laser or maser. We begin by establishing the corresponding notations.


179

The system consists of N identical two-level atoms coupled with a radiation field corresponding to n modes. Therefore, one can choose the Hilbert space h which consists of the tensor product of N copies of C2 and n copies of l2 (N). To simplify notations we simply identify any operator acting on a factor of the above tensor product with its canonical extension to h. Let σ1 , σ2 , σ3 be the Pauli matrices and define the spin raising and lowering operators σ± = (σ1 ± iσ2 )/2. The atoms are located on the sites r = 1, . . . , N of a one dimensional lattice, so that we denote by σ,r ( = 1, 2, 3, +, −) the spin component of the atom at the site r. The free evolution of the atoms is described by a generator Lmat which is bounded and given in Lindblad form as Lmat (x) = i[H, x] −

1 ∗ (Vj Vj x − 2Vj∗ xVj + xVj∗ Vj ), 2 j

(18)

where the sum contains a finite number of elements, H is bounded self-adjoint and the Vj ’s are bounded operators. Moreover, we denote by a∗j , aj , the creation and annihilation operators corresponding to the j-th mode of the radiation, (j = 1, . . . , n). These operators satisfy the canonical commutation relations: [aj , a∗k ] = δjk 1, [aj , ak ] = 0. The free evolution of the radiation is given by the formal generator Lrad (x) =

n

(κ (−a∗ a x + 2a∗ xa − xa∗ a ) + iω [a∗ a , x]) ,

(19)

=1

where κ > 0 are the damping and ω ∈ R are the frequencies corresponding to the -th mode of the radiation. The coupling between the matter and the radiation corresponds to a Hamiltonian interaction of the form: Hint =

i N 1/2

N n

λ (σ−,r a∗ e−2πik r − σ+,r a e2πik r ),

(20)

r=1 =1

where k is the wave number of the -th mode and the λ’s are real valued, N independent coupling constants. With the above notations, the formal generator of the whole dynamics is given by (21) L(x) = Lmat (x) + Lrad (x) + i[Hint , x] To identify L and G in our notations, we use in force the convention on the abridged version of tensor products with the identity. That is, here we find √ (22) L = κ a , ( = 1, . . . , n) All the remaining L ’s are bounded operators. Among them a finite number (indeed at most 3N ) coincides with some of the Vj ’s appearing in (18) and the other vanish.

180


So that the operator G becomes formally: G=−

1 ∗ L L − i ω a† a − iH − iHint , 2

(23)

where the sum contains only a finite number of non zero terms. To make the above expression rigorous some preliminary work is needed. Call (fm )m≥0 the canonical orthonormal basis on the space l2 (N). In the radiation space, which consists of the tensor product of n copies of l2 (N), we denote ⊗ . . . ⊗ fα(n) , fα = fα(1) 1 n ()

where α = (α1 , . . . , αn ) and fα is an element of the canonical basis of the copy of l2 (N). Thus, (fα )α∈Nn is the canonical orthonormal basis of the radiation space. With these notations we have 1 √ √ α fα−1 if α > 0 ∗ a fα = α + 1fα+1 , a fα = , (24) 0 if α = 0 where 1 is the vector with a 1 at the th coordinate and zero elsewhere. Thus, the operator G is well defined over vectors of the form ufα where u ∈ C2N and the symbol of tensor product is dropped. It is well known (see [41], Thm. 2.7 p.499) that a perturbation of a negative selfadjoint operator, relatively bounded with relative bound less than 1, is the infinitesimal generator n of a contraction semigroup. Therefore, we choose X formally given by X = =1 a∗ a . That is, Xufα = |α|ufα , where, |α| = α1 + . . . + αn . Since X k ufα = |α|k ufα it follows that the linear span of vectors of the form ufα is a dense subset of the analytic vectors for X. Therefore, by a theorem of Nelson (see e.g. [53]), X is essentially self-adjoint on the referred domain. From now on we identify X with its closure which is selfadjoint. We show now that Hint is relatively bounded with respect to X. Let ξ be a finite linear combination of elements of√the form α . By Schwarz’ √ inequality, and √ √ uf$ elementary inequalities like t + s ≤ t + s ≤ 2(t + s), 2 ts ≤ t + −1 s, we obtain Hint ξ ≤ ≤ ≤ ≤

1 N 1/2 1 N 1/2 1 N 1/2 1 N 1/2

n N

|λ |(a∗ ξ + a ξ)

r=1 =1 N n

1/2 |λ | 4ξ, a∗ a ξ + 2ξ2

r=1 =1

N n

N n √ 2(|λ |2 ξ, a∗ a ξ)1/2 + 2 |λ |ξ

r=1 =1 n N r=1 =1

r=1 =1

(a∗ a ξ

−1

+

n N √ |λ | ξ) + 2 |λ |ξ 2

r=1 =1


Finally, by the elementary inequality

Hint ξ ≤

n =1

s ≤

√

n

n

=1 s ,

181

it follows

N N n n n1/2 ∗ 1 √ a a ξ + ( 2 + −1 |λ |)|λ |ξ N 1/2 r=1 =1 N 1/2 r=1 =1

≤ N 1/2 n1/2 Xξ +

1 N 1/2

N n √ ( 2 + −1 |λ |)|λ |ξ, r=1 =1

thus, choosing < (N n)−1/2 , the above inequality yields the required relative boundedness of Hint with respect to X. As a result, the operator G appears as a dissipative perturbation of − 12 X, relatively bounded with respect to X, with bound strictly less than 1. Therefore, G is the generator of a contraction semigroup. Moreover, the domain of G coincides with that of X and hypothesis (H-min) easily checked. To apply our main result, we fix the domain D as the space of vectors ξ which are finite linear combinations of the form ufα . Notice that this is an invariant for X, L ≤ −Y , we G, and all the L ’s. To identify an appropriate operator Y to have −(X) first perform the computation of −(X). L For the sake of clarity, we avoid handling forms in the computations below. However, the reader may easily notice that all the expressions are well defined since the domain D is invariant under the action of the operators X, G and L . Firstly, it holds Lmat (X) = 0, since the Vj ’s act on the tensor product of N copies of C2 and leave the domain D invariant. Secondly, a straightforward computation using the canonical commutation relations, yields Lrad (X) = −2

n

κ a† a .

=1

Another easy computation yields i[Hint , X] = −iN

−1/2

n N

λ (σ−,r a† e−2πik r + σ+,r a e2πik r ).

r=1 =1

Summing up,

−(X) L = −2

n =1

κ a† a

−

i N 1/2

n N

λ (σ−,r a† e−2πik r + σ+,r a e2πik r ).

r=1 =1

To identify Y it suffices to control the term i[Hint , X]. For each ξ ∈ D, it follows

182


|ξ, i[Hint , X]ξ| =

1 N 1/2

n N −2πik r ∗ 2πik r λ ξ, (σ−,r a e + σ+,r a e ξ r=1 =1

≤

N n 1 2|λ |ξ(a ξ + a∗ ξ) 2N 1/2 r=1 =1

≤

n N (ξ, a∗ a ξ + ξ, a a∗ ξ) 2N 1/2 r=1 =1

+

N n 1 |λ |2 ξ2 2N 1/2 r=1 =1

≤ N 1/2 ξ, Xξ +

N n N 1/2 n 1 ξ2 + |λ |2 ξ2 . 2 2N 1/2 r=1 =1

So that choosing 0 < < 2N −1/2 min κ the required operator Y may be taken as Y = (2 min κ − N 1/2 )(X + c), where c > 0 is a suitable constant. The spectrum of X coincides with N. For each m ∈ N, the corresponding eigenspace is generated by the fα with |α| = m. Therefore, it follows that all spectral projections of X and Y associated with bounded intervals are finite dimensional. Similar arguments allow to check the hypotheses of Proposition 3.2 (with C = X) to show that the minimal QDS associated to the operators G and L , (1 ≤ ≤ n), is Markov (this was also proved in [4] by another method). To summarize, our main theorem implies the following Corollary 4.1. There exists an invariant state for the multimode Dicke model. 4.5 A Quantum Model of Absorption and Stimulated Emission This example corresponds to a family of models introduced by Gisin and Percival in [37]. The framework is given by the Hilbert space h = l2 (N) where, as usual, we call (en )n∈N the canonical orthonormal basis. The operators defining the formgenerator −(·) L are L1 = νa† a, L2 = µa, H = ξ(a† + a), where µ, ν > 0 and ξ ∈ R. Thus,

1 2 † 2 ν (a a) + µ2 a† a , 2 Let us check the existence of an invariant state by means of Theorem 4.2. Take, for instance X = (N + 1)2 , where N = a† a is the number operator. A straightforwrd computation yields −(X) L = iξ (a − a† )(N + 1) + (N + 1)(a − a† ) + µ2 N (1 − 2N ). (25) G = −iξ(a† + a) −


183

We first study the term iξ (a − a† )(N + 1) + (N + 1)(a − a† ) , which corresponds to i[H, X]. Call D the linear manifold generated by (en )n∈N . For any u ∈ D, we have |u, i[H, X]| = |ξ| (a − a† )u, (N + 1)u " 1" ≤ "(a − a† )u" (N + 1)u " 2" " " ≤ "N 1/2 u" (N + 1)u 2 2 ≤ 2 u, N u + u, (N + 1)2 . 2 Thus, −(X) L ≤ −2µ2 N 2 + µ2 N +

2 2 (N + 1)2 + 2 N. 2

Finally, if we call 2 2 2 Y = 2µ2 − N 2 − µ2 + 2 + 2 N − 1, 2 2 we obtain −(X) L ≤ −Y. In a similar way one may verify that the quantum dynamical semigroup is Markov too. To summarize, Corollary 4.2. The quantum semigroup which corresponds to the model of absorption and stimulated emission here before is Markov and has a stationary state. 4.6 The Jaynes-Cummings Model We follow our article [27] to introduce the Jaynes-Cummings model in Quantum Optics. To this aim we use the same space h = l2 (N), since here n = 1, we drop the index from the notations of creation and annihilation operators and S denotes the right-shift operator. In this framework the formal generator is given by λ2 µ2 ∗ (a ax − 2a∗ xa + xa∗ a) − (aa∗ x − 2axa∗ + xaa∗ ) 2 2 √ √ √ √ + R2 (cos(φ aa∗ )x cos(φ aa∗ ) − x) + R2 sin(φ aa∗ )S ∗ xS sin(φ aa∗ ),

L(x) = −

where λ, µ, R and φ are positive constants. In [27] the rigorous construction of the minimal QDS was done showing also that it is identity preserving. The above Jaynes-Cummings generator has a faithful invariant state if and only if µ2 > λ2 . This state can be computed explicitly. The interested reader is referred to [27].

184


To check conditions of Theorem 4.2, one can take X = a∗ a, the value of L(X) becoming √ L(X) = −(µ2 − λ2 )a∗ a + R2 sin2 (φ aa∗ ). Thus, it suffices to take Y = (µ2 − λ2 )a∗ a − R2 to prove the existence of a stationnary state via our main result. To prove the necessity, one can follow the argument explained in [27] inspired from classical probability.

5 Faithful Stationary States and Irreducibility Consider a probability space (Ω, F, P), a measurable space (E, E) and a Markov process (Ω, F, P, (Ft )t∈R+ , E, E, (Xt )t∈) , defined on (Ω, F, P) with states in E. The Markov semigroup generated by this process is given by Tt f (x) = E (f (Xt )|X0 = x), for all t ≥ 0, x ∈ E and any bounded and measurable function f defined on E. A function f of the above class is subharmonic (resp. superharmonic, resp. harmonic) for the given semigroup if Tt f ≥ f (resp. Tt f ≤ f , Tt f = f ) for all t ≥ 0. Now take a positive measure µ on (E, E) and consider the von Neumann algebra M = L∞ (E, E, µ). A state ν over this von Neumann algebra is given by a probability measure ν absolutely continuous with respect to µ. The state ν is faithful whenever ν(f ) = 0, for a positive f ∈ M, implies that f = 0, (i.e. f (x) = 0, µ-almost surely). One important question then arises: when does (Tt )t∈R+ has a faithful stationary state in M? This question appears in the non-commutative theory of Markov semigroups as well. Indeed, the existence of a faithful stationary state is a crucial hypothesis in most of the ergodic studies developed in this field (see for instance section 2 before and [35], [36], [28], [29]). In a previous paper (see [31] and section 4) we obtained sufficient conditions for the existence of a stationary state of a given quantum Markov semigroup. 5.1 The Support of an Invariant State Definition 5.1. Given a semifinite von Neumann algebra M of operators over a complex separable Hilbert space h, endowed with a trace tr(·), and a Quantum Markov Semigroup (Tt )t∈R+ on M, a positive operator a ∈ M is subharmonic (resp. superharmonic, resp. harmonic) for the semigroup if Tt (a) ≥ a, (resp. Tt (a) ≤ a, resp. Tt (a) = a), for all t ≥ 0. Subharmonic events play a fundamental role in the Potential Theory of classical Markov semigroups. They are related to stationarity, recurrence, supermartingale properties. In our framework, we will start by showing a relation between invariant states and subharmonics projections.


185

Lemma 5.1. Let p be a projection of the von Neumann algebra M, and x ∈ M a positive element. If pxp = 0, then p⊥ xp = pxp⊥ = 0 Proof. Suppose M ⊆ B(h) and let u, v ∈ h with pu = u, pv = 0. Since x is positive, zu + v, x(zu + v) is positive for every z ∈ C. Then, since pxp = 0, for every z ∈ C, we have also 2Re (z v, xu) + v, xv ≥ 0. Therefore v, xu must vanish and the conclusion readily follows. Theorem 5.1. The support projection of a stationary state for a quantum Markov semigroup is subharmonic. Proof. Let p be the support projection of a given stationary state ρ of (Tt )t∈R+ . That is, p is the projection on the closure of the rank of ρ, thus ρp = pρ = ρ, and T∗t (ρ) = ρ, (for all t ≥ 0). Let be given an arbitrary t ≥ 0. We first notice that pTt (p)p ≤ p, since p ≤ 1. Therefore, tr(ρ(p − pTt (p)p)) = tr(ρ(p − Tt (p))) = 0, and, since ρ is faithful on the subalgebra pMp, it follows pTt (p)p = p. On the other hand, pTt (p⊥ )p = pTt (1)p − pTt (p)p = p − p = 0. Moreover, since Tt (p⊥ ) is positive, the previous lemma yields pTt (p⊥ )p⊥ = 0 = p⊥ Tt (p⊥ )p. To summarize,

Tt (p) = p + p⊥ Tt (p)p⊥ ,

and the projection p is subharmonic. Proposition 5.1. For any Quantum Markov semigroup T the following propositions are equivalent: a) p is subharmonic for T . b) The subalgebra p⊥ Mp⊥ is invariant for T . c) For any normal state ρ such that pρp = ρ, it holds tr(ρTt (p⊥ )) = 0, for all t ≥ 0. Proof. Assume that condition a) holds. By hypothesis, we have that pTt (p)p = p, thus pTt (p⊥ )p = pTt (1)p − pTt (p)p = 0.

186


Therefore, for any positive x ∈ p⊥ Mp⊥ it follows pTt (x)p = 0 since 0 ≤ pTt (x)p ≤ x pTt (p⊥ )p = 0. From Lemma 5.1, pTt (x)p⊥ = p⊥ Tt (x)p = 0, since Tt (x) is positive. Thus Tt (x) = p⊥ Tt (x)p⊥ ∈ p⊥ Mp⊥ . The same conclusion holds for any arbitrary x ∈ p⊥ Mp⊥ since all those elements may be decomposed as a linear combination of four positive elements of p⊥ Mp⊥ . Now we prove that b) implies c). By hypothesis, for any x ∈ p⊥ Mp⊥ , it holds Tt (x) = p⊥ yp⊥ for some y ∈ M. Clearly, y = Tt (x) since v, Tt (x)u = v, yu for all vectors u and v for which u = p⊥ u, v = p⊥ v. Therefore, Tt (x) = p⊥ Tt (x)p⊥ . In particular, Tt (p⊥ ) = p⊥ Tt (p⊥ )p⊥ . From this it follows that, given a state ρ such that pρ = ρp = ρ, we have p⊥ ρ = ρp⊥ = 0 which yields tr(ρTt (p⊥ )) = 0. We finally prove that c) implies a). From c) we obtain that tr(ρpTt (p⊥ )p) = 0, thus pTt (p⊥ )p = 0. As a result, by Lemma 5.1, Tt (p⊥ ) = p⊥ Tt (p⊥ )p⊥ ≤ p⊥ , which gives Tt (p) = Tt (1 − p⊥ ) ≥ p. Definition 5.2. We say that a quantum Markov semigroup is irreducible if there is no non-trivial subharmonic projection. 5.2 Subharmonic Projections. The Case M = L(h) Now we concentrate on the case of M = L(h). The quantum Markov semigroup is the minimal obtained from an unbounded generator given as a sesquilinear form −(x)(v, L u) = Gv, xu + L v, xL u + v, xGu, ≥1

under the hypotheses of section 3, that is, (H-min) is supposed satisfied and the associated minimal semigroup is assumed to be Markov. Thus, for all x ∈ L(h), the quadratic form −(x) L is defined over the domain D(G) × D(G). We refer the reader to section 3 for the notations and concepts connected with the minimal quantum Markov semigroup associated to −(·). L In which follows, we use the same notation p for both, a closed subspace and the projection determined by this subspace.


187

Lemma 5.2. Let (Pt )t∈R+ be the semigroup generated by G. Then a closed subspace p is invariant for (Pt )t∈R+ if and only if for any u ∈ D(G) ∩ Rk(p) it holds Gpu = pGpu. Proof. If p is invariant for the semigroup, Pt p = pPt p, then it is also invariant for the resolvent: R(λ; G)p = pR(λ; G)p. As a result for any u ∈ D(G) such that pu = u, if we define uλ = λR(λ; G)u, then we obtain puλ = uλ too. Therefore D(G) ∩ Rk(p) is dense in Rk(p). Moreover, for any u ∈ D(G) ∩ Rk(p) we have 1 1 1 p (Pt u − u) = (Pt pu − pu) = (Pt u − u) . t t t Therefore, letting t → ∞, we obtain Gpu = pGpu. Conversely, if Gpu = pGpu for all u ∈ D(G) ∩ Rk(p), then p⊥ Gp is zero on D(G) and d ⊥ p Pt pu = p⊥ GPt pu = (p⊥ Gp)Pt u = 0. dt It follows that p⊥ Pt pu = 0 for all u ∈ D(G) ∩ Rk(p) and t ≥ 0, hence p Pt p = 0 since D(G) ∩ Rk(p) is dense in Rk(p). ⊥

Theorem 5.2. Under the previous hypotheses, a projection p is subharmonic for T if and only if the following conditions are satisfied: Gpu = pGpu, L pu = pL pu,

(26)

for all u ∈ D(G) ∩ Rk(p), ≥ 1. Proof. We start assuming that p is subharmonic, thus Tt (p) ≥ p for all t ≥ 0. From equation (7) we obtain p⊥ ≥ Tt (p⊥ ) ≥ Pt∗ p⊥ Pt . Therefore, for all u ∈ Rk(p), " "2 u, Pt∗ p⊥ Pt u = "p⊥ Pt u" = 0, that is p⊥ Pt p = 0. Thus Pt p = pPt p, for all t ≥ 0. Then Lemma 5.2 implies that Gpu = pGu for all u ∈ D(G) ∩ Rk(p). In addition, the equation satisfied by the minimal quantum semigroup yields ⎛ ⎞ t ⎝Gu, Ts (p⊥ )u + L u, Ts (p⊥ )L u + u, Ts (p⊥ )Gu⎠ ds ≤ 0, 0

≥1

for all t ≥ 0 and all u ∈ D(G). As a result, computing the derivative in 0 of the above equation, we obtain:

188


Gu, p⊥ u +

L u, p⊥ L u + u, p⊥ Gu ≤ 0.

≥1

Now, if u ∈ D(G) ∩ Rk(p) the above inequality gives " " "p⊥ L pu"2 ≤ 0, ≥1

that is p⊥ L pu = 0 or, equivalently, pL pu = pL u, for all ≥ 1 and u ∈ D(G) ∩ Rk(p). Conversely, we assume condition (26). We will prove that p is subharmonic by an induction argument which relays on the sequence (T (n) )n∈N used in the construction of T . Firstly, p is subharmonic for T (0) since (0)

Tt

(p⊥ ) = Pt∗ p⊥ Pt = p⊥ Pt∗ p⊥ Pt p⊥ ≤ p⊥ .

Secondly, assume that p is subharmonic for T (n) , we prove that it is subharmonic for T (n+1) too. Indeed, for all u ∈ D(G) ∩ Rk(p), the definition of T (n+1) and the induction hypothesis yield t (n+1) ⊥ (p )u ≤ u, Pt∗ p⊥ Pt u + L Pt−s u, p⊥ L Pt−s uds = 0, u, Tt ≥1

0

for any t ≥ 0. (n+1) ⊥ (n+1) ⊥ (p )p = 0 and Lemma 5.1 implies p⊥ Tt (p )p = It follows that pTt (n+1) ⊥ ⊥ pTt (p )p = 0. Therefore, (n+1)

Tt

(p⊥ ) ≤ p⊥ ,

for all t ≥ 0 and p is subharmonic for T (n) . Hence, p is subharmonic for the minimal semigroup T and the proof is complete. 5.3 Examples Gisin-Percival Model of Absorption and Stimulated Emission, Continued We continue the analysis of the model introduced in 4.5, and refer to the notations therein. We want to characterize all common invariant closed subspaces for G, L1 , L2 . Since L1 is a multiple of the number operator N , its invariant subspaces IK are spanned by {ek : k ∈ K}, where K ⊆ N. However, notice that if K is finite and k0 = max K, to have IK invariant also for L2 , one needs to have all of the ek for k ≤ k0 inside IK , since L2 is a multiple of the annihilation operator. Define


189

h0 = {0}; hk , the space generated by {e0 , . . . , ek−1 } for any k ≥ 1 and h∞ = h. The unique collection of invariant subspaces for L1 and L2 is (hk )k∈N∪{∞} . As a result, if ξ = 0, there is a full collection of non trivial invariant subspaces. Suppose ξ = 0. In this case there is no hk invariant under G for k > 0. Therefore, the only common invariant spaces for G, L1 , L2 are trivial: h0 and h. As a result, the QMS has a faithful stationary state, say ρ∞ . Moreover, in the next section we will see that given any other state ρ, the semigroup T associated to (G, L1 , L2 ) satisfy that tr(T∗t (ρ)X) → tr(ρ∞ X), for all X ∈ L(h). This means that any other w∗ -limit of T∗t (ρ), ρ say, has to satisfy tr(ρ X) = tr(ρ∞ X) for any X ∈ L(h), so that ρ = ρ∞ due to the faithfulness of ρ∞ .

6 The Convergence Towards the Equilibrium To illustrate the results of this section we will restrict the proofs to the case of a norm-continuous semigroup. This is the framework of the seminal paper of Frigerio and Verri (see [36]. The case of a semigroup with unbounded generators has been treated by us in [29], (see also [33], [34]). Throughout this section we assume that the QMS has a faithful normal stationary state ρ and we want to derive conditions under which T∗t (σ) converges in the w∗ topology towards ρ as t → ∞, for any initial state σ. Under the above basic assumtion, there exists a conditional expectation x → EF(T ) (x) in the sense of Umegaki, defined over the von Neumann algebra F (T ) of invariant elements under the action of T . We recall an early result of Frigerio and Verri ( [36], Theorem 3.3, p.281). Denote N (T ) the set of elements x ∈ B(h) for which Tt (x∗ x) = Tt (x∗ )Tt (x) and Tt (xx∗ ) = Tt (x)Tt (x∗ ), for all t ≥ 0 Theorem 6.1 (Frigerio–Verri). If the semigroup T has a faithful stationary state ρ and the set of fixed points of T coincides with N (T ), then w∗ − lim Tt (x) = EF(T ) (x) , t→∞

(27)

for all x ∈ B(h). The basic idea of the proof consists in associating with T a strongly continuous contraction semigroup on the Hilbert space of the GNS representation based on the state ρ. Alternatively, one can prove that M decomposes as a direct sum of the von Neumann algebra N (T ) and a Banach space D (T ) which corresponds to the space of observables x for which lim ω (Tt (x)) = 0,

t→∞

(28)

190


for any state ω. Thus, given any x ∈ L(h), we can write x = EN(T ) (x) + to D (T ), so that given (x − EN(T ) (x)). The element (x − EN(T ) (x)) belongs any state ω, limt→∞ ω(Tt (x)) − ω(Tt (EN(T ) (x)) = 0. If N (T ) = F (T ), then Tt (EN(T ) (x)) = Tt (EF(T ) (x)) = EF(T ) (x) and lim ω(Tt (x)) − ω(EF(T ) (x)) = 0. t→∞

6.1 Main Results We begin by establishing a property of the space N (T ). Proposition 6.1. Under the assumption of this section about the existence of a faithful normal stationary state for the norm continuous quantum Markov semigroup T , the space N (T ) is a von Neumann algebra which coincides with the generalized commutator algebra of L = (Lk , L∗k ; k ≥ 1), denoted by L . Proof. The property of N (T ) being a von Neumann algebra is obtained in [36] through an application of Tomita-Takesaki theory (the conditional expectation exists since N (T ) is invariant under the modular automorphism associated to the faithful normal stationary state). Define Γ (x, y) := L(xy) − xL(y) − L(x)y, for all x, y ∈ L(h). As it was established in the previous chapter [52] of this volume, Γ (x∗ , x) ≥ 0 for any x ∈ L(h). Notice that x ∈ N (T ) if and only if Γ (x∗ , x) = 0 = Γ (x, x∗ ). A straightforward computation shows that (L∗k x∗ xLk − x∗ L∗k xLk + x∗ L∗k Lk x − L∗k x∗ Lk x) Γ (x∗ , x) = k≥1

=

∗

[Lk , x] [Lk , x].

k≥1

∗ ∗ Similarly, Γ (x, x∗ ) = k≥1 [L∗k , x] [L∗k , x]. Since each term [Lk , x] [Lk , x] (re∗ ∗ ∗ ∗ spectively [Lk , x] [Lk , x]) is positive, we have Γ (x , x) = 0 = Γ (x, x∗ ) if and ∗ only if [Lk , x] [Lk , x] = 0 for all k ≥ 1, which means that x is an element of L . Theorem 6.2. A norm continuous quantum Markov semigroup converges in the sense that w∗ − lim Tt (X) = T∞ (X), (29) t→∞

for all X ∈ B(h), whenever the generalized commutator L is reduced to the trivial algebra CI. Proof. This result follows straightforward from the Theorem of Frigerio and Verri, since N (T ) = L .


191

Proposition 6.2. Under the above hypotheses the set F (T ) of fixed elements for the semigroup is given by F (T ) = {Lk , L∗k , H; k ≥ 1}

(30)

Proof. Since F (T ) ⊂ N (T ), and N (T ) = L , it follows that F (T ) ⊂ L . So that, for all x ∈ F (T ) and any u, v ∈ h it holds: 0 = v, L(x)u ∞ ∞ 1 ∗ 1 =− Lk Lk v, xu + Lk v, xLk u 2 2 k=1

+

∞ 1

2

Lk v, xLk u −

k=1

k=1

∞ 1

2

v, xL∗k Lk u

k=1

− iHv, xu − v, ixHu. We now study the right hand side of the above equation. Since xLk = Lk x, the first two terms cancel and the computation Lk v, xLk u = x∗ Lk v, Lk u = Lk x∗ v, Lk u = x∗ v, L∗k Lk u, shows that the third and fourth terms cancel as well. From the above we deduce xH = Hx. Therefore, x belongs to {Lk , L∗k , H; k ≥ 1} . Reciprocally, if X ∈ {Lk , L∗k , H; k ≥ 1} , the equation for v, L(x)u gives 0 and we obtain that x is a fixed point of T . The corollary which follows is easily derived from the propositions and theorem before. Corollary 6.1. For any norm continuous quantum Markov semigroup, the convergence towards the equilibrium holds if {Lk , L∗k , H; k ≥ 1} = {Lk , L∗k ; k ≥ 1} . The sufficient condition obtained for proving the convergence towards the equilibrium is necessary, at least for a wide class of operators H, as we state in the following theorem. Theorem 6.3. Let be given a norm continuous quantum Markov semigroup for which H is a bounded self–adjoint operator with pure point spectrum. Then Tt (·) converges towards the equilibrium if and only if {Lk , L∗k , H; k ≥ 1} = {Lk , L∗k ; k ≥ 1} .

(31)

192


Proof. From the corollary before, (31) is a sufficient condition for the convergence towards the equilibrium. We will prove below that it is a necessary condition as well. Indeed, the hypotheses assumed imply that Tt (x) = eitH xe−itH , for all x ∈ N (T ). For any two different eigenvalues λ and µ of H, choose corresponding eigenvector v, u ∈ h. Then, e−itH v, xe−itH u = eit(µ−λ) v, Xu, converges when t → ∞. Therefore, v, xu = 0 and x commute with H. Consequently, {Lk , L∗k , H; k ≥ 1} = {Lk , L∗k ; k ≥ 1} . Remark 6.1. All the results of this section have been extended by the authors in [29] (see also [33], [34]) to QMS defined on L(h) with unbounded generators given as a form, under some suitable additional hypotheses. These hypotheses are the following: 1. The traditional hypothesis (H-min) used in the construction of the minimal semigroup. 2. The assumption that the minimal semigroup is Markov. 3. The existence of a domain D which is a core for both G and G∗ . 4. For all u ∈ D, the image R(n; G)u by the resolvent of G, belongs to D(G∗ ) and the sequence (nG∗ R(n; G)u)n≥1 strongly converges. This hypothesis, together with the previous one, allow to construct a quantum cocycle which is a dilation of the semigroup T . There exists also a dual cocycle and a corresponding semigroup T! . The last technical hypothesis is 5. The semigroup associated to the dual cocycle preserves the identity. We call natural a QMS which satisfies the above set of hypotheses. All the previous results still hold replacing norm continuous QMS by natural QMS with some minor changes which we precise below: In Prop.6.2 Suppose that the closure of H (which is unbounded) is self–adjoint. In Prop.6.1, 6.1,6.3 Suppose either that (a) H is bounded; or (b) H is selfadjoint and eitH (D) ⊂ D(G), 6.2 Examples The Asymptotic Behavior of the Jaynes–Cummings Model in Quantum Optics Here we consider again the model introduced in subsection 4.6, (see [27] and [28]), which is the quantum Markov semigroup associated to master equations in Quantum


193

Optics. The initial space is h = 2 (N) endowed with the creation (resp. annihilation) operator a† (resp. a), and the number operator denoted N . In addition, the coefficients G and Lk (k = 1, . . . , 4) are given by the expressions √ L1 = µa, L2 = λa† , L3 = R cos(φ aa† ), √ 4 † 1 ∗ † sin(φ aa ) √ , G=− Lk Lk , L4 = Ra 2 aa† k=1

where the parameters φ, R ≥ 0, λ < µ, specify the physical model. In this case the natural set D to choose is the domain of the number operator. Moreover, the existence of a stationary state for T has been proved in [27]. Indeed if λ < µ, then T has a stationary state given by ρ∞ =

∞

πn |en en |

n=0

where (πn )n≥0 is the sequence defined by π0 = c,

πn = c

√ n λ2 k + R2 sin2 (φ k) µ2 k

(n ≥ 1).

k=1

where c is a suitable normalization constant. The remaining hypotheses showing that the semigroup is natural have been checked in [27] as well. Now, to verify the hypotheses of Theorem 6.2, it suffices to study the action of operators on the canonical basis (em ; m ≥ 0) of h. In particular, it brings about a recurrence relationship among the elements of the basis from which it follows that er , Xem = 0 for all element X of the generalized commutator algebra of Lk , L∗k , (k = 1, . . . , 4). Corollary 6.2. The quantum Markov semigroup introduced before approaches the equilibrium in the sense of the w∗ topology, as t → ∞. As a trivial consequence of the above corollary, the Cesàro mean of the semigroup converge in the w∗ topology. This result had been stated in [28] with a different direct proof. A Class of Examples with a Non-Trivial Fixed Point Algebra Keeping the notations on spaces and operators of the above example, consider a quantum Markov semigroup with generator given by L1 = α(N ), Lk = 0, (k = 1), H = β(N ), with α and β given functions, α assumed to be injective and β real–valued. So that, any faithful state which is a function of the number operator is an invariant state.

194


In addition the algebras {Lk , L∗k , H; k ≥ 1} and {Lk , L∗k ; k ≥ 1} coincide with {N } if and only if the support of β is included in that of α. Therefore, the hypotheses of the Corollary are satisfied, whenever the support of β is included in that of α and the semigroup converges towards the equilibrium. Simple Absorption and Stimulated Emission Now we complete the example 4.5. In this case, the reader can easily verify that

{H, Lk , L∗k ; k = 1, 2} = {Lk , L∗k ; k = 1, 2} . Therefore, Corollary 6.3. If ξ = 0, the quantum model of simple absorption and stimulated emission introduced in 4.5 has a unique faithful stationary state and the quantum Markov semigroup converges towards the equilibrium, that is w∗

T∗t (ρ) −−→ ρ∞ , for any state ρ where ρ∞ denotes the stationary state.

7 Recurrence and Transience of Quantum Markov Semigroups Within this section we explore the probabilistic notion of recurrence (and transience) for non commutative Markov semigroups. These notions are closely related to the concept of potential as we will see below. 7.1 Potential Let T be a Quantum Markov Semigroup (QMS) on a von Neumann algebra M of operators on a complex Hilbert space h. Inspired by the classical theory of Markov processes [22], this section introduces the non commutative version of potential and discusses its main properties. This is the main tool in the study of recurrence and transience. Throughout this paper, the use of quadratic forms settings will follow the book of Kato (see [41]). Definition 7.1. Given a positive operator x ∈ M we define the form-potential of x as a quadratic form U(x) on the domain

∞ u, Ts (x)uds < ∞ , D(U(x)) = u ∈ h : 0

by

U(x)[u] = 0

∞

u, Ts (x)uds, (u ∈ D(U(x))).


195

This is clearly a symmetric and positive form and by Thm. 3.13a and Lemma 3.14a p.461 of [41] it is also closed. Therefore, when it is densely defined, it is represented by a self-adjoint operator (see Th.2.1, p.322, Th. 2.6, p.323 and Th. 2.23 p.331 of [41]). This motivates the following definition. Definition 7.2. A positive x ∈ M such that D(U(x)) is dense is called T –integrable or simply integrable. We denote M+ int the cone of positive integrable elements of M. For any x ∈ M+ int , we call potential of x the self-adjoint operator U(x) which represents U(x). Note that D(U(x)1/2 ) = D(U(x)) (see Th. 2.23, p.331 in [41]). We recall that a closed operator A is affiliated with a von Neumann algebra M if a D(A) ⊆ D(A) and a A ⊆ Aa for all a ∈ M . Proposition 7.1. For all x ∈ M+ int , the operator U(x) is affiliated with M. t Proof. Fix y ∈ M and define Xt = 0 Ts (x)ds, for all t ≥ 0. Clearly, both Xt 1/2 and Xt belong to M. Given any u ∈ h,

t

1/2

yu, Ts (x)yuds = yXt

1/2

u, yXt

2

u ≤ y u, Xt u.

0

Thus, if u ∈ D(U(x)), then t≥0

t

2

yu, Ts (x)yuds ≤ y

sup 0

∞

2

u, Ts (x)uds = y U(x)[u].

0

It follows that, if u ∈ D(U(x)) = D(U(x)1/2 ), then yu ∈ D(U(x)). Now, if v, u ∈ D(U(x)), then y ∗ v, yu ∈ D(U(x)) and

t

∗

y v, Ts (x)uds = 0

t

Ts (x)v, yuds, 0

so that letting t → ∞ and using complex polarization, we get y ∗ v, U(x)u = U(x)v, yu. That is, v, y U(x)u = U(x)v, yu it follows that yu ∈ D(U(x)) and U(x)yu = y U(x)u, hence y U(x) ⊆ U(x)y. Proposition 7.2. Let T be a Quantum Markov Semigroup and let x ∈ M positive. Then the orthogonal projection p onto the closure of D(U(x)) is subharmonic. In particular, if T is irreducible, then D(U(x)) is either dense or {0}. Proof. We first notice that p ∈ M. Indeed, arguing as in the proof before, we can show that for every u ∈ D(U(x)) and y ∈ M , yu ∈ D(U(x)). Hence, pypu = pyu = yu = ypu.

196


In other words, since D(U(x)) is dense in the range of p, we obtain pyp = yp. On the other hand, y ∗ ∈ M , so that py ∗ p = y ∗ p. Therefore, pyp = py. Hence yp = py, so that p ∈ M = M. We now show that Tt (p) ≥ p for any t ≥ 0. Let ρ be a density matrix ρ such that λk |uk uk |, λk ≥ 0, λk = 1, uk ∈ D(U(x)). ρ= k

k

Note that ρ defines a normal linear functional on M. Therefore ρ ∈ M∗ . Moreover, denote ϕ ∈ M∗ the state given by ϕ(a) = tr(ρa), for all a ∈ M. For any t ≥ 0 there exists (see [23] Th.1, p.57) a density matrix ρt such that T∗t (ϕ)(a) = tr(ρt a) for all a ∈ M. Notice that for all s ≥ 0, tr(ρt Ts (a)) = T∗t (ϕ)(Ts (a)) = tr(ρTt+s (a)). Hence, ∞ ∞ ∞ tr(ρt Ts (a))ds = tr(ρTt+s (a))ds = tr(ρTs (a))ds < ∞. 0

0

t

It follows that ρt =

λk (t)|uk (t)uk (t)|,

k

with uk (t) ∈ D(U(x)), for all k ≥ 1 and t ≥ 0 such that λk (t) > 0. As a result, the range of ρt is included in D(U(x)), i.e. pρt = ρt p = pρt p = ρt . Thus, tr(ρTt (p)) = tr(ρt p) = tr(ρt ) = 1, and 0 = tr(ρ(p − Tt (p))) = tr(ρ(p − pTt (p)p)). However, we also have pTt (p)p ≤ pTt (1)p ≤ p. Therefore, pTt (p)p = p, i.e. pTt (p⊥ )p = 0, (see Lemma II.1 in [32]) so that Tt (p) ≥ p. The second part is a trivial consequence of the above. Potentials are a natural source of superharmonic (or excessive) operators. Indeed, heuristically, ∞ ∞ Tt (U(x)) = Tt ( Ts (x)ds) = Ts (x)ds ≤ U(x), 0

t

however U(x) is possibly unbounded. Further on, bounded potentials will be associated with our concept of transience (see Theorems 7.2 and 7.4). Theorem 7.1. For any x ∈ M+ int , the contraction y = U(x)(1 + U(x))−1 ,

(32)

is superharmonic and Tt (y) converges strongly to 0 as t → ∞. t Proof. Fix x ∈ M+ int and define Ut (x) = 0 Ts (x)ds (t ≥ 0). For any s, t ≥ 0, Tt (Us (x)) =

t+s

Tr (x)dr = Ut+s (x) − Ut (x). t

(33)


197

It follows: Tt (Us (x)) ≤ Ut+s (x).

(34)

Since Tt (·) is in particular 2-positive, identity preserving and the function x → (1 + x)−1 is operator monotone (see e.g. [13]), we have (1 + Tt (Us (x))) From (34), (1 + Ut+s (x))

−1

−1

≤ Tt ((1 + Us (x))−1 ).

≤ Tt ((1 + Us (x))−1 ).

It follows: Tt (Us (x)(1 + Us (x))−1 ) = 1 − Tt ((1 + Us (x))−1 ) ≤ 1 − (1 + Ut+s (x))

−1

= Ut+s (x) (1 + Ut+s (x)) The map Tt (·) is normal and Ut+s (x) (1 + Ut+s (x)) as s → ∞. Therefore, letting s → ∞ yields Tt (y) ≤ y. Finally, (33) implies

−1

−1

.

strongly converges to y

Tt (Us (x)(1 + Us (x))−1 ) ≤ Tt (Us (x)) = Ut+s (x) − Ut (x), so that for all u ∈ D(U(x)), u, Tt (Us (x)(1 + Us (x))−1 )u ≤

t+s

u, Tr (x)udr. t

Letting s → ∞ again, u, Tt (y)u ≤

∞

u, Tr (x)udr,

t

thus, u, Tt (y)u vanishes, as t goes to infinity. Since D(U(x)) is dense and the operators Tt (y) are uniformly bounded in norm by y ≤ 1, the last statement of the theorem follows. Proposition 7.3. For any x ∈ M+ , let K(x) = {u ∈ D(U(x)) : U(x)[u] = 0}. Then the projection p on K(x) is subharmonic. Proof. We use here the notations of the previous proof. Note that for x ∈ M+ , U(x)[u] = 0 if and only if Us (x)u = 0 for each s ≥ 0. Fix s > 0 and let qn (s) denote the spectral projection of Us (x) associated with the interval ]1/n, Us (x)], (n ≥ 1). It is worth noticing that q(s) = l.u.b.qn (s) is the projection onto the closure of the range of Us (x). Equation (34) yields Tt (qn (s)) ≤ nTt (Us (x)) ≤ n Ut+s (x).

198


Since Tt (qn (s)) ≤ 1 we obtain, Tt (qn (s))n ≤ n Ut+s (x), that is Tt (qn (s)) ≤ n1/n Ut+s (x)1/n . Therefore, letting n → ∞, Tt (q(s)) ≤ q(t + s). Now, notice that the family q(s) is increasing with s and q = l.u.b.q(s) is equal to 1 − p, the projection onto the orthogonal of K(x). The conclusion follows from the previous inequality letting s → ∞. 7.2 Defining Recurrence and Transience Let T be a QMS on a von Neumann algebra M. We say that a self-adjoint operator X is strictly positive if u, Xu > 0 for any u ∈ D(X), u = 0 (we will write simply X > 0). Theorem 7.2. The following statements are equivalent: 1. There exists a positive x ∈ M with U(x) bounded and U(x) > 0. 2. There exists a strictly positive x ∈ M with U(x) bounded. 3. There exists a positive x ∈ M with U(x) > 0. 4. There exists an increasing sequence of projections (pn ; n ≥ 1), with l.u.b.pn = 1 and U(pn ) bounded for all n. Proof. 1⇒2: Let xλ = Rλ (x) (λ > 0), where Rλ (·) is the resolvent of the semigroup T . Since U(x) > 0, then xλ > 0. Moreover, the resolvent identity implies U(xλ ) = U(Rλ (x)) = λ−1 (U(x) − Rλ (x)) ≤ λ−1 U(x). Thus, U(xλ ) is bounded. 2⇒1: Clearly if x > 0 then U(x) > 0. 1⇒3 is self-evident. 3⇒1: Let x ∈ M positive with U(x) > 0 and set y as in Theorem 7.1. Clearly 0 < y < 1, and is a superharmonic operator. We may assume y in the domain of the generator L of T (otherwise replace y by Rλ (y); Tt (Rλ (y)) still vanishes as t → ∞), then L(y) ≤ 0 and t Ts (−L(y))ds = y − Tt (y), (t ≥ 0). 0

Letting t → ∞ yields U(−L(y)) = y. Thus −L(y) satisfies condition 1. 4⇒1: Define cn = 2−n U(pn )−1 , and x = n≥0 cn pn . Then x is strictly positive, U(x) is bounded and U(x) > 0. 1⇒4: By the argument of 1⇒2 we can suppose that x > 0. It suffices then to take pn as the spectral projection of x associated with the interval ]1/n, x].


199

Corollary 7.1. If M = B(h) with h separable, then the statements of Theorem 7.2 are all equivalent to the following condition there exists an increasing sequence of finite dimensional projections (pn ; n ≥ 1), with l.u.b.pn = 1 and U(pn ) bounded for all n. Proof. Clearly it suffices to prove that the statements of Theorem 7.2 imply the above condition on finite dimensional projections. Let (pm ; m ≥ 1) be an increasing sequence of projections satisfing the statement 4. For each m let (pm,k ; k ≥ 1) be an increasing sequence of finite dimensional projections on h with l.u.b.k pm,k = pm . Note that 0 ≤ U(pm,k ) ≤ U(pm ) for all m, k. Therefore we have U(pm,k ) ≤ U(pm ) < ∞. Finally, since h is separable, a diagolisation argument shows the existence of a subsequence (pmn ,kn ; n ≥ 1) with l.u.b.n pmn ,kn = 1 and U(pmn ,kn ) < ∞ for all n. Theorem 7.3. The following are equivalent: 1. For each positive x ∈ M and u ∈ h either u ∈ D(U(x)) or u ∈ D(U(x)) and U(x)[u] = 0. 2. For each projection p and u ∈ h either u ∈ D(U(p)) or u ∈ D(U(p)) and U(p)[u] = 0. Proof. Clearly 1⇒2. We prove then that 2⇒1. Let x ∈ M and u ∈ h. If u ∈ D(U(x)) then, for each spectral projection p of x associated with an interval ]r, x], u ∈ D(U(p)). Therefore, by condition 2, we have U(p)[u] = 0 i.e. u, Tt (p)u = 0 for all t ≥ 0. It follows then that u, Tt (x)u = 0 for all t ≥ 0. As a consequence U(x)[u] = 0. Corollary 7.2. If M = B(h) with h, the statements of Theorem 7.3 are all equivalent to the following conditions: for each finite dimensional projection p and u ∈ h either u∈ / D(U(p)) or u ∈ D(U(p)) and U(p)[u] = 0. Proof. Suppose that the above condition on finite dimensional projections holds and let p be any projection in M. Let (pn ; n ≥ 1) be an increasing sequence of finite dimensional such that l.u.b.pn = p. If u ∈ D(U(p)) then u ∈ D(U(pn )) and U(pn )[u] for all n ≥ 1. This implies clearly u, Tt (pn )u = 0 for all n ≥ 1 and all t ≥ 0 and, letting n tend to infinity, u, Tt (p)u = 0 for all t ≥ 0. It follows that U(p)[u] = 0. Definition 7.3. A QMS is transient (resp. recurrent) if any of the equivalent conditions of Theorems 7.2 (resp. Theorem 7.3) holds. Proposition 7.4. If a QMS is irreducible, then it is either recurrent or transient. Proof. Indeed, if a QMS is irreducible, then the domain of the form-potential U(x) is either {0} or dense by Proposition 7.2. Corollary 7.3. A transient semigroup in B(h) with h separable has no invariant state.

200


Proof. Suppose that ρ is an invariant state and take (pn ; n ≥ 1) as in Corollary 7.1. Fix m ≥ 1 such that tr(()ρpm ) > 1/2. Since U(pm ) is bounded, using the separability of h and a diagonalisation argument we can find a sequence (tk ; k ≥ 1) diverging to +∞ such that Ttk (pn ) → 0 strongly as k → ∞. On the other hand, using the invariance of ρ, we have tr(()ρpm ) = tr(T∗tk (ρ)pm ) = tr(ρTtk (pm )), and letting k → ∞ we obtain the contradiction tr(ρpm ) = 0. Theorem 7.4. An irreducible QMS T is transient if and only if there exists a nontrivial T -superharmonic operator in M. Proof. If T is transient then, by Theorem 7.2 1, there exists a positive x ∈ M with U(x) bounded and U(x) > 0. We have then ∞ u, Ts (x)uds u, Tt (U(x))u = t

for all u ∈ h. It follows that U(x) is a superharmonic operator for T and it is not a multiple of the identity operator since Tt (U(x)) converges strongly to 0 as t goes to infinity. Conversely if there exists a non-trivial T -superharmonic operator y in M by adding a multiple of 1 we can assume that y is also positive. Suppose first, in addition, that y is not harmonic i.e. Tt (y) < y for some t > 0. Note that Rλ (y) is also non-trivial and satisfies Tt (Rλ (y)) ≤ Rλ (y), for all t ≥ 0 and Tt (Rλ (y)) < Rλ (y) for some t > 0. Therefore, replacing y by Rλ (y) if necessary, we can assume also that y belongs to the domain of the generator L. We have then L(y) < 0 and t u, Ts (−L(y))uds = u, (y − Tt (y))u ≤ u, yu. 0

It follows then, letting t go to infinity, that U(−L(y)) ≤ y and T is transient by Theorem 7.2 2. It remains to show that we can suppose that y is not harmonic. Indeed, if y is harmonic, then from the Schwarz inequality Tt (y ∗ )Tt (y) ≤ Tt (y ∗ y), we have y 2 = Tt (y ∗ )Tt (y) ≤ Tt (y 2 ). Now, if y 2 is not harmonic, we can apply the above argument to (1 + y 2 )1 − y 2 . n If y 2 is also harmonic we can try with y 4 , y 8 , ... until we find an n such that y 2 is subharmonic but not harmonic. In case we do not find such an n then, arguing as in n n the proof of Theorem 7.1, we can show that the operators y 2 (s + y 2 )−1 (n ≥ 1, s > 0) are T -superharmonic. Then, if y is non-trivial, Lemma 7.1 shows that T is not irreducible. This completes the proof. Lemma 7.1. Let T be a QMS on a von Neumann algebra M and let y be a strictly positive T -harmonic operator in M. Suppose that, for every n ≥ 1 and every s > 0 n n the operators y 2 (s + y 2 )−1 are T -superharmonic. Then every spectral projection of y associated with an interval ]r, +∞[ is T -superharmonic.


201

Proof. Note that, for each r > 0, the operator lim (r−1 y)2 (s + (r−1 y)2 )−1 = n

n

n

1 E{r} + E]r, +∞[ s+1

where E{r} denotes the orthogonal projection on the (possibly empty) eigenspace of y corresponding to r and E]r, +∞[ the spectral projection of y associated with the interval ]r, +∞[ and the limit exists in the strong operator topology. It follows that Tt (s + 1)−1 E{r} + E]r, +∞[ ≤ (s + 1)−1 E{r} + E]r, +∞[. The conclusion follows letting s tend to infinity. 7.3 The Behavior of a d-Harmonic Oscillator Let h = L2 (Rd ; C) and let M = L(h). Our framework here is the same as that of the harmonic oscillator in [44], Ch. III. By a d-harmonic oscillator, also called Quantum Brownian Motion, we mean a quantum Markov process with associated (minimal) semigroup T on M associated with the form generator 1 ∗ 1 ∗ aj aj x − 2aj xa∗j + xaj a∗j − a aj x − 2a∗j xaj + xa∗j aj , −(x) L =− 2 j=1 2 j=1 j d

d

where a∗j , aj are the creation and annihilation operators √ √ aj = (qj + ∂j ) / 2, a∗j = (qj − ∂j ) / 2, ∂j being the partial derivative with respect to the j th coordinate qj . The commutative von Neumann subalgebra Mq of M, generated by q, whose elements are multiplication operators Mf by a function f ∈ L∞ (Rd ; C) is T invariant and Tt (Mf ) = MTt f where 2 1 (Tt f )(x) = f (y)e−|x−y| /2t dy. (35) d/2 (2πt) Rd The same conclusion holds for the commutative algebra Mp = F ∗ Mq F , where F denotes the Fourier transform. Therefore, our process deserves the name of quantum Brownian motion since its contains a couple of non commuting classical Brownian motions. Moreover, the von Neumann algebra MN generated by the number operator N = j a∗j aj is also T invariant and the classical semigroup obtained by restriction of T to MN is a birth and death on N with birth rates (n + 1)n≥0 and death rates (n)n≥0 . Also, an application of subsection 5.2 shows that T is irreducible. The unit vector e0 (q) = π −d/4 exp(−|q|2 /2) satisfies aj e0 = 0 for all j. The rank-one projection |e0 e0 | onto e0 belongs to MN and satisfies

202


Tt (|e0 e0 |) =

1 −N (1 + 1/t) (1 + t)d

(36)

This formula can be checked as follows. Notice first that each Weyl operator W (z) (see [44], III.4) belongs to the domain of L and L(W (z)) = −|z|2 W (z) (e.g. by [29], Lemma 1.1) Therefore, we have Tt (x)(W (z)) = exp(−t|z|2 )W (z) and the canonical commutation relation √ √ √ W (−ζ/ 2)W (z)W (ζ/ 2) = exp(−i 2Imz, ζ)W (z) leads to the explicit formula (see [5]) for x = W (z) ∈ L(h) √ √ 1 Tt (x) = W (−ζ/ 2)xW (ζ/ 2) exp(−|ζ|2 /2t) dζ (2πt)d R2d

(37)

where ζ = r + is with r, s ∈ Rd and dζ means drds. By normality this formula also holds for an arbitrary x ∈ L(h). We now check (36). Indeed, for each unit vector eα (α ∈ Nd ) of the canonical orthonormal basis of h given by d dimensional Hermite polynomials multiplied by the function e0 , we have 2 √ 1 , W (ζ/ 2)e eα , Tt (|e0 e0 |)eα = exp(−|ζ|2 /2t) dζ e α 0 (2πt)d R2d |ζ1 |2α1 · · · |ζd |2αd 1 = exp(−(1 + 1/t)|ζ|2 /2) dζ d (2πt) R2d 2|α| α1 ! · · · αd ! where |α| = α1 + · · · + αd . By the change of variables ζ = ξ/(1 + 1/t)1/2 we find eα , Tt (|e0 e0 |)eα = cα

(1 + 1/t)−|α| (1 + t)d

where cα is a strictly positive constant that can be evaluated by computing a Gaussian integral and shown to be equal to 1. By means of (36), for each d ≥ 2, we compute ∞ ∞ (1 + 1/t)−|α| eα , Tt (|e0 e0 |)eα dt = dt < +∞. (1 + t)d 0 0 Moreover, since the restriction of T to M is also irreducible, for each β, we have Ttβ (|e0 e0 |) ≥ κ(β, tβ )|eβ eβ | for some tβ > 0 and some constant κ(β, tβ ) > 0. It follows that, for each d ≥ 2, our QMS is transient. On the other hand, when d = 1, suppose that T is again transient and let (pn )n≥1 be an increasing sequence of projections with l.u.b.pn = 1 and U(pn ) bounded. We have then ∞ ∞ dt 2 e0 , Tt (pn )e0 dt = |e0 , pn e0 | 1+t 0 0 which diverges whenever |e0 , pn e0 |2 is nonzero. This contradicts the fact that e0 belongs to the domain of U(pn ) for all n ≥ 0. Therefore, T being irreducible, it must be recurrent.


203

Corollary 7.4. The d-harmonic oscillator is recurrent for d = 1 and transient for d ≥ 2.

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Continual Measurements in Quantum Mechanics and Quantum Stochastic Calculus Alberto Barchielli Dipartimento di Matematica, Politecnico di Milano, Piazza Leonardo da Vinci 32, 20133 Milano, Italy e-mail: [email protected] URL: http://www.mate.polimi.it/qp/

1

Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 208 1.1 1.2 1.3

2

Unitary Evolution and States . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 210 2.1 2.2 2.3 2.4 2.5

3

Indirect Measurements on SH . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 230 Characteristic Functionals . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 233 The Reduced Description . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 241 Direct Detection . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 247 Optical Heterodyne Detection . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 252 Physical Models . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 257

A Three–Level Atom and the Shelving Effect . . . . . . . . . . . . . . . . . . . . . 258 4.1 4.2 4.3 4.4

5

Quantum Stochastic Calculus . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 210 The Unitary System–Field Evolution . . . . . . . . . . . . . . . . . . . . . . . . . 217 The System–Field State . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 223 The Reduced Dynamics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 225 Physical Basis of the Use of QSC . . . . . . . . . . . . . . . . . . . . . . . . . . . . 228

Continual Measurements . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 230 3.1 3.2 3.3 3.4 3.5 3.6

4

Three Approaches to Continual Measurements . . . . . . . . . . . . . . . . . 208 Quantum Stochastic Calculus and Quantum Optics . . . . . . . . . . . . . . 208 Some Notations: Operator Spaces . . . . . . . . . . . . . . . . . . . . . . . . . . . . 209

The Atom–Field Dynamics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 259 The Detection Process . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 262 Bright and Dark Periods: The V-Configuration . . . . . . . . . . . . . . . . . 264 Bright and Dark Periods: The Λ-Configuration . . . . . . . . . . . . . . . . . 267

A Two–Level Atom and the Spectrum of the Fluorescence Light . . . . 269 5.1 5.2 5.3

The Dynamical Model . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 270 The Master Equation and the Equilibrium State . . . . . . . . . . . . . . . . . 274 The Detection Scheme . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 277

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5.4

The Fluorescence Spectrum . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 282

References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 288

1 Introduction 1.1 Three Approaches to Continual Measurements We speak of continual measurements in the case in which one ore more observables of a quantum system are followed with continuity in time. Traditional presentations of quantum mechanics consider only instantaneous measurements, but continual measurements on quantum systems are a common experimental practice; typical cases are the various forms of photon detection. The statements of a quantum theory about an observable are of probabilistic nature; so, it is natural that a quantum theory of continual measurements give rise to stochastic processes. Moreover, a continually observed system is certainly open. All these things shows that the development and the applications of a quantum theory of continual measurements need quantum measurement theory, open system theory, quantum optics, operator theory, quantum probability, quantum and classical stochastic processes. . . The first consistent paper treating continual measurements was published in 1969 and concerns counting of quanta [43], but some ideas on quantum counting formulae for photons had already been introduced before [66]. There are essentially three approaches to continual measurements [18, 21, 64]. These approaches have received various degrees of development, any one of them has its own merits and range of applicability, but “morally” all the three approaches are equivalent and one can go from one to the other and this feature is certainly at the bases of the flexibility and interest of the theory. The first approach is the operational one, which is based on positive operator valued measures or (generalized) observables and operation valued measures or instruments [22, 23, 44]. A variant of this approach is based on the Feynman integral [15, 22, 72, 78]. The second approach is based on quantum stochastic calculus and quantum stochastic differential equations [14, 24] and it is connected to quantum Langevin equations and the notion of input and output fields in quantum optics [54, 55]. The last approach is based on (classical) stochastic differential equations and the notion of a posteriori states [21, 29] and it is related to some notions appeared in quantum optics: quantum trajectories, Monte–Carlo wave function method, unravelling of master equation [33, 82]. This report is concerned mainly with the second approach, the one based on quantum stochastic calculus. 1.2 Quantum Stochastic Calculus and Quantum Optics QSC Quantum stochastic calculus (QSC) [65, 84] was developed originally as a mathematical theory of quantum noise in open systems and its first applications in mathematical physics were the construction of unitary dilations of quantum dynamical

Quantum Continual Measurements

209

semigroups [65, 84] and of quantum stochastic processes [51]. Soon after it was applied also to measurement theory in quantum mechanics [14, 24]. The “integrators” of QSC are Bose fields (annihilation and creation processes), which play the role of quantum analogues of independent Wiener processes, and some expressions quadratic in the field operators (conservation processes). The starting point for the applications of QSC in quantum optics is to take these Bose fields as an approximation of the electromagnetic field. The explicit introduction of QSC in quantum optics was made in Ref. 54, but the use of the related δ-correlated noise is older [70]. There are various kinds of applications of QSC to quantum optics. The Bose fields are merely considered as a source of noise and quantum stochastic differential equations (QSDE’s) are used for guessing the correct master equation for the system of interest [53, 67, 76, 77]; the fields are used for modelling quantum input and output channels [13, 14, 17, 18, 40, 54, 69]; QSDE’s are used for describing various arrangements for detecting photons [14, 16, 18, 31, 32, 80]. All these kinds of applications are related; there is not a sharp distinction [18, 55]. A central point in QSC is the ‘quantum stochastic Schrödinger equation’ or Hudson–Parthasarathy equation (39), giving the unitary dynamics of a quantum system interacting with the Bose fields.

QSDE

1.3 Some Notations: Operator Spaces Let A and B be two Banach spaces; then, we denote by B(A; B) the vector space of linear bounded operators from A into B and we set B(A) := B(A; A). Let K be a complex separable Hilbert space; we denote by U(K) the set of unitary operators on it. Let us recall that in a general quantum theory the states are positive, normalized, linear functionals over a C ∗ - or W ∗ -algebra; we shall consider only the so called normal states, which are represented √ by trace–class operators. So, we introduce the trace class T (K) := t ∈ B(K) : Tr t∗ t < ∞ and the set of statistical operators, or states, S(K) := s ∈ T (K) : s ≥ 0, Tr[s] = 1 ; we denote √ by t1 := Tr t∗ t the norm in T (K). Let H and K be two complex separable Hilbert spaces; the partial trace over K is defined by: for t ∈ T (H ⊗ K), TrK {t} ∈ T (H) is the operator satisfying TrH (X TrK {t}) = TrH⊗K {(X ⊗ 1l)t} ,

∀X ∈ B(H) .

B(·; ·) B(·) U(·)

T (·) S(·) · 1 partial trace

(1)

Let us end by recalling the definition of core for a selfadjoint operator; see, for instance, [84] p. 64. A closable and densely defined operator T in a Hilbert space H is called symmetric if T ⊂ T ∗ . The operator T is called selfadjoint if T = T ∗ . The operator T is called essentially selfadjoint if its closure is selfadjoint. Let D0 ⊂ D(T ) be a linear manifold and let T0 be the restriction of T to D0 . If T is selfadjoint and the closure of T0 is T , then D0 is called a core for T .

core

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Alberto Barchielli

2 Unitary Evolution and States 2.1 Quantum Stochastic Calculus We are assuming that the reader is familiar with the main features of QSC, in the version based on the symmetric Fock space, and the Hudson–Parthasarathy equation [65, 84]. In the following we recall a few notions and results of QSC. The Fock Space Γ Z

We denote by Γ the symmetric (or boson) Fock space over the “one–particle space” L2 (R+ ) ⊗ Z, where Z is a separable complex Hilbert space ([84] p. 124); we shall see in the physical examples how to choose Z. The space L2 (R+ ) ⊗ Z is naturally identified with L2 (R+ ; Z), so that a vector f in it is a square integrable function from R+ into Z. So, we have Γ := Γsymm L2 (R+ ) ⊗ Z , L2 (R+ ) ⊗ Z L2 (R+ ; Z). (2)

e(f )

Let us denote by e(f ), f ∈ L2 (R+ ; Z), the exponential vectors, whose components in the 0, 1, . . . , n, . . . particle spaces are e(f ) := 1, f, (2!)−1/2 f ⊗ f, . . . , (n!)−1/2 f ⊗n , . . . ; (3) the internal product between two exponential vectors is given by e(g)|e(f ) = expg|f .

ψ(f )

E(·) E Γ(s,t) Γ(t

Once normalized, the exponential vectors are called coherent vectors: 1 ψ(f ) := exp − f 2 e(f ). 2

(4)

(5)

In particular the vector e(0) ≡ ψ(0) is the Fock vacuum. If M is a dense linear manifold in L2 (R+ ; Z), then the linear span E(M) of the ), f ∈ M, is vectors e(f dense in Γ ; we call exponential domain the set E := E L2 (R+ ; Z) , i.e. the linear span of all the exponential vectors. An important feature of the Fock space Γ is its structure of continuous tensor product. For any choice of the times 0 ≤ s < t let us introduce the spaces Γ(s,t) := Γsymm L2 (s, t) ⊗ Z , Γ(t := Γsymm L2 (t, +∞) ⊗ Z , (6) and for any of such spaces its exponential vectors. Then we have the natural identification ([84] p. 179) Γ Γ(0,s) ⊗ Γ(s,t) ⊗ Γ(t (7) (here 0 < s < t) based on the factorization of the exponential vectors


e(f ) e f(0,s) ⊗ e f(s,t) ⊗ e f(t ,

211

(8)

where f(s,t) (τ ) := 1(s,t) (τ ) f (τ ),

f(t (τ ) := 1(t,+∞) (τ ) f (τ ).

(9)

Similarly, if P is any orthogonal projection, one has the factorization Γ = Γsymm P L2 (R+ ; Z) ⊗ Γsymm (1l − P )L2 (R+ ; Z) .

(10)

f(s,t) , f(t

The Weyl Operators and the Bose Fields The Weyl operator W(g; U ), g ∈ L2 (R+ ; Z), U ∈ U L2 (R+ ; Z) , is the unique unitary operator ([84] Section 20) defined by 3 2 2 (11) W(g; U ) e(f ) = exp − 12 g − g|U f e(U f + g)

W(g; U )

or by W(g; U ) ψ(f ) = exp {i ImU f |g} ψ(U f + g) .

(12)

From the definition one obtains easily the inverse W(g; U )−1 = W(g; U )∗ = W(−U ∗ g; U ∗ )

(13)

and the composition law W(h; V ) W(g; U ) = exp {−i Imh|V g} W(h + V g; V U ) ;

(14)

moreover, by particularizing this equation to V = U = 1l, one gets the Weyl form of the canonical commutation relations (CCR): W(h; 1l) W(g; 1l) = W(g; 1l) W(h; 1l) exp {−2i Imh|g} .

CCR

(15)

The Weyl operators allow to introduce some important selfadjoint operators in Γ ([84] Section 20), which play the double role of being the starting point to construct the integrators of QSC and of representing the main observables used in the the theory of continual measurements. Let us collect in a unique theorem Propositions 20.4, 20.7, 20.11, 2.16 and Corollaries 20.5 and 20.6 of Ref. 84. Theorem 2.1. Let us take h ∈ L2 (R+ ; Z); then, the map κ → W(iκh; 1l) is a strongly continuous one parameter group and we denote by Q(h) its Stone generator: W(iκh; 1l) = exp{iκQ(h)}. (16) Moreover, one has (i) Q(h) is essentially selfadjoint in the domain E(M), where M is any dense subset of L2 (R+ ; Z); (ii) E is a core for Q(h); (iii) the linear manifold of all finite particle vectors is a core for Q(h);

Q(h)

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Alberto Barchielli

(iv) E is included in the domain of the product Q(h1 )Q(h2 ) · · · Q(hn ), ∀n, ∀h1 , . . . , hn ∈ L2 (R+ ; Z); (v) [Q(h), Q(g)] e(f ) = {2i Imh|g} e(f ), ∀h, g, f ∈ L2 (R+ ; Z). Let B be a selfadjoint operator in L2 (R+ ; Z) with domain D(B); then, the map κ → W(0; exp{iκB}) is a strongly continuous one parameter group and we denote λ(B) by λ(B) its Stone generator: W(0; exp{iκB}) = exp{iκλ(B)}.

(17)

Moreover, one has (a) E(D(B)) is included in the domain of λ(B); (b) E(D(B 2 )) is a core for λ(B); (c) if B is bounded, λ(B) is essentially selfadjoint in the domain E; (d) i[λ(B1 ), λ(B2 )] e(f ) = λ (i[B1 , B2 ]) e(f ), for any two bounded selfadjoint operators B1 , B2 and ∀f ∈ L2 (R+ ; Z); Ti = Q(hi ), (e) E is included in the domain of the product T1 T 2 · · · Tn , where hi ∈ L2 (R+ ; Z), or Ti = λ(Bi ), Bi = Bi∗ ∈ B L2 (R+ ; Z) . For any h ∈ L2 (R+ ; Z) and any selfadjoint operator B in L2 (R+ ; Z) let us set λ(B, h) := W(−h; 1l) λ(B) W(h; 1l) .

(18)

Then, the operator λ(B, h) is the generator of the unitary group κ → W(−h; 1l)W(0; exp{iκB})W(h; 1l) (19) ≡ exp i Im eiκB hh W eiκB − 1l h; eiκB and it is essentially selfadjoint on the linear manifold generated by e(f − h) : f ∈ D(B 2 ) . When B is also bounded, E is a core for λ(B, h) and, on the exponential domain E, one has λ(B, h) = λ(B) + a(Bh) + a† (Bh) + h|Bh1l .

(20)

The operators a(·) and a† (·) are defined here below in eq. (21). a(h), a† (h)

By defining a(h) =

1 Q(h) + iQ(ih) , 2

a† (h) =

1 Q(h) − iQ(ih) , 2

(21)

one obtains two mutually adjoint operators, satisfying ([84] Proposition 20.12) the eigenvalue relation a(h) e(f ) = h|f e(f ) (22) and, at least in the domain E, the CCR [a(h), a(g)] = [a† (h), a† (g)] = 0 ,

[a(h), a† (g)] = h|g .

(23)


213

So, we recognize the annihilation and creation operators and we call them, collectively, the (smeared) Bose fields; in quantum optics the two selfadjoint operators Q(h) and Q(ih) sometimes referred to as two conjugated field quadratures. are 2 (R ; Z) is bounded If B ∈ B L + but not selfadjoint, one defines λ(B) := λ 12 (B + B ∗ ) + iλ 2i1 (B − B ∗ ) . All matrix elements on exponential vectors and commutation relations involving Q(h), a(h), a† (h), λ(B) are deduced from the properties of the Weyl operators and of the exponential vectors and are given in Ref. 84 Section 20. Moreover, also the linear manifold of all finite particle vectors is contained in the domains of Q(h), a(h), a† (h), λ(B) ([84] Proposition 20.14). The annihilation, creation and conservation processes Let us fix a complete orthonormal system (c.o.n.s.) {zk , k ≥ 1} in Z and for any f ∈ L2 (R+ ; Z) let us set fk (t) := zk |f (t). We denote by Ak (t), A†k (t), Λkl (t) the annihilation, creation and conservation processes associated with such a c.o.n.s. ([65] Sect. 2): A†k (t) := a† zk ⊗ 1(0,t) , (24a) Ak (t) := a zk ⊗ 1(0,t) , Λkl (t) := λ (|zk zl |) ⊗ 1(0,t) ; (24b)

c.o.n.s. {zk }, fk (t) Ak (t), A†k (t)

for these processes one has

Λkl (t)

t

Ak (t) e(f ) =

fk (s) ds e(f ) ,

(25a)

gk (s) ds e(g)|e(f ),

(25b)

gk (s) fl (s) ds e(g)|e(f ).

(25c)

0

e(g)|A†k (t)e(f ) =

t

0

t

e(g)|Λkl (t)e(f ) = 0

Let us recall that by construction these operators are defined at least on E and on this domain A†k (t) is the adjoint of Ak (t); moreover, Ak (t) + A†k (t), i A†k (t) − Ak (t) , Λkk (t) are essentially selfadjoint on E. Another form of the CCR follows from (24a) and (23): on the exponential domain, and on the finite particle vectors, one has [Ak (t), Al (s)] = [A†k (t), A†l (s)] = 0,

[Ak (t), A†l (s)] = δkl min{t, s}. (26)

In theoretical physics it is usual to write formally Ak (t) =

t

ak (s) ds , 0

A†k (t) =

0

t

a†k (s) ds ,

Λkl (t) = 0

t

a†k (s)al (s) ds ,

where the “Bose fields” ak (t), a†k (t) satisfies the (heuristic) CCR [ak (t), a†l (s)] = δkl δ(t − s),

[ak (t), al (s)] = [a†k (t), a†l (s)] = 0 .

(27)

(28)

214

Alberto Barchielli

Quantum Stochastic Integrals The System Space

H SH

We are interested in a quantum system interacting with the Bose fields we have introduced; this quantum system is described in a complex separable Hilbert space H, called the system space or the initial space ([84] p. 179); let us call this quantum system “system SH ” or simply “the system”. Operators acting in H are extended to H ⊗ Γ by the convention that they act as the identity on Γ ; the tensor product with the identity is not always indicated. A similar extension is understood for operators acting in Γ . So, K ∈ B(H) or K ⊗ 1l, Ak (t) or 1l ⊗ Ak (t) are the same. Adapted processes An adapted process is a time dependent family of operators {L(t), t ≥ 0}, such that L(t) acts trivially as the identity on Γ(t and possibly non trivially in H ⊗ Γ(0,t) ; an adapted process is something containing the fields onlyup to time t. In the case of a bounded adapted process, this simply means L(t) ∈ B H ⊗ Γ(0,t) ; in the general case the definition is the following.

Definition 2.1 ([84] p. 180). Let D and M be dense linear manifolds in H and L2 (R+ ; Z), respectively, such that 1(s,t) f ∈ M whenever f ∈ M for all 0 ≤ s < ⊗ t < ∞. Denote by D ⊗ E(M) the linear manifold generated by all the vectors of the form u ⊗ e(f ), u ∈ D, f ∈ M. A family {L(t), t ≥ 0} of operators in H ⊗ Γ adapted is an adapted process with respect to (D, M) if process (i) for any t, the domain of L(t) contains D ⊗ E(M); (ii) L(t)u⊗e(f(0,t) ) ∈ H⊗Γ(0,t) and L(t)u⊗e(f ) = L(t)u ⊗ e(f(0,t) ) ⊗e(f(t ) for all t ≥ 0, u ∈ D, f ∈ M. regular

M dim f

It is said to be regular if, in addition, the map t → L(t)u⊗e(f ) from R+ into H ⊗Γ is continuous for every u ∈ D, f ∈ M. It is convenient to fix M once for all; we follow the choice of Ref. 71: M := f ∈ L2 (R+ ; Z) ∩ L∞ (R+ ; Z) : fk (t) ≡ 0 for all but a finite number of indices k . (29) For f ∈ M let us set dim f := max k fk is a non-zero vector in L2 (R+ ) . Let us note that the definitions of M and dim f depend on the initial choice of the c.o.n.s. {zk } in Z and that, being M dense in L2 (R+ ; Z), then E(M) is total in Γ . Quantum stochastic integrals and Ito table In QSC integrals of “Ito type” with respect to dAk (t), dA†k (t), dΛkl (t) are defined ([84] pp. 188–190, 224–225); the integrands are adapted processes with some conditions to assure the existence of the quantum stochastic integrals. We shall use the class of integrands given in the definition below. It is the one used in Ref. 71 and it allows to give meaning to all the integrals we need; it is a bit larger of the one introduced by Parthasarathy [84], but all the results of Ref. 84 continue to hold.


215

Definition 2.2 ([65] Proposition 3.2; [84] pp. 189, 221–222, 224; [71]). A family {Lkl , k, l ≥ 0} of (H, M) adapted processes is said to be stochastically integrable if, for all t ≥ 0, l ≥ 0, u ∈ H, f ∈ M, t ∞

Lkl (s)u ⊗ e(f )2 1 + f (s)2 ds < +∞ .

stochastically integrable

0 k=0

We denote by L(M) the class of stochastically integrable families of (H, M) adapted processes. Note that M and, so, the class of stochastically integrable processes L(M) depend on the initial choice of the c.o.n.s. {zk } in Z. The definition of quantum stochastic integral goes trough a suitable limit on the integral of sequences of “simple processes” ([84] Section 27); then, the following result holds. Proposition 2.1 ([84] Proposition 27.1). Let {Lkl , k, l ≥ 0} ∈ L(M), X(0) ∈ B(H); then t

∞ Lk0 (s)dA†k (s) L00 (s)ds + X(t) := X(0) + 0

k=1

+

∞

L0l (s)dAl (s) +

l=1

∞

Lkl (s)dΛkl (s)

(30)

k,l=1

is a regular (H, M) adapted process and, ∀u ∈ H, ∀f ∈ M, ∀t ≥ 0,

2

[X(t) − X(0)] u ⊗ e(f ) ≤ 2 exp ×

dim f

t ∞

l=0

t

1 + f (s) ds 2

0

Lkl (s)u ⊗ e(f )2 1 + f (s)2 ds .

(31)

0 k=0

The main practical rules to manipulate the quantum stochastic integrals and their products are the facts that 1. dAk (t), dA†k (t), dΛkl (t) commute with adapted processes at time t, so that they can be shifted towards the right or the left, according to the convenience; 2. the products of the fundamental differentials satisfy the Ito table dAk (t) dA†l (t) = δkl dt , dΛkr (t) dA†l (t)

=

δrl dA†k (t) ,

dAk (t) dΛrl (t) = δkr dAl (t) , dΛkr (t) dΛsl (t) = δrs dΛkl (t) ;

all the other products and the products involving dt vanish; 3. dAk (t) e(f ) = dt fk (t) e(f ), e(f )| dA†k (t) = fk (t) dt e(f )|, † dΛkl (t) e(f ) = dAk (t) fl (t) e(f ).

(32)

L(M)

216

Alberto Barchielli

By means of these rules the matrix elements on exponential vectors of quantum stochastic integrals can be computed and products of quantum stochastic integrals can be differentiated (quantum Ito’s formula); see [84] pp. 221–224. To be more precise, the following results hold. Proposition 2.2 ([84] Corollary 27.2). Let {Lkl , k, l ≥ 0} , {Mlk , k, l ≥ 0} ∈ L(M), X(0) , Y (0) ∈ B(H); let X(t) be defined by eq. (30) and Y (t) be defined in a similar way in terms of the processes Mlk . Then, for all u, v ∈ H, f, g ∈ M the matrix elements v ⊗ e(g)|X(t)u ⊗ e(f ), v ⊗ e(g)|Y (t)u ⊗ e(f ), Y (t)v ⊗ e(g)|X(t)u⊗e(f ) are just the ones that one can compute by means of the practical rules given above, i.e.

v ⊗ e(g) [X(t) − X(0)] u ⊗ e(f ) =

t

0

× Lk0 (s) +

∞ l=1

k=1

0 k gk (s)Ll (s)fl (s) u ⊗ e(f ) , (33)

∞

L0l (s)fl (s) +

∞

/ ds v ⊗ e(g) L00 (s) + gk (s)

k,l=1

Y (t) v ⊗ e(g)|X(t) u ⊗ e(f ) − Y (0) v ⊗ e(g)|X(0) u ⊗ e(f ) t

= ds Y (s) v ⊗ e(g)|L00 (s) u ⊗ e(f ) 0

+ M00 (s) v ⊗ e(g)|X(s) u ⊗ e(f ) + +

∞

∞

M0k (s) v ⊗ e(g)|Lk0 (s) u ⊗ e(f )

k=1

gk (s) Y (s) v ⊗ e(g)|Lk0 (s) u ⊗ e(f )

k=1

+ Mk0 (s) v ⊗ e(g)|X(s) u ⊗ e(f ) +

∞

Mkl (s) v ⊗ e(g)|Ll0 (s) u ⊗ e(f )

l=1

∞ + Y (s) v ⊗ e(g)|L0l (s) u ⊗ e(f ) + M0l (s) v ⊗ e(g)|X(s) u ⊗ e(f ) l=1

+ +

∞

∞

M0k (s) v k=1

⊗

e(g)|Lkl (s) u

⊗ e(f ) fl (s)

gk (s) Y (s) v ⊗ e(g)|Lkl (s) u ⊗ e(f ) + Mkl (s) v ⊗ e(g)|X(s) u ⊗ e(f )

k,l=1

+

∞

Mkr (s) v

⊗

e(g)|Lrl (s) u

⊗ e(f ) fl (s) . (34)

r=1

Moreover, the quantum stochastic integral (30) is uniquely determined by the matrix elements (33).


217

To handle a product Y (t)X(t) is a more delicate problem; in general we do not even know if H ⊗ E(M) is included in the domain of this product. Definition 2.3. Let {Lkl , k, l ≥ 0}, {L†k l , k, l ≥ 0} ∈ L(M) be such that v ⊗ e(g)|Llk (t)u ⊗ e(f ) = L†k (t)v ⊗ e(g)|u ⊗ e(f ), ∀k, l, t, ∀u, v ∈ H, ∀f, g ∈ M; l then, {Lkl , k, l ≥ 0}, {L†k , k, l ≥ 0} is called an adjoint pair in L(M). l Proposition 2.3 ([84] Proposition 25.12, [71] p. 518). Let {Lkl , k, l ≥ 0}, † ∗ {L†k l , k, l ≥ 0} be an adjoint pair in L(M), X(0) ∈ B(H), X (0) = X(0) ; let † X(t) be defined by eq. (30) and X (t) be defined in a similar way in terms of L†k l , X † (0). Then, X(t)∗ = X † (t), ∀t ≥ 0, on H ⊗ E(M). Proposition 2.4 ([84] Proposition 25.26). Let {Lkl , k, l ≥ 0} , {Mlk , k, l †k k ≥ 0} , {M †k l , k, l ≥ 0} ∈ L(M), with {Ml , k, l ≥ 0} , {M l , k, l ≥ 0} an adjoint pair, X(0) , Y (0) ∈ B(H); let X(t) be defined by eq. (30) and Y (t) be defined in a similar way in terms of Mlk , Y (0). Let us define, ∀k, l ≥ 0, ∀t ≥ 0, Flk (t) := Mlk (t)X(t) + Y (t)Lkl (t) +

∞

Mjk (t)Ljl (t) .

(35)

j=1

Suppose that i) Y (t)X(t), t ≥ 0, in an (H, M ) adapted process, ii) {Flk , k, l ≥ 0} ∈ L(M). Then, on H ⊗ E(M), one has t

∞ 0 F0k (s)dA†k (s) Y (t)X(t) = Y (0)X(0) + F0 (s)ds + 0

+

k=1 ∞

Fl0 (s)dAl (s)

l=1

+

∞

Flk (s)dΛkl (s)

. (36)

k,l=1

Parthasarathy gives the proof of this proposition only in the case of finitely many integrators, but nothing changes in the case of infinitely many integrators and of integrands in L(M); the existence of the adjoint pair is needed in the proof, but it does not appear in the final statement. The meaning of Proposition 2.4 is that, under the hypotheses given, Y (t)X(t) can be differentiated according the practical rules of QSC. 2.2 The Unitary System–Field Evolution The Hudson–Parthasarathy Equation The ingredients of the Hudson–Parthasarathy equation are system operators and fields. We consider the simplest version of this equation: only bounded system operators are involved. This is not enough for all physical applications, but includes significant cases and allows to develop a general theory which gives an idea of what could be done even in other cases.

adjoint pair

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Alberto Barchielli

The system operators H Rk Skl

and Skl , k, l ≥ 1, be bounded operators in H such that H ∗ = H Let H, Rk∗, k ≥ 1 ∗ and j Sjk Sjl = j Skj Slj = δkl ; if Z is infinite dimensional, the set of indices is convergent infinite and the previous series and k Rk∗ Rk are assumed to be strongly to bounded operators. From these conditions, we have that also the series k Rk∗ Skl is strongly convergent to a bounded operator. It is useful to construct from H, Rk , Skl three operators S ∈ U(H ⊗ Z),

R ∈ B(H; H ⊗ Z),

R, S, K by Ru =

(Rk u) ⊗ zk ,

K ∈ B(H)

(37a)

∀u ∈ H ,

(37b)

∀ u, v ∈ H ,

(37c)

k

or, equivalently, v ⊗ zk |Ru = v|Rk u , S :=

Skl ⊗ |zk zl | ,

(37d)

kl

K := −iH −

1 ∗ 1 Rk Rk ≡ −iH − R∗ R . 2 2

(37e)

k

C(f )

Another useful operator, for f ∈ Z, is C(f ) : H → H ⊗ Z ,

C(f )u = u ⊗ f ,

∀u ∈ H .

By the positions (37) we have also the useful relations ∗ gk (s)Rk = C g(s) R ,

(37f)

(38a)

k

∗ gk (s) (Skl − δkl ) fl (s) = C g(s) (S − 1l)C f (s) ,

kl

Rk∗ Skl fl (s) = R∗ SC f (s) .

(38b) (38c)

kl

The evolution equation U (t)

Theorem 2.2 ([84] Proposition 27.5 p. 225, Theorem 27.8 p. 228). In the hypotheses above, there exists a unique (H, M) adapted process U (t) satisfying the initial condition U (0) = 1l and the QSDE dU (t) =

k

Rk dA†k (t) +

(Skl − δkl ) dΛkl (t)

kl

−

kl

Rk∗ Skl dAl (t) + K dt U (t).

(39)


219

Moreover, U (t) is uniquely extended to a unitary process, which turns out to be strongly continuous in t. The adjoint process U (t)∗ is strongly continuous and it is the unique unitary adapted process satisfying U (0)∗ = 1l and the adjoint equation dU (t)∗ = U (t)∗

Rk∗ dAk (t) +

k

∗ (Skl − δkl ) dΛlk (t)

kl

−

∗ Skl Rk dA†l (t) + K ∗ dt . (40)

kl

By the practical rules of QSC (Proposition 2.2) we get from (39): ∀u, v ∈ H, ∀f, g ∈ M

t

v ⊗ e(g)|U (t) u ⊗ e(f ) − v|u exp{g|f } = +

gk (s) (Skl − δkl ) fl (s) −

kl

2 / ds v ⊗ e(g) gk (s)Rk

0

Rk∗ Skl fl (s)

k

3 0 + K U (s) u ⊗ e(f ) ; (41)

kl

it is also true that this equation uniquely determines U . Corollary 2.1 ([56] Corollary 3.2 p. 26). The solution U of (39) is the unique unitary adapted process satisfying (41) for every t ≥ 0, u, v ∈ H, f, g ∈ M. Proof. Let U be a unitary adapted process satisfying (41) and let us define ! (t) := 1l + U

t 0

Rk dA†k (s) +

k

(Skl − δkl ) dΛkl (s)

kl

−

Rk∗ Skl

dAl (s) + K ds U (s).

kl

We see that, by the hypotheses on the system operators and the unitarity of U (s), ! (t) is the coefficients Rk U (s), . . . satisfy the conditions in Definition 2.2; then, U well defined by Proposition 2.1 and its matrix elements on exponential vectors are given by Proposition 2.2. So, for every t ≥ 0, u, v ∈ H, f, g ∈ M, we have v ⊗ ! (t) u⊗e(f ) = v⊗e(g)|U (t) u⊗e(f ); having equal matrix elements on a e(g)|U ! (t) and U (t) are equal and this implies that U ! (t) satisfies the total set of vectors, U ! (t) = U (t) = U (t). QSDE (39). The uniqueness of the solution of (39) implies U The Hamiltonian Evolution As soon as Hudson and Parthasarathy introduced their equation, Frigerio and Maassen independently realized that each unitary solution U is naturally associated to a strongly continuous one–parameter unitary group V [50, 51, 73, 74]. This

220

Γt) , Γ!

Alberto Barchielli

is important for physical applications: a strongly continuous one–parameter unitary group is what we want in quantum mechanics to give the dynamics of an isolated system, here system SH and fields. To obtain this result we need to enlarge the Fock space Γ ; it is convenient to consider this ampliation of Γ only in this subsection, because it has no effect in the rest of the paper. With the notations of eq. (6), we have Γ ≡ Γ(0 ; now, let us introduce the spaces Γt) := Γsymm L2 (−∞, t) ⊗ Z and Γ! := Γsymm L2 (R) ⊗ Z ≡ Γ0) ⊗ Γ(0 . With the usual convention of not to write the tensor products with the identity, the solution U (t) of eq. (39) can be understood as a unitary operator on H ⊗ Γ!. Then, we introduce the strongly continuous one–parameter unitary group θ of the shift operators on L2 (R; Z) and its second quantization Θ on Γ!: for every t ∈ R

θt , Θt

θt f (r) = f (r + t),

∀f ∈ L2 (R; Z),

(42a)

Θt e(f ) = e(θt f ),

∀f ∈ L (R; Z);

(42b)

2

we extend Θt to the space H ⊗ Γ!. Now one can prove the cocycle property (43) for U , which Accardi already showed to give rise to groups [1, 7]. Theorem 2.3 ([50, 51, 73, 74]). Let Θ be the strongly continuous one–parameter unitary group defined by (42) and let U be the solution of the QSDE (39) with system operators satisfying the conditions of Theorem 2.2. Then, they are related by the cocycle property (of U with respect to Θ) U (s + t) = Θs∗ U (t) Θs U (s), Vt

U (t, s)

∀s, t ≥ 0,

and the family of unitary operators V = {Vt }t∈R , defined by 1 Θt U (t), if t ≥ 0, Vt = ∗ U (|t|) Θt , if t ≤ 0,

(43)

(44)

is a strongly continuous one–parameter unitary group. Moreover, the two–parameter family of unitary operators U (t, s) := Θt∗ Vt−s Θs ≡ Θs∗ U (t − s)Θs ,

s ≤ t,

(45)

is strongly continuous in t and s and satisfies the composition law U (t, s) U (s, r) = U (t, r) ,

r ≤ s ≤ t.

(46)

The operator U (t, s) is adapted to H ⊗ Γ(s,t) , i.e. it acts as the identity on Γs) ⊗ Γ(t and with respect to t it satisfies the Hudson–Parthasarathy equation (39) with initial condition U (s, s) = 1l. Proof. Let us note that eq. (39) gives also

Quantum Continual Measurements t+s

U (t + s) − U (s) = s

Rk dA†k (r) +

k

−

221

(Skl − δkl ) dΛkl (r)

kl

Rk∗ Skl dAl (r) + K dr U (r) .

(47)

kl

Let us consider Xs (t) := Θs U (s + t)U (s)∗ Θ−s ; note that Xs (0) = 1l. By Proposition 2.2, the definition of Θ (42), the previous equation and a change of integration variable we get / v ⊗ e(g) Xs (t) − 1l u ⊗ e(f ) = v ⊗ e(θ−s g) t+s 2 dr gk (r − s) Rk + gk (r − s) (Skl − δkl ) fl (r − s) s

−

k

kl

3 0 Rk∗ Skl fl (r − s) + K U (r)U (s)∗ u ⊗ e(θ−s f )

kl

t 2 dτ gk (τ ) Rk + gk (τ ) (Skl − δkl ) fl (τ ) = v ⊗ e(g) /

0

k

−

kl

Rk∗ Skl fl (τ )

3 0 + K Xs (τ ) u ⊗ e(f ) .

kl

Therefore Xs (t) satisfies eq. (41) as U (t) and, by Corollary 2.1, U (t) = Xs (t), which is equivalent to the cocycle property (43). Let us prove now the group property for V ; from the definition (44) one has the unitarity of Vt and ∀t ∈ R . (48) Vt∗ = V−t , From the cocycle property (43) and the fact that Θ is a group one gets, ∀t, s ≥ 0, Vt Vs = Θt U (t)Θs U (s) = Θt+s Θs∗ U (t)Θs U (s) = Θt+s U (t + s) = Vt+s . (49) All the other combinations of positive and negative times can be examinated and give the same result. For instance, for s ≤ 0, t+s ≥ 0, one has from (49) Vt+s V−s = Vt , which is equivalent to the group property Vt+s = Vt Vs due to (48). Being V a unitary group, it is enough to prove its strong continuity in 0, which follows from the unitarity and the strong continuity of U and Θ. For t ≥ 0 and Υ ∈ H ⊗ Γ! we have " " " " " " " " " Vt − 1l Υ " = " Θt U (t) − 1l Υ " ≤ "Θt U (t) − 1l Υ " + " Θt − 1l Υ " " " " " = " U (t) − 1l Υ " + " Θt − 1l Υ " → 0 as t ↓ 0 . For t ≤ 0, we have " " " " " Vt − 1l Υ " = " U (|t|)∗ Θt − 1l Υ " " " " " ≤ "U (|t|)∗ Θt − 1l Υ " + " U (|t|)∗ − 1l Υ " " " " " = " Θt − 1l Υ " + " U (|t|) − 1l Υ " → 0

as t ↑ 0 .

222

Alberto Barchielli

From U (t, s) = Θs∗ U (t − s)Θs and Corollary 2.1 one has immediately that U (t, s) is adapted to H ⊗ Γ(s,t) and satisfies the QSDE (39). From U (t, s) = Θt∗ Vt−s Θs and the fact that Θ and Vt are strongly continuous unitary groups one has immediately the composition law (46) and, by using also U (t+r, s)−U (t, s) = Θt∗ (Θr∗ Vr −1l)Vt−s Θs and U (t, s+r)−U (t, s) = Θt∗ Vt−s (Vr∗ Θr −1l)Θs , the strong continuity in t and s. The interaction picture Theorem 2.3 is essential for the interpretation of the whole construction. The group V (44) is the reversible evolution of the isolated system SH plus Bose fields. The free evolution of the fields is supposed to be given by Θ, and hence, physically, the degree of freedom described by L2 (R) is thought to be the conjugate moment of the one–particle energy. Then, U (t) = U (t, 0) = Θt∗ Vt is the evolution operator giving the state dynamics from time 0 to time t of the whole system in the interaction picture with respect to the free field dynamics. In quantum mechanics probabilities, mean values, . . . can be reduced to expressions like as (50) B, ˜st := TrH⊗Γ! {BVt˜sVt∗ } , where ˜s ∈ S(H ⊗ Γ!) is the initial state at time zero and B ∈ B(H ⊗ Γ!). To pass to the interaction picture means to write (50) as B, ˜st = TrH⊗Γ! {B(t)U (t)˜sU (t)∗ } ,

B(t) := Θt∗ BΘt .

(51)

If B(t) ∈ B(H ⊗ Γ ) at a certain time t (i.e. it acts as the identity on Γ0) ) and ˜s = s0) ⊗ s with s0) ∈ S(Γ0) ) and s ∈ S(H ⊗ Γ ), we can get ride of Γ0) and we write (52) B, ˜st = TrH⊗Γ {B(t)U (t)sU (t)∗ } . This is the case when B ∈ B(H) (one gets B(t) = B, ∀t); but this is not the only possible case and also field observables can be involved. By (25a) and (42) one obtains Θs∗ Ak (t)Θs = Ak (t + s) − Ak (s) ,

(53)

which shows that the fields Ak (t), and therefore also A†k (t), Λkl (t), are already in the interaction picture. This conclusion is clearer if we use the heuristic notation (27) and the “energy representation” of the fields: +∞ 1 eiωt ak (t)dt . (54) a ˆk (ω) = √ 2π −∞ Indeed we get Θs∗ Ak (t)Θs =

0

t

1 dτ √ 2π

+∞

−∞

dω e−iω(τ +s) a ˆk (ω) ,

(55)


Θs∗ a ˆk (ω)Θs = e−iωs a ˆk (ω) .

223

(56)

From the next subsection on, we shall go back to use Γ and not Γ!, because automatically we work in the interaction picture and consider only states and observables adapted to (0, +∞) in the sense above. The Hamiltonian operator Being a strongly continuous unitary group, V is differentiable on the domain of its generator, it gives rise to a Schrödinger equation of usual type and a selfadjoint operator with the role of Hamiltonian exists. The characterization of this Hamiltonian required some effort; the results are in Refs. 34–38, 57, 58. Also before these works, it was clear that this Hamiltonian must be unbounded either from above, either from below; in this sense, the dynamics V , or, equivalently, U , must necessarily be an approximation to a “true” dynamics with a physical Hamiltonian bounded from below. Let us also stress that the unitary groups Θ and V are strongly differentiable on the dense domains of their Hamiltonians; being the two Hamiltonians unbounded, there is no surprise that the product U of the two groups be not differentiable. From this point of view the surprise is that U satisfies a closed equation, the QSDE (39). 2.3 The System–Field State Once the dynamical equation (39) is constructed, one needs an initial state

s

s ∈ S(H ⊗ Γ ) . From a mathematical point of view any statistical operator is a possible initial state; from a physical point of view the whole theory is an approximation and whether this approximation is good or not can depend also on the initial state. So, the interpretation of the theory depends not only on the dynamics (37)–(39), but also on the initial state; moreover, such a state must be sufficiently simple to allow computations. The usual choice for the initial state is a factorized state s = ρ0 ⊗ σ ,

ρ0 ∈ S(H) ,

σ ∈ S(Γ ) .

(57) η(f )

Let us use the notation η(f ) := |ψ(f )ψ(f )| ,

f ∈ L2 (R+ ; Z) ,

(58)

for a pure coherent state. The coherent states are the only statistical operators in S(Γ ) which enjoy the factorization property σ = σ(0,s) ⊗ σ(s , σ(0,s) ∈ S(Γ(0,s) ), σ(s ∈ S(Γ(s ), ∀s ≥ 0; indeed, from (8) one has ∀s ≥ 0 , (59) η(f ) = η f(0,s) ⊗ η f(s , with η f(0,s) ∈ S(Γ(0,s) ) , η f(s ∈ S(Γ(s ) .

224

Alberto Barchielli

In the following, we list and comment possible choices for σ. S1.

σ = η(0),

the vacuum [65].

This is the case when the fields act essentially as a reservoir. The reduced dynamics of system SH turns out to be time homogeneous and to be given by a quantum dynamical semigroup. S2.

σ = η(f ),

a coherent state for the field [18].

Now the fields provide also a coherent source which stimulates the system SH . This is the typical choice when a “perfectly” coherent laser is present; a coherent and monochromatic laser could be represented by η(f ) with f (t) = 1[0,T ] (t) e−iωt λ ,

λ∈Z,

ω > 0,

(60)

where T is a very large time; eventually, one takes T → +∞ at the end in the physical quantities. Equation (59) implies a related factorization property for the state at time t in the interaction picture, because U is an adapted process: (61) U (t) [ρ0 ⊗ η(f )] U (t)∗ = U (t) ρ0 ⊗ η f(0,t) U (t)∗ ⊗ η f(t , ∗ with U (t) ρ0 ⊗ η f(0,t) U (t) ∈ S(Γ(0,t) ) , η f(t ∈ S(Γ(t ) . a mixture of coherent states [28]. S3. σ = Ec η(f ) E

c

Here we mean that there is a random variable f in a probability space (Ω c , F c , P c ) with values in L2 (R+ ; Z). Then, the expectation is given by c E η(f ) = η f (·; w) P c (dw), (62) Ωc

where the integral can be understood in the topology induced in T (Γ ) by the duality with B(Γ ); being η(f ) a pure state, this means: ∀A ∈ B(Γ ), ψ f (·; w) A ψ f (·; w) P c (dw). (63) TrΓ {Aσ} = Ωc

It is always possible to think f as a stochastic process defined for times in R+ with values in Z and with trajectories in L2 (R+ ; Z); moreover, by taking a filtration containing its natural one, it is always possible to take as f an adapted, or non anticipating, process. So we complete S3 with S3’. (Ω c , F c , P c ) is a probability space with a filtration {Ftc , t ≥ 0}, i.e. Ftc is a σ-algebra with Fsc ⊂ Ftc ⊂ F c for all times 0 ≤ s ≤ t; f (t), t ≥ 0, is a progressively measurable process, and hence adapted, with f (t; w) ∈ Z, f (·; w) ∈ L2 (R+ ; Z), for w ∈ Ω c . Now the factorization property (61) does not hold, but we have only U (t) [ρ0 ⊗ σ] U (t)∗ = Ec U (t) ρ0 ⊗ η f(0,t) U (t)∗ ⊗ Ec η f(t Ftc (64)


225

As an example take the “phase diffusion model” of a laser, used in Ref. 28 in the study of the fluorescence spectrum of a two–level atom: the field state is given by S3, where f is the process f (t) = e−i(ωt+

√

B W (t))

1(0,T ) (t) λ ,

λ∈Z,

ω > 0,

B ≥ 0;

(65)

W (t) is a real standard Wiener process canonically realized in the Wiener probability space (Ω c , F c , P c ). In the case S3 we have a demixture {η f (·; w) , P c (dw)} of a statistical operator σ into pure states η(f ). Often in quantum mechanics the point of view is taken that in a single, individual experiment a pure state is realized; then, if there is not a perfect control of the preparation, in replicas of the experiment other pure states are realized according to some probability law: mixed states arise due to our imperfect knowledge of the initial state. This interpretation is not always justified, certainly not in the typical situations of statistical mechanics when thermal states and thermodynamical limits enter into play. Another difficulty is that, given a mixed state σ, there are infinitely many demixtures, one of them being the one determined by its eigenvalues and eigenvectors. However, in our case the demixture {η f (·; w) , P c (dw)} can be thought as a special one among the possible demixtures of σ, as the physical one. For instance in the example (65), we have a laser nearly monochromatic, nearly coherent, but with a fluctuating phase, fluctuating in time and from an experiment to another; t → f (t; w) gives the history of the laser in a single experiment, while from an experiment to another it is w to change. In quantum optics the mixtures of coherent states S3, and the particular cases S2 and S1, are called classical states; all the other states are called quantum states. Among the quantum states are the Scrödinger cats, which are quantum superpositions of coherent vectors, such as |αψ(f ) + βψ(g)αψ(f ) + βψ(g)|. To my knowledge, quantum states have never been used as initial states in the “quantum stochastic framework”, when the QSC is based on Fock space; some “non classical” situations have been approached by using versions of QSC based on non Fock representations of the CCR (thermal and squeezed noise) [54, 55].

2.4 The Reduced Dynamics System Observables in the Heisenberg Picture Let us consider any observable X ∈ B(H) of the quantum system SH ; X can be in particular a selfadjoint operator or even a projection operator. . . We already discussed the interaction picture, but we can use also the Heisenberg picture; being Vt the unitary group giving the system field dynamics, the observable X in the Heisenberg picture becomes X(t) = Vt∗ (X ⊗ 1l)Vt . Recalling that Vt = Θt U (t) and that Θt commutes with X ⊗ 1l, we obtain X(t) = U (t)∗ (X ⊗ 1l)U (t). By the rules of QSC, X(t) can be differentiated; the result is a “quantum stochastic” Heisenberg equation.

226

jt

Alberto Barchielli

Proposition 2.5 ([84] Corollary 27.9). Let us define jt (X) := U (t)∗ (X ⊗ 1l)U (t) ,

∀X ∈ B(H) ;

(66)

then, we have ∞ djt (X) = jt L0 [X] dt + jt Rk [X] dA†k (t) k=1 ∞ ∞ + jt Rk [X ∗ ]∗ dAk (t) + jt Skl [X] dΛkl (t) , k=1

L0

(67)

k,l=1

where L0 [X] := i[H, X] −

∞

1 ∗ Rk [Rk , X] + [X, Rk∗ ]Rk , 2

(68a)

k=1

Rk [X] := Skl [X] :=

∞ l=1 ∞

Slk∗ [X, Rl ]

(68b)

∗ Sjk XSjl − δkl X .

(68c)

j=1

The Master Equation ρ(t)

The reduced statistical operator is defined by the partial trace ρ(t) := TrΓ {U (t)sU (t)∗ }

(69)

or, equivalently, by TrH {Xρ(t)} = TrH⊗Γ {jt (X)s} , ρ(f ; t)

If we set

∀X ∈ B(H).

ρ(f ; t) := TrΓ {U (t) (ρ0 ⊗ η(f )) U (t)∗ } ,

(70)

then the reduced statistical operator, for the three choices discussed in Section 2.3, turns out to be given by case S1 ρ(t) = ρ(0; t); case S2 ρ(t) = ρ(f; t); case S3 ρ(t) = Ec ρ(f ; t) . We can always write

ρ(t) = Ec ρ(f ; t)

(71)


227

by understanding that the classical expectation Ec has no effect when f is not random. By Propositions 2.5 and 2.2, ρ(f ; t) satisfies the integral equation ρ(f ; t) = ρ0 +

t

ds L f (s) [ρ(f ; s)],

(72)

0

where the integral can be interpreted again in the topology induced by the duality with B(H) and L f (s) is the bounded operator on T (H) given by ∞

1 L(f )[(] = −i [H(f ), (] + ([Rk (f )(, Rk (f )∗ ] + [Rk (f ), (Rk (f )∗ ]) , (73a) 2 k=1

Rk (f ) = C(zk )∗ [R + (S − 1l) C(f )] , H(f ) = H + i [C(f )∗ R − R∗ C(f )] +

(73b)

i4 C(f )∗ (S − S ∗ ) C(f ) 2

5 − R∗ (S − 1l) C(f ) + C(f )∗ (S ∗ − 1l) R .

(73c)

For a sufficiently regular f , eq. (72) can be differentiated and becomes the quantum master equation d ρ(f ; t) = L f (t) [ρ(f ; t)]. (74) dt The infinitesimal generator L f (t) is known as Liouville operator or Liouvillian; the name comes from the Liouville equation in classical statistical mechanics, which became in quantum mechanics the Liouville–von Neumann equation dρ(t)/dt = −i[H, ρ(t)] for an isolated system and the master equation (74) for an open system without memory. From (73a) the Lindblad structure ([84] Corollary 30.13 p. 268) of the Liouvillian is apparent; by (37), a more compact form is L(f )[(] = −

1 ∗ 1 ∗ R R + R∗ SC(f ) + iH (−( R R + C(f )∗ S ∗ R − iH 2 2 ∗ + TrZ R + SC(f ) ( R + C(f )∗ S ∗ − f 2 ( . (75)

In the case S1 one has the autonomous master equation d ρ(t) = L0 [ρ(t)], dt

(76)

where L0 ≡ L(0) is given by eq. (73a) with f = 0 and its adjoint L0 is given in eq. (68a). In the case S2 the reduced operator ρ(t) satisfies the master equation (74), with a time dependent Liouvillian. Finally, in the case S3, the reduced operator does not satisfy any closed equation.

L(f ), Rk (f ), H(f )

228

Alberto Barchielli

2.5 Physical Basis of the Use of QSC The Quasi–Monochromatic Paraxial Approximation of the Electromagnetic Field In 1978 Yuen and Shapiro [89] started to develop a theory of quantum–field propagation as a boundary–value problem; in particular, they treated the case of quasi–monochromatic paraxial fields, i.e. fields whose significant (nonvacuum state) modes all have temporal frequencies in the vicinity of a nominal carrier fre quency ω0 and satisfy k ⊥ L(ω0 /c)2 , where k ⊥ is the wave–vector component orthogonal to the direction of propagation. In such approximations they found, for the positive and negative frequency parts of the electric field, the CCR with a Dirac delta in time, as in (28). Moreover, they showed that, in the quasimonochromatic paraxial limit, the spatial propagation along the axial direction involves pure translation in time, as for the solutions of the one–dimensional wave equation. These ideas were used by Frigerio and Ruzzier in an attempt to develop a relativistic version of QSC [52] and by the author in developing a photon detection theory [18]. A consequence of the idea of the quasimonochromatic paraxial approximation is that the Hilbert space Z, which appear in the definition of the Fock space Γ , must contain the field degrees of freedom linked to the nominal carrier frequencies involved in the problem, the directions of propagation, the polarization. The possible polarization states for the electromagnetic field are only two (two linear or two circular polarizations) and often, for sake of simplicity, polarization is even not considered. The other two things, nominal carrier frequencies and directions of propagation, depend on what is relevant in the matter–field interaction and, so, the choice of Z depends on the specific problem and, in particular, on the quantum system SH . Approximations in the System–Field Interaction In Ref. 54 Gardiner and Collet discuss the physical approximations needed to pass from a quasi–physical Hamiltonian to an evolution like (39), at least in the case S = 1l. They work with the Heisenberg equations of motion for system operators and obtain at the end equations like (67); let us give an idea of these approximations by working with the evolution operator [18]. Let us consider our system SH interacting with some Bose fields aj (ω) (we are in the frequency domain), satisfying the CCR’s [ai (ω), aj (ω )] = 0,

[ai (ω), a†j (ω )] = δij δ(ω − ω ) .

(77)

A generic system–field interaction, linear in the field operators and in the rotating wave approximation, can be written as 1 Ωj +θj √ HI = i kj (ω) Rj a†j (ω) − Rj∗ aj (ω) dω , (78) 2π Ωj −θj j where the Rj are system operators and the kj (ω) are real coupling constants. We shall consider the limiting case in which the coupling constants become independent


229

of frequency and the field spectrum becomes flat and broad [kj (ω) → 1, θj → +∞]. In quantum optics this is often a good approximation [54]. First we pass to the interaction picture with respect to the free dynamics of the fields and take kj (ω) = 1 (flat spectrum). The interaction Hamiltonian becomes 5 4 Rj a HI (t) = i ˜†j (t) − Rj∗ a ˜j (t) , (79) j

1 a ˜j (t) := √ 2π

Ωj +θj

Ωj −θj

aj (ω) e−iωt dω .

(80)

˜t in the interaction picture can be written as Moreover, the time evolution operator U 2 t 3 ← − ˜ U (t) = T exp −i [H + HI (s)] ds , (81) 0

← − where H is the system Hamiltonian and T is the time–ordering prescription, which is usual in theoretical physics; for a mathematical presentation of the time ordered exponentials in QSC see Ref. 63. By taking the limit θj → +∞ (broad–band approximation), we obtain formally ˜j (t) satisfy the CCR (28). Moreover, we have that the quantities aj (t) = lim a θj →+∞

t

θj →+∞

−→ Aj (t) , 5 4 Rj dA†j (s) − Rj∗ dAj (s) ,

a ˜j (s) ds 0 θj →+∞

−iHI (s) ds

−→

(82a) (82b)

j

˜ (t) U

θj →+∞

−→ U (t) ,

t4 5 ← − † ∗ U (t) ≡ T exp −i H ds + i Rj dAj (s) − Rj dAj (s) . 0

(82c) (83)

j

By writing U (t + dt) in the form 53 2 4 Rj dA†j (t) − Rj∗ DAj (t) Ut , U (t + dt) = exp −iH dt +

(84)

j

by expanding the exponential and by using the multiplication table (32), one sees that U (t) satisfies the Hudson–Parthasarathy equation (39) with S = 1l. Note that the term − 21 Rj† Rj dt in K (37e) comes from the second order term in the expansion of the exponential. Let us stress that this construction shows that the fields aj (t) used in QSC are the formal limit θj → +∞ of the quantities (80). This explains once again the fact that a field aj (t) has to be considered as a wave packet with some carrier frequency Ωj and bandwidth 2θj ; then, the approximation of infinite bandwidth is taken. Many other limiting schemes justifying the Hudson–Parthasarathy equation have been developed, also in mathematically rigourous forms [4–6].

230

Alberto Barchielli

3 Continual Measurements 3.1 Field Observables and Indirect Measurements on SH When the fields represent pure noise, it is natural to consider system observables as in Section 2.4; but in other situations, as when the fields are intended to represent the electromagnetic field, the natural observables are field quantities, from which inferences are done on the system SH . We are interested in the behaviour of the system SH , but we measure field observables; this scheme is known as indirect measurement. Another way to think to this situation is the following one. We cannot act directly on our system SH , but any action is mediated by some quantum input and output channel. We can think of an atom driven by a laser (input) and emitting fluorescence light (output) or of the light entering (input) and leaving (output) an optical cavity. In these examples the role of input and output channels is played by the electromagnetic field and we can think of approximating it by the Bose fields on which QSC is based. So, we have to identify the main field observables, which eventually we want to take under measurement with continuity in time.

Counts of Quanta N (P ; t)

Let P ∈ B(Z) be an orthogonal projection; for any t ≥ 0, we introduce the operator zk |P zl Λkl (t) . (85) N (P ; t) := λ P ⊗ 1(0,t) = kl

By Theorem 2.1, this operator is essentially selfadjoint on E and its domain includes also the finite particle number vectors. From (25c) we have e(g)|N (P ; t)e(f ) = exp g(0,t) |(1l − P )f(0,t) + g(t |f(t ∞ n n g(0,t) |P f(0,t) ; (86) × n! n=0 by taking into account the factorization (10), one sees that the eigenvalues of N (P ; t) are the integers n = 0, 1,. . . and that the eigenspace corresponding to 2 (P Z) ⊗ 1 n is the “n-particle sector of Γ L (R ) ” symm + (0,t) ⊗Γsymm 1l − P ⊗ 1(0,t) Z ⊗ L2 (R+ ) . Therefore, we can interprete N (P ; t) as the number operator which counts the quanta injected in the system up to time t with state in P Z. Another way to see that N (P ; t) is a number operator is to use the heuristic rules of QSC; by (85), (32) and the fact that P is a projection, we have immediately 2 (87) dN (P ; t) = dN (P ; t) ,


which shows that an infinitesimal increment has eigenvalues 0 and 1. By (17) and (85), we have exp{iκN (P ; t)} = W 0; exp{iκP ⊗ 1(0,t) }

231

(88)

and by (14) one sees that the unitary groups generated by N (P ; t) and N (P ; s) commute; therefore, {N (P ; t), t ≥ 0} is a set of jointly diagonalizable selfadjoint operators, or, in physical terms, of compatible observables. The same is true for N (Pα ; t) t ≥ 0 , α = 1, 2, . . . with Pα Pβ = δαβ Pα = δαβ Pα∗ , (89) i.e. P1 , P2 , . . . are mutually orthogonal projections. In the case of photons the measurement of number operators can be experimentally realized through the so called direct detection, which we present in Section 3.4. Measurements of Field Quadratures Let us consider now the field quadratures

t t † Q(h; t) := Q h(0,t) = hk (s) dAk (s) + hk (s) dAk (s) , k

0

Q(h; t) (90)

0

which are essentially selfadjoint operators √ on E (Theorem 2.1). √ The spectrum of Q(h; t) is the whole real axis because ( 2 h)−1 Q(h; t) and ( 2 h)−1 Q(ih; t) form a couple of canonically conjugated selfadjoint operators (the commutator gives i). By (15), (16), we have that 2 Q(hα ; t) , t ≥ 0 , α = 1, 2, . . . , with hα (s)|hβ (s) = δαβ hα (s) , (91) is a family of compatible observables. Definition 2.2 and Proposition 2.1 guarantee that the quantum stochastic integral in (90) is well defined In the case of photons the measurement of field quadratures can be experimentally realized through the so called heterodyne detection, which we present in Section 3.5. Field Observables in the Heisenberg Picture In Section 2.2 we discussed the fact that all the fields we have introduced are expressed in the interaction picture and, so, this is true also for the field observables (85) and (90). However, in order to construct a theory of continual measurements, based on the usual rules of quantum mechanics, which require the existence of joint spectral measures, we need observables commuting at different times in the Heisenberg picture; so, we have to show that the observables introduced above continue to commute at different times even in the Heisenberg picture.

232

Aout j (t) † Aout (t), j out Λij (t),

Qout (h; t), N out (P ; t)

Alberto Barchielli

Let us call “input fields” the fields before the interaction with the system SH , i.e. the fields Ak (t), A†k (t), Λkl (t), . . . and let us call “output fields” the fields after the interaction with the system SH or, in other words, the fields in the Heisenberg picture. We have ∗ (92) Aout j (t) := U (t) Aj (t)U (t) † out (t), Λout (h; t), N out (P ; t). Note that, if D and similar definitions for Aout ij (t), Q j ∗ is the domain of Aj (t), then U (t) D is the domain of Aout j (t) and similar statements for the other operators; Qout (h; t), N out (P ; t) remain selfadjoint operators. By Theorem 2.3 we have

U (T ) = U (T, t)U (t) ,

∀T ≥ t ,

(93)

with U (T, t) adapted to H⊗Γ(t,T ) and, so, commuting with Aj (t), A†j (t), Λij (t), . . . Therefore, we have ∗ Aout j (t) = U (T ) Aj (t)U (T ) ,

∀T ≥ t .

(94)

This implies immediately that the output fields satisfies the same commutation rules of the input fields, for instance the CCR (26): the output fields remain Bose free fields. Moreover, we have that now {N out (Pj ; t), t ≥ 0, j = 1, 2, . . .}, with P1 , P2 , . . . mutually othogonal projections, and {Qout (hj ; t), t ≥ 0, j = 1, 2, . . .}, with h1 (s), h2 (s), . . . mutually orthogonal vectors for any s, are two families of compatible observables in the Heisenberg picture as we wanted. By applying the formal rules of QSC we can express the output fields as the quantum stochastic integrals [14] Aout j (t) =

t 0

† Aout (t) j

Λout ij (t)

=

=

(95a)

,

(95b)

k

t 0

∗

U (s)

∗ Sjk U (s)dA†k (s)

+ U (s)

∗ U (s)∗ Sik Sjl U (s) dΛkl (s) +

kl

+

∗

Rj∗ U (s) ds

k

t 0

U (s)∗ Sjk U (s)dAk (s) + U (s)∗ Rj U (s) ds ,

∗ U (s)∗ Sik Rj U (s) dA†k (s)

k ∗

U (s)

Ri∗ Sjl U (s) dAl (s)

∗

+ U (s)

.

Ri∗ Rj U (s) ds

(95c)

l

From these equations one explicitly sees that the output fields carry information on system SH : the quantities Rk , Skl are the system operators appearing in the system– field interaction. Moreover, these equations allow to write our observables as


N out (P ; t) =

t 0

+

233

U (s)∗ C(zk )∗ S ∗ (1l ⊗ P ) SC(zl )U (s) dΛkl (s)

kl

U (s)∗ C(zk )∗ S ∗ (1l ⊗ P ) RU (s) dA†k (s)

k

+

U (s)∗ R∗ (1l ⊗ P ) SC(zl )U (s) dAl (s)

l

+ U (s) R (1l ⊗ P ) RU (s) ds , (96) ∗

out

Q

(h; t) =

t 0

U (s)∗ C(zk )∗ S ∗ C h(s) U (s) dA†k (s)

k

+

∗

∗ U (s)∗ C h(s) SC(zl )U (s) dAl (s)

l ∗

+ U (s)

4

∗ 5 R C h(s) + C h(s) R U (s) ds ; (97) ∗

these two equations give us an idea of how the output observables depend on the field operators and on the system ones. In eqs. (95)–(97) it is possible to check that the quantum stochastic integrals in the r.h.s. are all well defined, but a rigorous proof of anyone of these formulae needs to use two times Proposition 2.4 and to control the domain of the triple product. However we do not need this, because we can shortcut this difficulty by using Weyl operators. 3.2 Characteristic Functionals Let us recall some very well known facts about selfadjoint operators (observables) and their distribution laws; see for instance Section 10 of Ref. 84. Let X be a selfadjoint operator and exp {ikX} the groupgenerated by X; then, there exists a unique projection–valued measure (pvm) ξ on R, B(R) such that ikX = eikx ξ(dx) , ∀k ∈ R . (98) e R

Let X ≡ (X1 , . . . , Xd ) be a set of d mutually commuting selfadjoint operators, in the sense that the groups generated by them commute or that the associated pvm ξj commute; then, there exists a unique pvm ξ on Rd , B(Rd ) such that e

ik·X

≡

d j=1

e

ikj Xj

eik·x ξ(dx) ,

= Rd

∀k ∈ Rd .

(99)

Moreover, in the state (, the characteristic function (Fourier transform) of the probability law

pvm

234

Alberto Barchielli

P X (dx) = Tr ( ξ(dx)

(100)

of the observable associated to X is eik·x P X (dx) = Tr ( eik·X .

(101)

Rd

These results extend to “infinitely many” commuting selfadjoint operators; only uniqueness is lost. Proposition 3.1. Let {ξt , t ∈ T } be a family of commuting pvm on R, B(R) and let Xt be the selfadjoint operator associated with ξt . Then, there exist a measurable space (Ω, F), 3 a pvm ξ on (Ω, F) and a family of real valued measurable functions 2 ˜ t , t ∈ T on Ω such that X ikXt

e

≡

ikx

e R

˜

eikXt (ω) ξ(dω) ,

ξt (dx) =

∀k ∈ R, t ∈ T .

(102)

Ω

Proof. This proposition is given as an exercise by Parthasarathy ([84] Exercise 10.11 p. 59), with the hint: use Bochner’s Theorem, Kolmogorov’s Consistency Theorem and Zorn’s Lemma. In the situation described in this proposition, if ( is a fixed state and we set P (dω) := Tr{( ξ(dω)} , 2 3 ˜ t (·) , t ∈ T bewe have that (Ω, F, P ) is a classical probability space and X comes a classical stochastic process. The characteristic functions of the finite– dimensional distributions of this process are given by

n n ˜ exp i kj Xtj (ω) P (dω) = Tr ( exp i kj Xtj . (103) Ω

j=1

j=1

Let us consider now the case in which the index becomes time plus a discrete label: T = {(α, s) : α = 1, . . . , d, 0 < s ≤ t}. Then, we denote the ˜ process by X(α, s; ω), the operators by X(α, s) and we assume, for simplicity, ˜ X(α, 0; ω) = 0, X(α, 0) = 0. Instead of considering the finite–dimensional distri˜ butions of the process X(α, s), it is equivalent and simpler to introduce the finite– dimensional distributions of the increments of the original process, whose characteristic functions are Ω

n d ˜ ˜ exp i kα (sj ) X(α, sj ; ω) − X(α, sj−1 ; ω) P (dω) α=1 j=1

n d = Tr ( exp i kα (sj ) X(α, sj ) − X(α, sj−1 ) , α=1 j=1

0 = s0 < s1 < · · · < sn ≤ t .

(104)


235

The Characteristic Functional for the Counts of Quanta Let us consider the family of compatible observables {N (Pα ; t), t ≥ 0, α = 1, 2, . . . , d}; P1 , . . . , Pd are mutually othogonal projections on Z. According to the discussion above and Proposition 3.1, we can handle the stochastic process associated to these operators by means of the finite–dimensional characteristic functions for the increments, which in turn can be summarized in a characteristic functional, which is suggested by the structure of eq. (104) and which now we construct. Let us introduce the test functions k ∈ L∞ R+ ; Rd , the unitary operators St (k) on L2 (R+ ; Z) by d St (k) := exp i Pα ⊗ 1(0,t) kα

(105a)

α=1

or by d St (k)f (s) = exp i1(0,t) (s) kα (s)Pα f (s) α=1

≡ 1(0,t) (s)

d 4

5 eikα (s) − 1 Pα f (s) + f (s)

(105b)

α=1

and the characteristic operator 6t (k) := W 0; St (k) . Φ

(106)

6t (κk) is a unitary group with selfadjoint generaBy (17) and (105a) the map κ → Φ tor λ

Pα ⊗ 1(0,t) kα

α

=

t zk kα (s)Pα zl dΛkl (s) kl

0

α

≡

α

t

kα (s) dN (Pα ; s)

(107)

0

and, so, we can write t 6 Φt (k) = exp i kα (s) dN (Pα ; s) . α

(108)

0

6t (k) contain the Now, by recalling that our initial state is s and that N (Pα ; s) and Φ free–field dynamics, but not the system–field interaction, we can define the characteristic functional by 3 2 6t (k)U (t)sU (t)∗ . (109) Φt (k) := Tr Φ

236

˜α (s) N

Alberto Barchielli

By taking in Φt (k) a simple function k, we obtain a characteristic function of the ˜α (s). All the type (104) for the increments of a process which we denote by N ˜α (s) itself ˜ finite–dimensional distributions for the increments of Nα (s) and for N are contained in the characteristic functional (109). By using the output fields and in particular the property (94), it is suggestive to write 1 t 7 out Φt (k) = Tr exp i kα (s) dN (Pα ; s) s , (110) α

0

where Heisenberg–picture commuting operators N out (Pα ; s) explicitly appear. The Characteristic Functional for the Field Quadratures Let us consider the family of compatible observables {Q(hα ; t), t ≥ 0, α = 2 1, 2, . . . , d}, with hα (s)|hβ (s) = δαβ hα (s) ; we can repeat the construction of the previous subsection. By (90) we have d α=1

t

kα (s) dQ(hα ; s) = Q kα hα ; t

0

(111)

α

and, by taking into account (16), we can write the characteristic operator as an adapted Weyl operator again:

d t 6 kα (s) dQ(hα ; s) Φt (k) = exp i α=1

0

= exp iQ kα hα ; t kα hα 1(0,t) ; 1l . =W i α

˜ α (s) Q

(112)

α

˜ α (s) associated with the selfadThen, the characteristic functional of the process Q joint operators Q(hα ; s) is given by (109) again or by 1

t 7 out Φt (k) = Tr exp i kα (s) dQ (hα ; s) s . α

(113)

0

Field Observables and Adapted Weyl Operators By the use of adapted Weyl operators and characteristic operators we can unify the field observables (85) and (90) and generalize them by including observables of the type (18). By putting together the structures (19) and (112) and by impos6t (k ) = Φ 6t (k + k ), which gives the commutativity of the associated 6t (k) Φ ing Φ observables, we arrive to the following theorem.


237

Theorem 3.1.4 Let B 1 , B 2 , . . 5. , B d be commuting selfadjoint operators in Z, i.e. α β B α = B α∗ , eiκα B , eiκβ B = 0, ∀κα , κβ ∈ R, ∀α, β = 1, . . . , d. Let us take

B1, B2, . . . , Bd

c ∈ L1loc (R+ ; Rd ), b ∈ L2loc (R+ ; Z) and hα ∈ L2loc (R+ ; Z), α = 1, . . . , d, such that

c b hα

α

Imhα (t)|hβ (t) = 0 ,

eiκB hβ (t) = hβ (t) , ∀t ≥ 0,

∀κ ∈ R,

∀α, β = 1, . . . , d. (114) For any test function k ∈ L∞ (R+ ; Rd ) let us define St (k) ∈ U L2 (R+ ; Z) , 6t (k) ∈ U(Γ ) by rt (k) ∈ L2 (R+ ; Z) and the characteristic operator Φ St (k)f (s) = 1(0,t) (s) S k(s) − 1l f (s) + f (s) ,

∀f ∈ L2 (R+ ; Z) , (115a)

d α S k(s) = eikα (s)B ,

(115b)

α=1

rt (k)(s) = 1(0,t) (s) r(k; s) , d

r(k; s) = i

(115c)

kα (s)hα (s) + S k(s) − 1l b(s) ,

(115d)

α=1

t α 6 Φt (k) = exp i ds kα (s)c (s) + Im b(s) S k(s) b(s) 0

α

× W rt (k); St (k) .

(116)

Then, the characteristic operator has the following properties: 1. localization properties: 6t 1(t ,t ) k = Φ 6t 1(t Φ 1

2

2

1 ,t2 )

k ∈ U Γ(t1 ,t2 ) ,

0 ≤ t 1 < t2 ≤ t ;

(117)

2. group property: 6t (k) Φ 6t (k ) = Φ 6t (k + k ) , Φ

∀k, k ∈ L∞ (R+ ; Rd ) ;

(118)

6t (k) is strongly continuous in k ∈ L∞ (R+ ; Rd ) and in t ≥ 0; 3. continuity: Φ 4. matrix elements: 6t (k)e(f ) = e(g)|e(f ) e(g)|Φ

t 1 × exp ds − kα (s)hα (s)|hβ (s)kβ (s) 2 0 αβ α +i kα (s) c (s) + hα (s)|f (s) + g(s)|hα (s) α

+ g(s) + b(s) S k(s) − 1l f (s) + b(s)

;

(119)

St (k) rt (k) 6t (k) Φ

238

Alberto Barchielli

60 (k) = 1l, Φ 6t (k) is the unique unitary solution of 5. given the initial condition Φ the QSDE

6 6 zl S k(t) − 1l zm dΛlm (t) dΦt (k) = Φt (k) +

lm

zl |r(k; t)dA†l (t) −

l

r(k; t)|S k(t) zl dAl (t)

l

kα (t)cα (t) + b(t)| S k(t) − 1l b(t) + i α

1 α β − kα (t)h (t)|h (t)kβ (t) dt . 2

(120)

αβ

ξ(dω) ˜ X(α, t; ·) X(α, t)

Moreover, there exists a measurable 3 a family 2 space (Ω, F), a pvm ξ on (Ω, F), ˜ of real valued measurable functions X(α, t; ·) , α = 1, . . . , d, t ≥ 0 on Ω, a family of commuting and adapted selfadjoint operators X(α, t), α = 1, . . . , d, ˜ t ≥ 0 such that X(α, 0; ω) = 0, X(α, 0) = 0 and, for any choice of n, 0 = t0 < t1 < · · · < tn ≤ t, κjα ∈ R,

n d j 6 Φt (k) = exp i κα X(α, tj ) − X(α, tj−1 ) j=1 α=1

n d ˜ ˜ tj ; ω) − X(α, exp i κjα X(α, tj−1 ; ω) ξ(dω) ,

= Ω

where kα (s) =

(121)

j=1 α=1

n j=1

1(tj−1 ,tj ) (s) κjα .

Proof. Equations (117) follow immediately from the definition of the characteristic operator and from the properties of the Weyl operators. One can check that the definitions of St (k) and rt (k) are such that St (k)St (k ) = St (k + k ) , St (k)−1 = St (k)∗ = St (−k) , rt (k) + St (k)rt (k ) = rt (k + k ) .

(122) (123)

Together with (14) and (114), these equations imply (118). The matrix elements (119) follow by simple computations from the definition (11) of the Weyl operators. 6t (k) and the fact that E is dense, it is enough to prove By the unitarity of Φ the strong continuity on the exponential vectors. By the unitarity and the properties (117) and (118), the strong continuity on the exponential vectors reduces to the check of the continuity of the matrix elements (119). By checking that the condition of Definition 2.2 is satisfied, one has that the r.h.s. of (120) is well defined. By differentiating the matrix elements (119) one gets


239

the QSDE (120); by passing to the equation for the matrix elements, which turns out to be a closed ordinary differential equation, one obtains the uniqueness of the solution. The last statement is an application of Proposition 3.1 to the present case. Continual measurements and infinitely divisible laws ˜ It is important to realize that in a coherent state ψ(f ) the process X(α, t) has independent increments; here we are not considering the interaction with system SH . Indeed, by (119), (121) and (8), one obtains 6t (k)ψ(f ) = ψ(f )|Φ

n /

d κjα X(α, tj ) ψ(1(tj−1 ,tj ) f ) exp i α=1

j=1

0 − X(α, tj−1 ) ψ(1(tj−1 ,tj ) f ) ;

(124)

by the localization properties (117), we can reintroduce ψ(f ) in every factor and we obtain, again by (121), the independence of the increments:

n d ˜ ˜ tj ; ω) − X(α, exp i κjα X(α, tj−1 ; ω) ψ(f )|ξ(dω)ψ(f )

Ω

=

j=1 α=1 n

j=1

Ω

d ˜ ˜ tj ; ω) − X(α, exp i κjα X(α, tj−1 ; ω) ψ(f )|ξ(dω)ψ(f ). α=1

(125) This fact implies that, in a time–homogeneous case, the increments follow an infinitely divisible law. Indeed, let us take f = 0, b(s) = b, c(s) = c, h(s) = h, kα (s) = κα and let us denote by ζB (dx) the joint spectral measure of the B’s; then, one has

d 0 / iκα X(α,t) 6 ψ(0) Φt (κ) ψ(0) ≡ ψ(0) e ψ(0) = exp it κα cα α

α=1

4 5 t exp i − κα hα |hβ κβ + t κα xα − 1 b|ζB (dx)b . 2 Rd α

(126)

αβ

By comparing this result with the Lévy–Khintchin formula, one sees that (126) is the characteristic function of an infinitely divisible distribution on Rd , but not the most general one because b|ζB (dx)b is a finite measure. The representations of infinitely divisible laws have been studied ([84] Section 21) and from there we can take a suggestion on how we can generalize the ob6t (k) are maintained and the most servables of Theorem 3.1. All the properties of Φ general infinitely divisible distribution is obtained if everywhere in Theorem 3.1 8 2 1+|B|2 b(s) and cα (s) by cα (s) − b(s) 1+|B| B α b(s) ; here b(s) is replaced by 2 2 |B|

|B|

240

Alberto Barchielli

d 2 |B|2 := α=1 (B α ) . This is only an indication of a possible generalization, but we do not touch any more this more general characteristic operator in this work. The output characteristic operator 6out (k) Φ t

The observables in the Heisenberg description can now be introduced implicitly by defining the output characteristic operator 6t (k)U (t) . 6out (k) = U (t)∗ Φ Φ t

(127)

t out 6out Φ (k) = exp i k (s) dX (α; s) , α t

(128)

Formally we have

α

0

but we do not need to give a rigourous meaning to the “Heisenberg” observables X out (α; t) and to the integrals with respect to dX out (α; s); all we need is to differ6out (k), which is done in Proposition 3.2. entiate Φ t

The Characteristic Functional and the Finite Dimensional Laws Φt (k)

∆X(t1 , t2 ) ξ(dx; t1 , t2 )

By considering also the interaction with system SH , we have that the characteristic ˜ is again given by (109): functional of the process X 3 2 2 3 6out 6t (k)U (t)sU (t)∗ ≡ Tr Φ Φt (k) = Tr Φ (129) t (k)s . All the probabilities describing the continual measurement of the observables X(α, t) are contained in Φt (k); let us give explicitly the construction of the joint probabilities for a finite number of increments. 2 3 ˜ The measurable functions X(α, t; ·) , α = 1, . . . , d, t ≥ 0 , introduced in Theorem 3.1, represent the output signal of the continual measurements. Let us ˜ ˜ ˜ ˜ denote by ∆X(t1 , t2 ) = X(1, t2 ) − X(1, t1 ), . . . , X(d, t2 ) − X(d, t1 ) the vector of the increments of the output in the time interval (t1 , t2 ) and by ξ(dx; t1 , t2 ) the joint pvm on Rd of the increments X(α; t2 ) − X(α; t1 ), α = 1, . . . , d. Note that, because of the properties of the characteristic operator, not only the different components of an increment are commuting, but also increments related to different time intervals; this implies that the pvm related to different time intervals commute. Moreover, the localization properties of the characteristic operator give ξ(A; t1 , t2 ) ∈ B(Γ(t1 ,t2 ) ) ,

for any Borel set A ⊂ Rd .

(130)

As in the last part of Theorem 3.1, let us consider 0 = t0 < t1 < · · · < tn ≤ t, n kα (s) = j=1 1(tj−1 ,tj ) (s) κjα , κj = κj1 , . . . , κjd ; then we can write


241

d n Φt (k) = Tr exp i κjα X(α, tj ) − X(α, tj−1 ) U (t)sU (t)∗ = Rnd

n

j=1 α=1

e

iκj ·xj

Pρ0 ∆X(t0 , t1 ) ∈ dx1 , . . . , ∆X(tn−1 , tn ) ∈ dxn ,

j=1

(131) where the physical probabilities are given by Pρ0 ∆X(t0 , t1 ) ∈ A1 , . . . , ∆X(tn−1 , tn ) ∈ An

n = Tr ξ(Aj ; tj−1 , tj ) U (t)sU (t)∗ .

(132)

j=1

Obviously, Φt (k) is the characteristic function of the physical probabilities Pρ0 ∆X(t0 , t1 ) ∈ A1 , . . . , ∆X(tn−1 , tn ) ∈ An and it uniquely determines them. 3.3 The Reduced Description of the Continual Measurements An essential step in the theory is to eliminate the degrees of freedom of the fields and to pass to a reduced description based only on system SH . This is similar to the passage to the reduced dynamics in Section 2.4 and, indeed, the quantities ρ(f ; t) (70) and L f (t) (73) will be involved also here. The Reduced Characteristic Operator Definition 3.1. For f ∈ L2 (R+ ; Z), k ∈ L∞ (R+; Rd ), t ≥ 0, let us define the reduced characteristic operator Gt (f ; k) ∈ B T (H) by: ∀a ∈ B(H), ∀( ∈ T (H), 2 3 6t (k) U (t) ( ⊗ η(f ) U (t)∗ . (133) TrH a Gt (f ; k)[(] = TrH⊗Γ a ⊗ Φ Let us recall that the symbol η(f ) for a coherent state is defined in eq. (58). By the definition of reduced characteristic functional, for the three choices of initial state proposed in Section 2.3 the characteristic functional is given by S1. Φt (k) = TrH Gt (0; k)[ρ0 ] , S2. Φt (k) = TrH Gt (f ; k)[ρ0 ] , S3. Φt (k) = Ec TrH Gt (f ; k)[ρ0 ] ; let us recall that in this case f is random. In (133) only unitary operators are involved and this implies that it is easy to apply Proposition 2.4 to the triple product; we get the following results. 6out (k) and Gt (f ; k) be defined by (127), (133), with all the Proposition 3.2. Let Φ t hypotheses given in the previous sections.

Gt (f ; k)

242

Alberto Barchielli

The output characteristic operator (127) satisfies the QSDE ∗ 6out dΦ t (k) = U (t)

+ +

4

C(zl )∗ S ∗ S k(t) − 1l SC(zm ) dΛlm (t)

lm

C(zl )∗ S ∗ C r(k; t) + S k(t) − 1l R dA†l (t)

l

∗ 5 −C r(k; t) S k(t) + R∗ S k(t) − 1l SC(zl ) dAl (t)

l

+ b(t)| S k(t) − 1l b(t) + i kα (t)cα (t) α

1 − kα (t)hα (t)|hβ (t)kβ (t) + R∗ C r(k; t) 2 αβ ∗ ∗ 6out (k) . − C r(k; t) S k(t) R + R S k(t) − 1l R dt U (t)Φ t The reduced characteristic operator satisfies the equation t Gt (f ; k)[(] − ( = Ks f ; k(s) ◦ Gs (f ; k)[(] ds ,

(134)

(135)

0

Kt (f ; κ)

with generator 2 3 Kt (f ; κ)[(] = L f (t) [(] + TrZ 1l ⊗ (S(κ) − 1l) J (f ; t)[(] 1 − κα hα (t)|hβ (t)κβ ( + i κα Z α (f ; t)( + (Z α (f ; t)∗ , (136a) 2 α αβ

∗ 1 α c (t) + C hα (t) R + SC f (t) , (136b) 2 4 ∗ ∗ 5 ; J (f ; t)[(] = R + SC f (t) + C b(t) ( R∗ + C f (t) S ∗ + C b(t) (136c) L f (t) is given by eq. (75). Z α (f ; t) =

Z α (f ; t), J (f ; t)

6t (k); due to the unitarity of the Proof. Let us apply Proposition 2.4 to U (t)∗ a ⊗ Φ adapted processes involved, there is no problem to control the domains and we get

6t (k) 6t (k) = U (t)∗ Φ d U (t)∗ a ⊗ Φ C(zl )∗ S ∗ a ⊗ S k(t) − a ⊗ 1l × C(zm ) dΛlm (t) − +

l

l

lm

C(zl )∗ S ∗ R − C r(k; t) a dA†l (t)

∗ R − C r(k; t) a ⊗ S k(t) C(zl ) dAl (t) ∗


243

+ K ∗ a + b(t)| S k(t) − 1l b(t)a + i kα (t)cα (t) a α

1 α β ∗ kα (t)h (t)|h (t)kβ (t) a + R C r(k; t) a dt . − 2

(137)

αβ

By appling Proposition 2.4 again we get

∗ ∗ 6 d U (t) a ⊗ Φt (k) U (t) = U (t) C(zl )∗ S ∗ a ⊗ S k(t) S − a ⊗ 1l × C(zm ) dΛlm (t) − +

4

lm

C(zl )∗ S ∗

R − C r(k; t) a − a ⊗ S k(t) R dA†l (t)

l

5 ∗ R∗ − C r(k; t) a ⊗ S k(t) − aR∗ SC(zl ) dAl (t)

l

kα (t)cα (t) a + L0 [a] + b(t)| S k(t) − 1l b(t)a + i α

1 − kα (t)hα (t)|hβ (t)kβ (t) a + R∗ C r(k; t) a 2 αβ ∗ ∗ 6t (k) U (t). − C r(k; t) a ⊗ S k(t) R + R a ⊗ S k(t) − 1l R dt Φ

(138)

By taking the matrix elements with respect to the coherent vector |ψ(f ) we get eqs. (135), (136a); by taking a = 1l we get (134). If the time dependence of the generator is sufficiently regular we have the differential equation d Gt (f ; k)[(] = Kt f ; k(t) ◦ Gt (f ; k)[(] , G0 (f ; k) = 1l , (139) dt which is a modification of a master equation. This kind of equations was introduced in [22, 23], inside of the operational approach, and it was related to the approach based on QSDE in [24]. The problem of generators of the type (136a) was studied in [25, 61, 62]. Let us define a two–time modification of the reduced characteristic operator by t2 Ks (f ; κ) ◦ Gts1 (f ; κ)[(] ds . (140) Gtt12 (f ; κ)[(] − ( = t1

Then, for 0 = t0 < t1 < · · · < tn ≤ t, kα (s) = κj1 , . . . , κjd , eq. (135) gives

n j=1

1(tj−1 ,tj ) (s) κjα , κj =

n Gt (f ; k) = Gttn (f ; 0) ◦ Gttn−1 (f ; κn ) ◦ · · · ◦ Gtt01 (f ; κ1 ) .

(141)

Moreover, we have Gtt23 (f ; κ) ◦ Gtt12 (f ; κ) = Gtt13 (f ; κ) .

(142)

Gtt12 (f ; κ)

244

Alberto Barchielli

The reduced dynamics Υ (f ; t, s)

Let us set Υ (f ; t, s) := Gst (f ; 0) ;

(143)

by (141) we have the composition law Υ (f ; t3 , t1 ) = Υ (f ; t3 , t2 ) ◦ Υ (f ; t2 , t1 ) ,

0 ≤ t1 ≤ t2 ≤ t3 .

(144)

Then, by comparing (72) with (135), (136a), (144) we obtain ρ(f ; t) = Υ (f ; t, 0)[ρ0 ] = Υ (f ; t, s)[ρ(f ; s)] .

(145)

In the case S2 the reduced statistical operator is ρ(t) = ρ(f ; t) and, so, Υ (f ; t, s) has the meaning of reduced evolution operator from s to t; eq. (144) says that this evolution is in some sense without memory. In the case S3 we have ρ(t) = Ec Υ (f ; t, 0)[ρ0 ] = Ec Υ (f ; t, s)[ρ(f ; s)] (146) and the lack–of–memory property is lost. From eqs. (140), (143), (136a) we get t2 Υ (f ; t2 , t1 )[(] − ( = L f (s) ◦ Υ (f ; s, t1 )[(] ds ,

(147)

t1

which is another form of the master equation (74). Instruments and Finite–Dimensional Laws

Itt12 (f ; A)

instrument

In the quantum theory of measurement an important notion is that of instrument and the operational approach to continual measurements, mentioned in the Introduction, is based on such a notion. Here we recall a few facts, without developing in full this side of the theory. By using the joint pvm ξ(dx; t1 , t2 ) of the increments X(α; t2 ) − X(α; t1 ), α = 1, . . . , d, we define the map–valued measure Itt12 (f ; ·), 0 ≤ t1 < t2 , f ∈ L2 (R+ ; Z), by: ∀a ∈ B(H), ∀( ∈ T (H), TrH a Itt12 (f ; A)[(] = TrH⊗Γ {a ⊗ ξ(A; t1 , t2 ) U (t2 , t1 ) ( ⊗ η(f ) U (t2 , t1 )∗ } , (148) where A is a Borel set in Rd ; by the factorization properties of Γ and η(f ), only f(t1 ,t2 ) , the part of f in (t1 , t2 ), is relevant for the definition of Itt12 (f ; A). The family of maps Itt12 (f ; ·) is a completely positive instrument [44, 64], whose characterizing properties are 1. Itt12 (f ; A) ∈ B T (H) ; t2 2. Tr It1 (f ; Rd )[(] = Tr {(}, ∀( ∈ T (H); n 3. Tr a∗i aj Itt12 (f ; A) |ψj ψi | ≥ 0, ∀n, ∀ψj ∈ H, ∀aj ∈ B(H); i,j=1


245

4. for any finite or countable (Borel) partition A1 , A2 , . . . of a Borel set A one has t2 t2 j It1 (f ; Aj )[(] = It1 (f ; A)[(], ∀( ∈ T (H). Then, Gtt12 (f ; κ) is the Fourier transform of the instrument Itt12 (f ; ·), i.e. t2 Gt1 (f ; κ)[(] = eiκ·x Itt12 (f ; dx)[(] , ∀( ∈ T (H) ,

(149)

Rd

and a Bochner type theorem holds which says that G uniquely determines I, see [25] p. 110 Theorem 1.5. By (131), (132), (141), (149) the probabilities (132) are given by Pρ0 ∆X(t0 , t1 ) ∈ A1 , . . . , ∆X(tn−1 , tn ) ∈ An 4 2 35 n (f ; An ) ◦ · · · ◦ Itt01 (f ; A1 )[ρ0 ] ; = Ec TrH Ittn−1

(150)

we use the convention that the classical expectation Ec has no effect when f is not random. Mean Values and Covariances ˜ As usual, all the moments of the process X(α, t) can be obtained by derivation of the characteristic functional. If we take kα (t) = κ1 δαα1 1(0,t1 ) (t) + κ2 δαα2 1(0,t2 ) (t) ,

(151)

the mean and the second moments are given by 4 5 ˜ j , tj ) = −i ∂ Φt ∨t (k) , Eρ0 X(α 1 2 ∂κj κ=0 ∂2 Φt1 ∨t2 (k) , ∂κ1 ∂κ2 κ=0 when they exist. Obviously, the covariance function is 4 5 ˜ 1 , t1 )X(α ˜ 2 , t2 ) = − Eρ0 X(α

4 5 ˜ 1 , t1 ), X(α ˜ 2 , t2 ) Cov X(α 4 4 4 5 5 5 ˜ 1 , t1 )X(α ˜ 1 , t1 ) Eρ X(α ˜ 2 , t2 ) . ˜ 2 , t2 ) − Eρ X(α = Eρ0 X(α 0 0

(152)

(153)

(154)

Proposition 3.3. Let the operators B α be bounded; then we have tj ∂ −i TrH {Gt1 ∨t2 (f ; k)[ρ0 ]} = dt TrH {Y αj (f ; t)ρ(f ; t)} , (155) ∂κj κ=0 0

−

∂2 TrH {Gt1 ∨t2 (f ; k)[ρ0 ]} ∂κ1 ∂κ2 κ=0

246

Alberto Barchielli

t1 ∧t2

= + + 0

0

t1

dt 0 t2 dt

dt [hα1 (t)|hα2 (t) + TrH {J α1 α2 (f ; t) ρ(f ; t)}]

t∧t2

0 t∧t1

ds TrH {Y α1 (f ; t)Υ (f ; t, s) ◦ Y α2 (f ; s)[ρ(f ; s)]}

ds TrH {Y α2 (f ; t)Υ (f ; t, s) ◦ Y α1 (f ; s)[ρ(f ; s)]} ,

(156)

0

where Y α (f ; t)[(] = Z α (f ; t)( + (Z α (f ; t)∗ + TrZ {1l ⊗ B α J (f ; t)[(]} ,

(157a)

4 ∗ Y α (f ; t) = Z α (f ; t) + Z α (f ; t)∗ + R∗ + C f (t) S ∗ 4 5 ∗ 5 + C b(t) 1l ⊗ B α R + SC f (t) + C b(t) , (157b) 4 ∗ ∗ 5 J αβ (f ; t) = R∗ + C f (t) S ∗ + C b(t) 1l ⊗ B α B β R + SC f (t) + C b(t) , (157c) Proof. From the definition of K (136a) and eq. (151) we get ∂ −i Ks f ; k(s) = 1(0,tj ) (s) Y αj (f ; s) , ∂κj κ=0

−

4 ∂2 Ks f ; k(s) [(] = 1(0,t1 ∧t2 ) (s) hα1 (t)|hα2 (t)( ∂κ1 ∂κ2 κ=0 2 + TrZ 1l ⊗ B α1 B α2 R + SC f (t) + C b(t) ∗ ∗ 35 . ( R∗ + C f (t) S ∗ + C b(t)

(158)

(159)

By (135), (143) we obtain −i

−

t ∂ ∂ Gt (f ; k) = ds (−i) Ks f ; k(s) ◦ Υ (f ; s, 0) ∂κj ∂κj κ=0 κ=0 0 t ∂ ds L f (s) ◦ (−i) Gs (f ; k) , + ∂κ κ=0 j 0

(160)

t ∂2 ∂2 Gt (f ; k) =− ds Ks f ; k(s) ◦ Υ (f ; s, 0) ∂κ1 ∂κ2 ∂κ1 ∂κ2 κ=0 κ=0 0 t ∂ ∂ ds (−i) Ks f ; k(s) ◦ (−i) Gs (f ; k) + ∂κ ∂κ κ=0 κ=0 1 2 0


247

t ∂ ∂ + ds (−i) Ks f ; k(s) ◦ (−i) Gs (f ; k) ∂κ ∂κ κ=0 κ=0 2 1 0 t 2 ∂ − ds L f (s) ◦ Gs (f ; k) . ∂κ ∂κ κ=0 1 2 0 By using (147), one can check that the solution of eq. (160) is t∧tj ∂ −i Gt (f ; k) = ds Υ (f ; t, s) ◦ Y αj (f ; s) ◦ Υ (f ; s, 0) ; ∂κj κ=0 0

(161)

(162)

then, this expression can be inserted into (161). By applying the expressions (160), (161) to ρ0 , by taking the trace and by using the definitions (157), one gets the final result. Note that the first and second moments turn out to be given by 5 tj 4 ˜ j , tj ) = Eρ0 X(α dt Ec [TrH {Y αj (f ; t)ρ(f ; t)}] ,

(163)

0

5 4 ˜ 1 , t1 )X(α ˜ 2 , t2 ) Eρ0 X(α t1 ∧t2 4 5 = dt hα1 (t)|hα2 (t) + Ec [TrH {J α1 α2 (f ; t) ρ(f ; t)}] 0 t1 t∧t2 dt ds Ec [TrH {Y α1 (f ; t)Υ (f ; t, s) ◦ Y α2 (f ; s)[ρ(f ; s)]}] + 0 0 t2 t∧t1 dt ds Ec [TrH {Y α2 (f ; t)Υ (f ; t, s) ◦ Y α1 (f ; s)[ρ(f ; s)]}] , (164) + 0

0

3.4 Direct Detection The Detection Scheme The measurement of an observable of the type N (P ; t) can be realized according to the scheme of Fig. 1, called direct detection. o /o /o /o /o /o /o o/ System SH /o /o /o /o o/ output /o /o /o /o /o o/ / Photocounter O field O O O f (t) O I(t) O O O input field

output field

Fig. 1. Direct detection

248

I(t)

Alberto Barchielli

The system SH is stimulated by some input field, say in a coherent state ψ(f ) or in a mixture of coherent states; then, it emits fluorescence light in various directions. A part of this output field reaches a photoelectron counter which produces some output current I(t) “proportional” to the rate of arrival of the photons. By denoting ˜ (t) the process which counts the photons arriving to the photocounter and by by N using Stieltjes integrals, the output current can be written as t ˜ (s) , F (t − s) dN (165) I(t) = 0

F (t)

where F is a response function which characterizes the apparatus. A typical choice is γ˜ F (t) = k exp − t ; (166) 2 k > 0 and γ˜ > 0 are constants which depend on the apparatus. If we do not consider the time–of–flight from the system SH to the detector and we denote by P the projection which gives the part of the field reaching the counter, we can say that the direct detection scheme described here realizes a continual measurement of the observables N (P ; t), t ≥ 0. There is no conceptual difficulty in considering more counters together, but we prefer to continue to study the case of a single detector. The general results given in the previous sections apply to the present case by taking

L˜ f (t) Y(f ; t) Y (f ; t)

˜ ˜ ˜ (t), • d = 1, X(α, t) ≡ X(t) = N (P ; t), X(α, t) ≡ X(t) =N α α • h (t) = 0, c(t) = 0, b(t) = 0, which gives Z (f ;t) = 0, r(k; t) = 0, • B α = P , with P 2 = P ∗ = P , which gives S k(t) − 1l = eik(t) − 1 P . Then, we obtain Kt (f ; k)[(] = L˜ f (t) [(] + eik(t) Y(f ; t)[(] ,

(167a)

˜ )[(] = − 1 R∗ R + R∗ SC(f ) + iH (−( 1 R∗ R + C(f )∗ S ∗ R − iH L(f 2 2 ∗ + TrZ 1l ⊗ (1l − P ) R + SC(f ) ( R + C(f )∗ S ∗ − f 2 ( , (167b) 2 Y α (f ; t)[(] ≡ Y(f ; t)[(] = TrZ 1l ⊗ P R + (S − 1l) C f (t) + C P f (t) 4 ∗ ∗ 53 ( R∗ + C f (t) (S ∗ − 1l) + C P f (t) , (167c) 4 ∗ ∗ 5 Y α (f ; t) ≡ Y (f ; t) = R∗ + C f (t) S ∗ − 1l + C P f (t) 4 5 1l ⊗ P R + S − 1l C f (t) + C P f (t) , (167d)


J αβ (f ; t) ≡ J(f ; t) = Y (f ; t)

249

(167e)

Usually the detector is placed in a position in which it is not reached by the direct light of the stimulating laser; in mathematical terms we have P f (t) = 0 ,

∀t .

(168)

Equations (167c) and (167d) are written in a way that puts in evidence the terms that disappear when condition (168) holds. Moments ˜ , the first two moments (163), (164) become In the case of the counting process N 5 t 4 ˜ (t) = Eρ0 N dτ Ec [TrH {Y (f ; τ )ρ(f ; τ )}] , (169) 0

4 5 4 5 ˜ (t)N ˜ (s) = Eρ N ˜ (t ∧ s) Eρ0 N 0 t∨s t∧s + dτ1 dτ2 Ec [TrH {Y (f ; τ1 )Υ (f ; τ1 , τ2 ) ◦ Y(f ; τ2 )[ρ(f ; τ2 )]}] t∧s 0 τ1 t∧s dτ1 dτ2 Ec [TrH {Y (f ; τ1 )Υ (f ; τ1 , τ2 ) ◦ Y(f ; τ2 )[ρ(f ; τ2 )]}] . +2 0

0

(170) Then, for the output current (165) we get Eρ0 [I(t)] = k

t

dτ e−˜γ (t−τ )/2 Ec [TrH {Y (f ; τ )ρ(f ; τ )}] ,

(171)

0

t∧s t+s Eρ0 [I(t)I(s)] = k2 dτ e−˜γ ( 2 −τ ) Ec [TrH {Y (f ; τ )ρ(f ; τ )}] 0 t∨s t∧s t∧s τ1 dτ1 dτ2 + 2 dτ1 dτ2 e−˜γ (t+s−τ1 −τ2 )/2 + k2 t∧s

0

0

0

× E [TrH {Y (f ; τ1 )Υ (f ; τ1 , τ2 ) ◦ Y(f ; τ2 )[ρ(f ; τ2 )]}] . c

(172)

In photocounting problems it is usual to measure the deviations from the variance of the Poisson process by means of the Mandel Q-parameter [19], defined by 5 5 4 4 ˜ (t) − N ˜ (s) − Eρ N ˜ (t) − N ˜ (s) Var N 0 4 5 Q(t, s) = , t > s. (173) ˜ (t) − N ˜ (s) Eρ0 N

Q(t, s)

250

Alberto Barchielli

For a Poisson process one has Q(t, s) = 0; the terms sub- and super–Poissonian statistics are used for the cases Q(t, s) < 0 and Q(t, s) > 0, respectively. The sub– Poissonian case Q(t, s) < 0 is considered as an index of “nonclassical” light. In our case we obtain the expressions 4 5 t ˜ ˜ dτ Ec [TrH {Y (f ; τ )ρ(f ; τ )}] , (174) Eρ0 N (t) − N (s) = s

Eρ0

2 5 4 ˜ (t) − N ˜ (s) ˜ (t) − N ˜ (s) N = Eρ0 N

t

+2

τ1

dτ1

dτ2 Ec [TrH {Y (f ; τ1 )Υ (f ; τ1 , τ2 ) ◦ Y(f ; τ2 )[ρ(f ; τ2 )]}] ,

s

s

(175)

dτ E [TrH {Y (f ; τ )ρ(f ; τ )}] c

Q(t, s) = 2 ×

t

−1

t

s τ1

2 dτ2 Ec [TrH {Y (f ; τ1 )Υ (f ; τ1 , τ2 ) ◦ Y(f ; τ2 )[ρ(f ; τ2 )]}] s 3 − Ec [TrH {Y (f ; τ1 )ρ(f ; τ1 )}] Ec [TrH {Y (f ; τ2 )ρ(f ; τ2 )}] . (176)

dτ1 s

In reality the interesting case, for which the Mandel Q-parameter was introduced, is that of a counting process with stationary increments; so, the most useful parameter is (177) Q := lim Q(t, 0) , t→+∞

if this limit exists. Probabilities for Counts Let us note that the operator L f (t) = Kt (f ; 0) = L˜ f (t) + Y(f ; t) Υ˜ (f ; t, s)

(178)

generates the dynamics Υ (f ; t, s) through eq. (147). In the probabilities constructing it is useful to introduce similar maps generated by L˜ f (t) : Υ˜ (f ; t, s)[(] − ( =

t

L˜ f (τ ) ◦ Υ˜ (f ; τ, s)[(] dτ .

(179)

s

Such maps turn out to be positive (even completely positive), but not trace preserving: 2 3 ( ≥ 0 ⇒ Υ˜ (f ; t, s)[(] ≥ 0 , TrH Υ˜ (f ; t, s)[(] ≤ TrH {(} . (180)


251

By using Υ˜ (f ; t, s) and Y(f ; t), we define the completely positive maps on T (H) Ist (f ; 0) =Υ˜ (f ; t, s) , t tm t Is (f ; m) = dtm dtm−1 · · · s

s

t2

dt1 Υ˜ (f ; t, tm )

s

(181)

◦ Y(f ; tm ) ◦ Υ˜ (f ; tm , tm−1 ) ◦ Y(f ; tm−1 ) ◦ · · · ◦ Υ˜ (f ; t2 , t1 ) ◦ Y(f ; t1 ) ◦ Υ˜ (f ; t1 , s) . Then, one can check that the solution of eq. (140) with generator (167a) can be written as ∞ eimκ Ist (f ; m) ; (182) Gst (f ; κ) = m=0

in the physical literature solutions of evolution equations written as expansions with respect to a part of the generator are called Dyson series. By the connection (149) with the instruments, we immediately identify {Ist (f ; m), m = 0, 1, . . .} as the instrument giving the counts in the time interval (s, t]. Instruments for counts of such a type were introduced by Davies [43, 44]. By combining eqs. (150) and (181), we can say that the quantities 4 2 35 (183a) Pt (0|ρ0 ) = Ec TrH Υ˜ (f ; t, 0)[ρ0 ] , 4 2 pt (tm , tm−1 , . . . , t1 |ρ0 ) = Ec TrH Υ˜ (f ; t, tm ) ◦ Y(f ; tm ) ◦ Υ˜ (f ; tm , tm−1 ) 35 ◦ Y(f ; tm−1 ) ◦ · · · ◦ Υ˜ (f ; t2 , t1 ) ◦ Y(f ; t1 ) ◦ Υ˜ (f ; t1 , 0)[ρ0 ] (183b) determine all the probabilities for counts. The quantity (183a) is the probability of having no count in the time interval (0, t], when the initial state of the system is ρ0 , and the probability of exactly m counts in the interval (0, t] is tm t t2 Pt (m|ρ0 ) = dtm dtm−1 · · · dt1 pt tm , tm−1 , . . . , t1 |ρ0 . (184) 0

0

0

The quantity (183b) is the probability density of a count at time t1 , a count at time t2 ,. . . , and no other count in the interval (0, t]; these quantities are called exclusive probability densities and from them also more complicated probabilities can be obtained. Indeed, the characteristic functional (129), from which all probabilities can be computed, turns out to be writable as Φt (k) = Pt (0|ρ0 ) +

∞ m=1

t

dtm

0

dtm−1 0

0

···

tm

t2

m dt1 exp i k(tn ) pt (tm , . . . , t1 |ρ0 ). n=1

(185)

252

Alberto Barchielli

3.5 Optical Heterodyne Detection Ordinary Heterodyne Detection

A0 (t) Γ

0

Also a different kind of measurement, the so called heterodyne detection [87, 90], can be described by using QSC. By inserting a beam splitter (a half transparent mirror) before the photoelectron counter, the output field from SH is made to beat with an intense laser field (local oscillator); only then, the intensity of the compound beam is measured by the photoelectron counter. This measurement scheme is illustrated in Fig. 2. Let us introduce a new field A0 (t) which does not interact with SH and which can be used to describe the local oscillator; the initial state of this new field is taken to be a coherent vector ψ(f0 ), where > 0 is a parameter which we shall send to infinity in order to have a very intense laser field. The space is now 0 Γ ⊗ Γ , Fock 0 2 0 2 Γ = Γ L (R+ ) ; we can also write Γ ⊗ Γ = Γ L (R+ ) ⊗ (C ⊕ Z) . Let us assume that the basis {zk } in Z is chosen in such a way that the index contains the direction of propagation and that only field 1 reaches the beam splitter. So, at the two input ports of the beam splitter the fields Aout 1 (t) and A0 (t) arrive. Let us call B+ (t) and B− (t) the fields leaving the two output ports; they are given by 1 1 B+ (t) = √ Aout 1 (t) + √ A0 (t) , 2 2 1 1 out B− (t) = √ A0 (t) − √ A 1 (t) . 2 2

(186)

In other terms the beam splitter operates the unitary transformation (z0 , z1 ) → (z+ , z− ), z± = √12 (z0 ± z1 ). The phases of all the fields can always be redefined in order to have no additional phase shifts in (186). Note that the B-fields satisfy the CCR’s as the input and the output A-fields. A photoelectron counter is placed in such a way that it collects the light coming out from one of the output ports of the beam splitter; let us say port 1. The detector

O

O

I(t) beam splitter O O /o output /o /o /o /o /o /o / O /o /o /o /o output /o /o /o / Photocounter port 1 field O O OO O local oscillator O O O output port 2

o/ /o /o o/ System SH o /o /o /o output O field O O O f (t) O O O O

O

O O O O

O

f0 (t)

Fig. 2. Heterodyne detection


253

counts the photons carried by field B+ (t); then, the number operator “measured” by the photodetector is ∗ P± = |z± z± | , N out + (t) = U (t) N (P+ ; t)U (t) , 1 N (P+ ; t) = [Λ11 (t) + Λ10 (t) + Λ01 (t) + Λ00 (t)] 2

(187)

The local oscillator is at disposal of the experimenter and its characteristics are known. So, we can subtract from the output of the counter the known signal 1 2 i 2 t 2 k(s)|f0 (s)|ds in the character2 |f0 (t)| ; this generates a phase factor − 2 0 istic operator. Moreover, we rescale the output of the counter by a factor 2/: this amounts to replace k(s) by 2k(s)/ everywhere in the characteristic functional. At the end, the output current is t 2 ˜ 2 dN+ (s) − |f0 (s)| ds , F (t − s) (188) I(t) = 0 which corresponds to the characteristic operator

t 2i t 2 6 Φt (k) = exp −i k(s)|f0 (s)| ds + k(s)dN (P+ ; s) . 0 0

(189)

In other terms the characteristic operator has the general form discussed in Theorem 2 3.1 with d = 1, hα = 0, b = 0, r(k; t) = 0, c(t) = − |f0 (t)| , S k(t) − 1l = 2ik(t)/ e − 1 P+ . By applying Proposition 3.2, we obtain that the reduced characteristic operator Gt (f ; k) satisfies eq. (135) with generator 1 2iκ/ 2 e −1 S1j fj (t) Kt (f ; κ)[(] = L f (t) [(]−iκ |f0 (t)| (+ R1 + 2 j × ( R1∗ + fi (t)S1i∗ + f0 (t) R1 + S1j fj (t) ( i

j

2 + ( R1∗ + fi (t)S1i∗ f0 (t) + 2 |f0 (t)| ( .

(190)

i

Now, we consider a very intense laser field for the local oscillator: → ∞. In this limit the generator of the reduced characteristic operator becomes 2 Kt (f ; κ)[(] = L f (t) [(] − κ |f0 (t)| (

∗ ∗ S1j fj (t) ( + ( R1 + fi (t)S1i f0 (t) . + iκ f0 (t) R1 + j

(191)

i

By comparing (191) with the general expression (136), we see that the reduced characteristic operator of heterodyne detection is given by a factor corresponding to the measurement of the compatible observables

254

Alberto Barchielli

Q(z1 ⊗ f0 ; t) =

t4

5 f0 (s) dA†1 (s) + f0 (s) dA1 (s) ,

t ≥ 0,

(192)

0

times the expression

2 1 t 2 k(s) |f0 (s)| ds ; exp − 2 0

(193)

this term represents a classical Gaussian noise to be added to the quantum noise intrinsic to the measurement of Q(z1 ⊗ f0 ; t). As we now see, it is possible to eliminate this extra noise. Balanced Heterodyne Detection The noise in the output current can be reduced by the measurement scheme called balanced heterodyne detection [88]. Now two identical photoelectron counters are used for detecting the photons in both the fields B+ (t) and B− (t) and the difference I1 (t) − I2 (t) of the two output currents is measured; the scheme of balanced heterodyne detection is given in Fig. 3. We scale again the final output current by a factor −1 , so that we have 4 5 1 t ˜+ (s) − dN ˜− (s) , F (t − s) dN (194) I(t) = 0 which corresponds to a continual measurement of the commuting operators X (t) =

1 [N (P+ ; t) − N (P− ; t)] .

(195)

O I(t)

output

O

O

O

O

O

O O O O

Photocounter 2 O

O

field

System SH

O

f (t)

O

O

O

O

O

O

O

I2 (t)

/− O

O O O beam output port 2 I1 (t) O rrsplitter r r O r rr O O rrrrr output /o o/ o/ /o /o /o /o /o /o /o /o r/ rO /o /o /o /o /o /o output /o /o /o o/ o/ / Photocounter 1 field port 1 rr O r r O r O rrr r r O rr O local oscillator O O O f0 (t)

Fig. 3. Balanced heterodyne detection


255

Then, the characteristic operator

t k(s) dX (s) exp i 0

has the structure given in Theorem 3.1 with d = 1, c = 0, hα = 0, rt (k) = 0, B α ≡ B = 1 (P+ − P− ), S k(t) − 1l = eik(t)/ − 1 P+ + e−ik(t)/ − 1 P− . Now we construct the reduced characteristic operator in three steps: first we eliminate the field A0 , then we take the limit of a very intense local oscillator → ∞, and finally we eliminate the other fields. By recalling that the field A0 does not interact with the system SH , we can do the first two steps by considering the matrix elements on the coherent vectors: 6 (k)ψ(g 2 ) := ψ(g 1 )Φ t Γ

t

0 / k(s) dX (s) ψ(f0 ) ⊗ ψ(g 2 ) . (196) ψ(f0 ) ⊗ ψ(g 1 ) exp i 0 Γ ⊗Γ

0

Then, by eq. (119) we obtain

4 2 ds 2 |f0 (s)| + g11 (s)g12 (s) 0

5 2 1 × cos k(s)/ − 1 + i f0 (s)g1 (s) + g1 (s)f0 (s) sin k(s)/ . (197)

6t (k)ψ(g 2 ) = ψ(g 1 )|ψ(g 2 ) exp ψ(g )Φ

t

1

In the limit of a strong local oscillator we get 6t (k)ψ(g 2 ) = lim ψ(g 1 )Φ 6t (k)ψ(g 2 ) = ψ(g 1 )|ψ(g 2 ) ψ(g 1 )Φ →∞

t 4 5 2 1 2 ds − k(s) |f0 (s)| + ik(s) f0 (s)g12 (s) + g11 (s)f0 (s) × exp , 2 0 (198) which is the characteristic operator of the observables Q(z1 ⊗ f0 ; t) (192). With the notations of the Theorem 3.1 we have d = 1,

B α = 0,

h (t) ≡ h(t) = f0 (t)z1 , α

c = 0,

b = 0,

St (k) = 1l,

r(k; t) = ik(t)f0 (t)z1 .

(199)

Then, the generator of the reduced characteristic operator becomes 1 2 Kt (f ; κ)[(] = L f (t) [(] − κ2 |f0 (t)| ( 2

∗ ∗ S1j fj (t) ( + ( R1 + fi (t)S1i f0 (t) , + iκ f0 (t) R1 + j

(200)

i

which is the similar to the expression (191), a part from a smaller noise due to the factor 1/2 in the second term.

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Alberto Barchielli

Moments By using h(t) = f0 (t)z1 , we can say that the balanced heterodyne scheme realizes a continual measurement of the compatible quantum observables 5 t 4 zj |h(s) dA†j (s) + h(s)|zj dAj (s) , Q(h; t) = t ≥ 0 ; (201) 0

j

˜ t) the associated stochastic process, the output current of the by denoting by Q(h; balanced heterodyne detection scheme is t ˜ s) . I(t) = F (t − s) dQ(h; (202) 0

The generator of the reduced characteristic operator associated to the process ˜ t) is Q(h; κ2 2 Kt (f ; κ)[(] = L f (t) [(] − h(t) ( + iκ [Z(f ; t)( + (Z(f ; t)∗ ] , 2 ∗ R + (S − 1l)C f (t) + h(t)|f (t). Z(f ; t) = C h(t)

(203) (204) (205)

Typical choices are γ˜ F (t) = k exp − t , 2 ˆ, h(t) = e−iνt h

γ˜ > 0 ,

ˆ ∈Z, h

ˆ (t) = 0 , h|f

ν ∈ R, ∀t .

(206) (207) (208)

These choices give " κ2 " "ˆ "2 Kt (f ; κ)[(] = L f (t) [(] − "h" ( + iκ [Z(f ; t)( + (Z(f ; t)∗ ] , 2 ∗ ˆ Z(f ; t) = eiνt C h R + (S − 1l)C f (t) .

(209) (210)

By changing ν, which means to change the measuring apparatus, the whole spectrum of SH can be explored. The condition (208) means that the light of the laser stimulating SH does not hit the detector directly. The first and second moments turn out to be given by Eρ0

4

5 t ˜ Q(h; t) = ds Ec [TrH {Y (f ; s)ρ(f ; s)}] , 0

(211)


257

t1 ∧t2 4 5 2 ˜ t1 )Q(h; ˜ t2 ) = Eρ0 Q(h; h(t) dt 0 t1 ∨t2 t1 ∧t2 dt ds Ec [TrH {Y (f ; t)Υ (f ; t, s) ◦ Y(f ; s)[ρ(f ; s)]}] + t1 ∧t2 t1 ∧t2

0

+2

t

dt

ds Ec [TrH {Y (f ; t)Υ (f ; t, s) ◦ Y(f ; s)[ρ(f ; s)]}] ,

(212)

Y(f ; t)[(] = Z(f ; t)( + (Z(f ; t)∗ ,

(213)

0

0

where

∗

Y (f ; t) = Z(f ; t) + Z(f ; t) .

(214)

By these equations, the measurement scheme we are discussing here can be interpreted as an imprecise, indirect, continual measurement of the system observables Y (f ; t). Then, for the output current (202) we get t dτ e−˜γ (t−τ )/2 Ec [TrH {Y (f ; τ )ρ(f ; τ )}] , (215) Eρ0 [I(t)] = k 0

t∧s

Eρ0 [I(t)I(s)] = k 0 t∨s dτ1 + k2 2

t∧s

0

e−˜γ (

t+s 2 −τ

) h(τ )2 dτ t∧s τ1 t∧s dτ2 + 2 dτ1 dτ2 e−˜γ (t+s−τ1 −τ2 )/2 0

0

× Ec [TrH {Y (f ; τ1 )Υ (f ; τ1 , τ2 ) ◦ Y(f ; τ2 )[ρ(f ; τ2 )]}] .

(216)

3.6 Physical Models In the next sections we want to present two concrete applications in quantum optics of the whole theory of quantum continual measurements. An interesting phenomenon is the so called shelving effect: a three-level system with a peculiar configuration of permitted transitions and suitably stimulated by lasers exhibits bright and dark periods in its fluorescence light. This phenomenon can have a nice mathematical treatment by using QSC and the theory of continual measurements (direct detection) [16, 20, 42]. Also the simplest quantum system, a two-level atom, presents interesting features. A noteworthy characteristic of its fluorescence spectrum is a three peaked shape in the case of a very intense stimulating laser (Mollow spectrum). Again QSC and the theory of continual measurements give a way of modelling and studying this system [26–28], giving a unified treatment to known results and allowing modifications of the known results by using an Hudson-Parthasarathy equation with S = 1l. It is in this problem that it is used a mixture of coherent states of type S3 as initial state [28].

258

Alberto Barchielli

4 A Three–Level Atom and the Shelving Effect Today experimental techniques allow to observe the fluorescent light emitted by a single atom or ion; therefore, it is possible to observe effects which are completely masked when many emitters are involved. One of these phenomena, the electron shelving effect, was proposed by Dehmelt as a very sensitive scheme for detecting very weak transitions in single ions [45, 46] and it was observed when single ion spectroscopy became feasible [30, 83, 85]. Consider a three–level atom with states |g (ground), |b (blue) and |r (red); assume that the blue transition b ↔ g is very strong and the red one r ↔ g is very weak, while the transition b ↔ r is prohibited. When both transitions are driven by two suitably tuned lasers, we expect the atom to emit blue fluorescent light. But sometimes, when the atom absorbs a red photon, the electron goes into the red state, which has a long lifetime (a fraction of a second), and the fluorescence light stops until the red state decays. Thus we expect to observe bright and dark periods, randomly distributed. In a pictorial language, we say that during a dark period the electron is ‘shelved’ in the red state. The energy–level scheme we have described, when indeed |g is the lowest state, is called the V configuration and it is given in Fig. 4; the simple arrows represent spontaneous decay and the double arrows represent absorption/stimulated emission. The same considerations apply to the so called Λ configuration when |g is the highest state (Fig. 4). Usually the electron jumps between the |g and the |b states emitting blue light, but sometimes the |g state decays into the |r one and it stays ‘shelved’ there until it absorbs a red photon. A more realistic model could be obtained by adding a weak |b ↔ |r transition [91]. However, this discussion is of a semi-classical character and does not takes into account that the atom-field interaction gives rise to quantum coherent superpositions of the atomic states. So, to explain the shelving effect we need a full quantum mechanical treatment. A first good quantum–mechanical explanation of this effect was given in [39]. |b≡|1

22 Y222 22 22 22 22 22 22 22 22 22 22 22 22 22 22 22 22 22 22 22 22 2

|r≡|2

@

|g≡|0

Fig. 4. Energy–level scheme for the V configuration.


259

|g≡|0

>^ > E >>> >>> >> >> >> >> >> >> >> >> >> >> >> > > |r≡|2 |b≡|1

Fig. 5. Energy–level scheme for the Λ configuration.

4.1 The Atom–Field Dynamics Let us concretize the previous discussion in the choice of the operators H, R, S appearing in the Hudson-Parthasarathy equation (39) and of the photon space Z; this choice fixes the atom-field dynamics. We denote by |j, j = 0, 1, 2 the three states: |g ≡ |0, |b ≡ |1, |r ≡ |2. The level scheme of Figs. 4 and 5 implies that the free atomic Hamiltonian is 1 2 ωj > 0 in the V-configuration, ωj |jj| , (217) H= ωj < 0 in the Λ-configuration. j=1 Moreover, we consider the simplest case: only the absorption/emission process is relevant and there is not direct scattering; so we take S = 1l .

(218)

According to the discussion on the quasi–monochromatic approximation of Section 2.5 we need a different field for any possible atomic transition, if well separated. We have two well separated transitions, the g ↔ b one and the g ↔ r one; so, we take: Z = Z 1 ⊕ Z 2 . Then, in the rotating wave–approximation, the operator R must give the two possible decays with emission of blue photons (in Z 1 ) and red photons (in Z 2 ); this implies 1 |0 ⊗ αj j| in the V-configuration, 1 2 j R=R +R , R = (219) |j ⊗ αj 0| in the Λ-configuration, αj ∈ Z j ,

" "2 γj := "αj " > 0 .

(220)

The two following quantities constructed from R appear in the master equation (74): 1 2 in the V-configuration, j=1 γj |jj| R∗ R = (221) (γ1 + γ2 )|00| in the Λ-configuration,

260

Alberto Barchielli

12 ∗

TrZ {R(R } =

γj j|(|j |00| 2 0|(|0 j=1 γj |jj|

in the V-configuration,

j=1

(222)

in the Λ-configuration,

Pure Decay In order to understand better the meaning of the various quantities appearing in the atom–field dynamics, let us start with the case of the atom not stimulated in any way; this correspond to the choice S1 for the state: the initial field is in the Fock vacuum (f ≡ 0). By eqs. (69), (70) we have ρ(t) = ρ(0; t) and this state satisfies the master equation (76). This equation can be easily written in our case and solved; the final result is: 1. In the case of the V-configuration: i, j = 1, 2, j|ρ(0; t)|i = exp − 12 (γi + γj ) t + i (ωi − ωj ) t j|ρ0 |i, j|ρ(0; t)|0 = 0|ρ(0; t)|j = exp − 12 γj t − iωj t j|ρ0 |0, 0|ρ(0; t)|0 = 1 −

2

e−γj t j|ρ0 |j.

(223a) (223b) (223c)

j=1

2. In the case of the Λ-configuration: i, j = 1, 2, (224a) 0|ρ(0; t)|0 = e−(γ1 +γ2 )t 0|ρ0 |0, 1 j|ρ(0; t)|0 = 0|ρ(0; t)|j = exp − 2 (γ1 + γ2 ) t − iωj t j|ρ0 |0, (224b) γ j 1 − e−(γ1 +γ2 )t 0|ρ0 |0. j|ρ(0; t)|i = ei(ωi −ωj )t j|ρ0 |i + δij γ1 + γ2 (224c) These equations confirm that ω1 , ω2 are the atomic frequencies and show that γ1 , γ2 are the spontaneous emission rates. The assumption of a weak red transition and a strong blue one gives γ1 ( γ2 > 0. Stimulating Lasers Let us consider now the case of interest, when we have two lasers stimulating the blue and the red transitions. This is the case of a state of type S2, with the field in a coherent state with f of the form f (t) = 1l[0,T ] (t)

2

e−iνj t λj ,

νj > 0 ,

λj ∈ Z j .

(225)

j=1

In all the following formulae we take T → +∞. By eqs. (69), (70), we have ρ(t) ≡ ρ(f ; t); this reduced state satisfies the master equation (74), with Liouvillian (75)


1 ∗ 1 ∗ R R + iH f (t) ( − ( R R − iH f (t) L f (t) [(] = − 2 2

261

+ TrZ {R(R∗ } ,

(226)

∗ H f (t) = H + iC f (t) R − iR∗ C f (t) 2 2 3 j j ωj |jj| + ieiνj t λj |αj σ− , − ie−iνj t αj |λj σ+ =

(227)

where (cf eq. (73c))

j=1 j σ− := |0j| ,

j σ+ := |j0| ,


j σ−

j σ+

in the Λ-configuration.

:= |j0| ,

:= |0j| ,

(228)

The explicit time dependence due to the lasers can be removed; in the physical parlance one says that the rotating frame is used. Let us set 1 +1 in the V-configuration, := (229) −1 in the Λ-configuration, ∆j := νj − |ωj | ,

Ωj := 2 αj |λj ,

βj := arg −iαj |λj ; (230)

note that one has

i iβj e Ωj . (231) 2 The ∆j are called the detuning parameters and the Ωj are called Rabi frequencies. To have a strong blue transition, strongly stimulated, and a weak red one we assume: αj |λj =

γ1 ( γ2 > 0 , γ1 ( Ω2 ,

Ω1 ( Ω 2 > 0 , Ω12 ( γ1 γ2 .

(232)

The approximation of taking two field types, one interacting with the blue transition and one with the red one, is reasonable only if the two lasers are not too much out of resonance; moreover, we want the two transitions to be not overdamped. These two conditions give the further assumptions |∆j | 2γj ,

2Ωj > γj ,

j = 1, 2.

(233)

Then, the new reduced state

2 2 νj |jj| ρ(t) exp −it νj |jj| ρ˜(t) := exp it j=1

(234)

j=1

satisfies the master equation d ρ˜(t) = L∆ [˜ ρ(t)] , dt

(235)

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Alberto Barchielli

where

L∆ [(] := K( + (K ∗ + TrZ {R(R∗ } , 2 Ωj iβj 1 ∗ −iβj e |j0| + e K := − R R − i |0j| − ∆j |jj| . 2 2 j=1

(236) (237)

4.2 The Detection Process Now we assume to have a detector able to count photons flying through a solid angle Sd not containing the direction of propagation of the lasers, so that the lasers do not send light directly to the counter and only fluorescence light is detected; the efficiency of the counter can be taken into account by choosing Sd smaller than the geometrical solid angle spanned by the detector. We can formalize this setup by saying that the detector performs a continual measurement of the observable N (P ; t) defined by eq. (85) with 1. P λj = 0, j = 1, 2: the laser light does not impinge directly on the detector; 2. P Z j ⊂ Z j , j = 1, 2: the detector does not mix up blue and red photons. Let us set

" "2 ηj := "P αj " ;

(238)

by their definitions, we have 0 ≤ ηj ≤ γj . We assume that “many” blue photons are detected, so we have (239) 0 ≤ η2 ≤ γ2 Lη1 ≤ γ1 . The whole information on the counting probabilities is contained in the characteristic functional (129), (185) or in the probabilities of no counts (183a) and the exclusive probability densities (183b). To compute these probabilities we need to particularize to our case the quantities of eqs. (167); we get Y(f ; t)[(] = TrZ {(1l ⊗ P ) R(R∗ } =: Y[(] , L˜ f (t) = L f (t) − Y

(240a) (240b)

From the expression of the probabilities (183a), (183b) we see that we can make everywhere the transformation (234) without changing such probabilities. This simply means that everywhere we have to make the substitutions L f (t) → L∆ and L˜ f (t) → L˜∆ , where L˜∆ := L∆ − Y . (241) In this way we get

2 3 ˜ Pt (0|ρ0 ) = TrH eL∆ t [ρ0 ]

(242)

for the probability of no counts up to time t and 2 ˜ ˜ pt (tm , tm−1 , . . . , t1 |ρ0 ) = TrH eL∆ (t−tm ) ◦ Y ◦ eL∆ (tm −tm−1 )

3 ˜ ˜ ◦ Y ◦ · · · ◦ eL∆ (t2 −t1 ) ◦ Y ◦ eL∆ t1 [ρ0 ]

for the exclusive probability densities.

(243)


263

More concretely we have L˜∆ [(] = K( + (K ∗ 12 (γ − η ) j|(|j |00| j j j=1 + 2 0|(|0 j=1 (γj − ηj ) |jj|

in the Λ-configuration,

2 i Ωj eiβj |j0| + e−iβj |0j| 2 j=1 1 γj 2 j=1 i∆j − 2 |jj| + 2 2 −i j=1 ∆j |jj| − γ1 +γ |00| 2

in the V-configuration, in the Λ-configuration,

K=−

1 2 κ(() := ρjump


Y[(] = κ(()ρjump ,

j=1 ηj j|(|j (η1 + η2 ) 0|(|0

1 |00| := 2

ηj j=1 η1 +η2

|jj|

(244)

(245)

(246a)

in the V-configuration, in the Λ-configuration, in the V-configuration, in the Λ-configuration.

By inserting these expressions into eq. (243) and setting ˜ ˜ w0 (t) := κ eL∆ t [ρ0 ] , w(t) := κ eL∆ t [ρjump ] ,

(246b) (246c)

(247)

we obtain pt (tm , . . . , t1 |ρ0 ) = Pt−tm (0|ρjump ) w(tm − tm−1 ) · · · w(t2 − t1 ) w0 (t1 ) . (248) Moreover, one can check immediately that d ˜ Pt (0|() = −κ eL∆ t [(] dt

(249)

and, then, one has Pt (0|ρjump ) = 1 −

t

w(s)ds , 0

Pt (0|ρ0 ) = 1 −

t

w0 (s)ds .

(250)

0

These equations say that our detection process is a delayed renewal counting process (an usual renewal counting process when w0 (t) ≡ w(t)); w(t) is the interarrival +∞ waiting–time density. By construction 0 w(t) dt ≤ 1, but it is possible to have +∞ w(t) dt < 1: this means that there is a non–zero probability that the detected 0 fluorescence stops.

264

Alberto Barchielli

Note that the probability density w(t) of the interarrival times is a continuous function and that w(0) = 0; this says that just after a count the atom cannot emit, but it needs some time to be excited again: this is the so called antibunching effect. From now on we assume that all the fluorescence photons are detected; we can think to have an array of perfect detectors spanning the whole solid angle around the atom, with the exception of a small angle containing the direction of propagation of the lasers. In other terms we give the process which counts all the emitted photons. Mathematically this amounts in taking P = 1l

ηj = γj ,

or

j = 1, 2 .

(251)

This simplifies all the computations, because we get L˜∆ [(] = K( + (K ∗ ,

t

Pt (0|ρjump ) = 1 − 0

t

Pt (0|ρ0 ) = 1 −

∗

˜

eL∆ t [(] = eKt (eK t ,

(252)

2 3 ∗ w(s)ds = Tr eKt ρjump eK t ,

(253a)

3 2 ∗ w0 (s)ds = Tr eKt ρ0 eK t .

(253b)

0

As far as many blue photons are detected and (239) holds, the assumption (251) should not alter the statistical properties of the counting process in an essential way. 4.3 Bright and Dark Periods: The V-Configuration As we have seen, all the probabilities depend on the waiting time densities w0 (t) and w(t). By particularizing eqs. (245)–(247) to the V case, we get K=

2 j=1

iβj i γj −iβj i∆j − |jj| − Ωj e |j0| + e |0j| , 2 2 κ(() =

2

γj j|(|j,

ρjump = |00|,

(254)

(255)

j=1

w0 (t) =

2

0 / ∗ γj j eKt ρ0 eK t j ,

(256a)

2 γj j eKt 0 .

(256b)

j=1

w(t) =

2 j=1

To obtain the expression of the interarrival time density w(t), we have to compute eKt |0. By setting


aj (t) := e−iβj j|eKt |0 ,

a0 (t) := 0|eKt |0 , we can write

w(t) =

2

j = 1, 2 ,

2

γj |aj (t)| ,

265

(257)

(258)

j=1

Pt (0|ρjump ) = 1 −

t

w(s)ds = 0

2

2

|aj (t)| .

(259)

j=0

By taking the time derivative, we get the system of linear differential equations ⎛ ⎞ 1 d a(t) = G a(t) , a(0) = ⎝0⎠ , (260) dt 0 ⎛

⎞ 0 −iΩ1 /2 −iΩ2 /2 0 ⎠, G := ⎝−iΩ1 /2 −ξ1 /2 0 −ξ2 /2 −iΩ2 /2

where

ξj := γj − 2i∆j ,

j = 1, 2 .

(261) (262)

The solution of the system (260) can be obtained by Laplace transform; we get (z0 + ξ1 /2)(z0 + ξ2 /2) z0 t e (z0 − z1 )(z0 − z2 ) (z1 + ξ1 /2)(z1 + ξ2 /2) z1 t (z2 + ξ1 /2)(z2 + ξ2 /2) z2 t e + e , (263a) + (z1 − z0 )(z1 − z2 ) (z2 − z0 )(z2 − z1 )

a0 (t) =

a1 (t) = −

iΩ1 2

a2 (t) = −

iΩ2 2

z0 + ξ2 /2 ez0 t (z0 − z1 )(z0 − z2 ) z1 + ξ2 /2 z2 + ξ2 /2 ez1 t + ez2 t , (263b) + (z1 − z0 )(z1 − z2 ) (z2 − z0 )(z2 − z1 )

z0 + ξ1 /2 ez0 t (z0 − z1 )(z0 − z2 ) z1 + ξ1 /2 z2 + ξ1 /2 ez1 t + ez2 t , (263c) + (z1 − z0 )(z1 − z2 ) (z2 − z0 )(z2 − z1 )

where z0 , z1 , z2 are the roots (which we have assumed to be all distinct) of the characteristic polynomial of the matrix G: z3 +

1 2 1 1 2 (ξ1 + ξ2 ) z 2 + Ω1 + Ω22 + ξ1 ξ2 z + Ω1 ξ2 + Ω22 ξ1 = 0 . (264) 2 4 8

266

Alberto Barchielli

By exploiting the assumptions (232) and (233), we can find an approximate expression for the three roots of this equation: Ω 2 ξ1 ξ2 − 2 2 2 2Ω1 2Ω12 2Ω12 + Ω22 − ξ12 Ω12 + Ω22 ξ1 Ω22 $ z1 − , 1− 2 +i 4 Ω1 Ω12 4Ω12 − ξ12 2Ω12 2Ω12 + Ω22 − ξ12 Ω12 + Ω22 ξ1 Ω22 $ . z2 − 1− 2 −i 4 Ω1 Ω12 4Ω12 − ξ12 Note that one has Re 4Ω12 − ξ12 = 4Ω12 − γ12 + 4∆12 > 0 and z0 −

(265a) (265b) (265c)

0 > Re z0 ( max {Re z1 , Re z2 } .

(266)

We can see that, for the values of interest of the parameters, the three roots are indeed distinct and with strictly negative real parts. Using this in eq. (259), we get

+∞

lim Pt (0|ρjump ) = 0 ,

w(s)ds = 1 .

t→+∞

(267)

0

Similar considerations apply to Pt (0|ρ0 ) and w0 (t). This implies that the fluorescence light never stops definitively. By (258), (263), many decay times appear in the expression of w(t); by (266), the longest one is (−2 Re z0 )−1 , while the others, (− Re z0 −Re zj )−1 , (− Re zi − Re zj )−1 , i, j = 1, 2 are much shorter; so, w(t) has a small long living tail. Indeed, by (258) and (263), we can write w(t) = wshort (t) + Π2 |Re z0 | e2 Re z0 t ,

(268)

where in wshort (t) we have grouped all the terms with a short decay time and 2

Π :=

γ1 Ω12 |z0 + ξ2 /2| + γ2 Ω22 |z0 + ξ1 /2| 2

2

8 |z0 − z1 | |z0 − z2 | |Re z0 |

2

;

(269)

moreover, the conditions (232) give Π 0 ,

(292)

where the atomic frequency ω0 must already include the Lamb shift. The Photon Space In the approximations we are considering [18, 89], the fields behave as monodimensional waves, so that a change of position is equivalent to a change of time and viceversa. Then, the space Z has to contain only the degrees of freedom linked to the direction of propagation and to the polarization. To describe a spin-1 0-mass particle we use the conventions of Messiah [79] pp. 550, 1032–1037. The space Z is spanned by the c.o.n.s. ! jm |j, m; ) ≡ Θ ,

j = 1, 2, . . . ,

m = −j, −j + 1, . . . , j,

) = ±1 ;


271

jm is the total angular momentum, ) = +1 denotes the electrical multipoles, ) = −1 denotes the magnetic multipoles and (−1)j ) is the parity. By using the spherical harmonics Ylm (θ, φ) and the orbital angular momentum operator , one has Yjm , −1 = $ 1 Θ jm j(j + 1)

+1 = i −1 , Θ p×Θ jm jm

(293)

where p is the direction versor given by p1 = sin θ cos φ ,

p2 = sin θ sin φ ,

p3 = cos θ .

(294)

The Interaction Let us consider now the terms with the creation and annihilation operators in the dynamical equation (39); they must describe the absorption/emission process. By asking spherical symmetry, parity conservation and only electrical dipole contribution in R, we must have R=α

F+

|+ ; F− ; 1; F+ , M F+ , M |,

α ∈ C,

α = 0 ,

(295)

M =−F+

|+ ; F− ; 1; F+ , M F−

=

1

|F− , m1 ⊗ |1, m2 ; +1F− , m1 ; 1, m2 |F+ , M ,

(296)

m1 =−F− m2 =−1

where by F− , m1 ; 1, m2 |F+ , M we denote the Clebsch-Gordan coefficients ([79] pp. 560–563). The interaction terms containing R are responsible for the spontaneous decay of the atom and, as we shall see, |α|2 turns out to be the natural line width. By eqs. (37) and (291) we have Rk = α

1

zk |1, m; +1Qm ,

(297)

m=−1

Qm =

F−

|F− , m1 F− , m1 ; 1, m|F+ , m1 + mF+ , m1 + m|,

(298)

m1 =−F−

R∗ R = |α|2 P+ ,

R k = P− R k P+ ,

Rk ρRk∗ = |α|

k

K−

1

(299)

Qm ρQ∗m ,

(300)

2 i |α| ω0 1l = − iω0 + P+ . 2 2

(301)

2

m=−1

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Alberto Barchielli

The interaction term containing the Λ-process must give the residual scattering when the atom is frozen in the up or down level, so we take the unitary operator S of the form S ± ∈ U(Z) . (302) S = P+ ⊗ S + + P − ⊗ S − , Then, by spherical symmetry and parity conservation we must have S± =

j ∞

|j, m; ) exp{2iδ± (j; ))}j, m; )|,

(303)

j=1 m=−j !=±1

0 ≤ δ± (j; )) < 2π. The unitary operators S + and S − represent the scattering operators for a photon impinging on the atom frozen in the up or in the down state; the δ’s are the phase shifts for these scattering processes. Quantities like ω0 , α, δ± (j; )) are phenomenological parameters, or, better, they have to be computed from some more fundamental theory, such as some approximation to quantum electrodynamics. Summarizing, the possible processes are: absorption, through the term containing R∗ , emission, through R, photon scattering with the atom in the up level, through P+ ⊗ S + , photon scattering with the atom in the down level, through P− ⊗ S − . An illustration of these processes is given in Fig. 6. The Balance Equation for the Number of Photons Let us introduce the observables, which we have already considered in Section 3.1 eqs. (85) and (96), “total number of photons in the time interval [0, t]” before and after the interaction with the atom, in (t) := N (1l; t) = Λkk (t) , Ntot (304) k out out ∗ in Ntot (t) := N (1l; t) = U (t) Ntot (t)U (t) . By eq. (96) we obtain in the present model the balance equation in (t) + Ntot

1 1 out (P+ − P− ) = Ntot (t) + U (t)∗ (P+ − P− )U (t) . 2 2

(305)

w7 7 'g 'g P+ ⊗S + w7 7w g' g' 7 w w7 g' g' g' g' w7 w7 7w 'O g' g' 'g 'g R∗ 'g g' g' g' 'g 'g g' g' g' g' g' g' R '7 \ ' w 7 ' g 7w g' g' w 7 7w g' 'g 7w 7w 'g g' − 7w 7w g' ' P− ⊗S Fig. 6. The dynamical processes: absorption, emission and direct photon scattering


273

Such an equation has a very important meaning: it says that the number of photons entering the system up to time t plus the photons stored in the atom at time 0 is equal to the number of photons leaving the system up to time t plus the photons stored in the atom at time t. The Phase Diffusion Model for the Laser In [68, 75] a laser model is considered which, translated in our setup, amounts in taking as the state of the laser a mixture of coherent vectors of the type S3, (65). Therefore, the initial state is taken to be s = ρ0 ⊗ Ec η(f ) , ρ0 ∈ S(H) , (306) f (t) = e−i(ωt+

√ B W (t))

λ∈Z,

1(0,T ) (t) λ ,

ω > 0,

B ≥ 0,

(307)

W (t) is a real standard Wiener process canonically realized in the Wiener probability space (Ω c , F c , P c ) (S3’); T is a large time and T → +∞ in the final results is always understood. This is the simplest model for a laser which is not perfectly monochromatic nor perfectly coherent. Only the phase fluctuates, not the intensity; moreover, the laser spectrum has a Lorentzian shape with bandwidth B: ω 2π

+∞

−∞

eiντ Ec [f (t)|f (t + τ )] dτ = ωλ2

B/(2π) ; (ν − ω)2 + B 2 /4

(308)

ωλ2 is the power of the laser. The whole model is meaningful only for ω not too “far” from ω0 . In some experiments the laser light is taken to be circularly polarized, because in this way, in the long run, only two states are involved in the dynamics ([60] p. 206) and the usual theory has been developed for systems with only two states [68, 81]. Let the incoming light have right circular polarization and propagate along the z axis; then, the electromagnetic selection rules imply that the atomic transitions which survive are: spontaneous emission with ∆M = 0, ±1, stimulated emission with ∆M = −1, absorption with ∆M = 1; the situation is summarized in the Fig. 7. M =−2

M =−1

M =0

M =1

M =−1

M =0

M =1

88 88 C 88 88 88 88 88 8 88 888 88 88 88 88

M =2

88 C C 88 88 88 8 8 888 8

Fig. 7. Allowed atomic transitions (case F+ = 2, F− = 1)

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Alberto Barchielli

In order to describe a well collimated laser beam propagating along the direction z (θ = 0) and with right circular polarization, we take λ = αΩ eiδ λ+ , λ+ (θ, φ) =

∆θ

$

Ω > 0,

1[0,∆θ] (θ)

3π(1 − cos ∆θ)

δ ∈ [0, 2π) 1 i + ij ; −√ 2

(309) (310)

in all the physical quantities the limit ∆θ ↓ 0 will be taken. Note that the power of the laser ωλ2 = 23 ω|α|2 Ω 2 /(∆θ)2 diverges for ∆θ ↓ 0, because we need a not vanishing atom-field interaction in the limit. In the following we shall need the relation 2j + 1 δm,1 . j, m; )|λ+ = −) (311) 12 5.2 The Master Equation and the Equilibrium State Let us start by considering the (not averaged) reduced statistical operator ρ(f ; t) = TrΓ {U (t) (ρ0 ⊗ η(f )) U (t)∗ } (70), which satisfies the master equation (72) or (74); the time-dependent Liouvillian (73) turns out to be L f (t) [(] = −i H f (t) , ( ∞ ∗ 5 4 ∗ 5 1 4 Rk f (t) (, Rk f (t) + Rk f (t) , (Rk f (t) , + 2

(312)

k=1

1 Rk f (t) = α zk |1, m; +1Qm + zk |(S − 1l)f (t)P , m=−1

(313)

=±

1 ω0 − Im f (t) S + − S − f (t) (P+ − P− ) H f (t) = 2 1 i 4 α 1 + e−2iδ− (1;+1) f (t)|1, m; +1Qm + 2 m=−1 5 − α 1 + e2iδ− (1;+1) 1, m; +1|f (t)Q∗m .

(314)

We see that the transitions between the two levels are due to the presence of the operators Qm (298); more precisely, the transitions from the up to the down level are due to the presence of Qm on the left of ( and of Q∗m on the right (emission), while Q∗m on the left and Qm on the right give the transitions from the down to the up level (absorption). The fact that the operators Rk f (t) contain a sum of terms proportional to Qm and of terms proportional to P± is an indication of an interference effect between absorption/emission and direct scattering.


275

Note that, when the field is in the Fock vacuum, only spontaneous emission is present; indeed, for f (t) = 0, the Liouvillian (312) reduces to L(0)[(] = −iω0 [P+ , (] −

1 1 2 |α| (P+ ( + (P+ ) + |α|2 Qm (Q∗m , 2 m=−1

(315)

which describes the atomic decay according to the usual selection rules for electric dipole and fixes the meaning of |α|2 as spontaneous decay rate or natural line width. By inserting the expression (307), (309), (310) of f (t) into eqs. (313), (314) we get √ (316) Rk f (t) = e−i ωt+ B W (t) UW (t)∗ D(zk )UW (t) , ˜ W (t) + 1 ω (P+ − P− ) , (317) H f (t) = UW (t)∗ HU 2

4

5 √ i ωt + B W (t) (P+ − P− ) , (318) UW (t) := exp 2 D(h) := α

1

h|1, m; +1Qm + αΩeiδ

m=−1

h| (S − 1l) λ+ P ,

=±

(319)

h∈Z, 4 5 ˜ = 1 ω0 − ω − |α|2 Ω 2 Imλ+ | S + − S − λ+ (P+ − P− ) H 2 (320) 5 4 i 2 + |α| Ω eiδ 1 + e2iδ− (1;+1) Q∗1 − e−iδ 1 + e−2iδ− (1;+1) Q1 . 4 This result suggests to consider the random atomic state in the “rotating frame” ρ˜(f ; t) := UW (t)ρ(f ; t)UW (t)∗ .

(321)

By classical stochastic calculus we obtain the stochastic equations of Ito type √ i 1 dUW (t) = ωdt + B dW (t) (P+ − P− ) − Bdt UW (t) (322) 2 8 and d˜ ρ(f ; t) =

i√ B [P+ − P− , ρ˜(f ; t)] dW (t) + L˜B [˜ ρ(f ; t)] dt , 2

(323)

where B L˜B [(] := ([(P+ − P− ) (, P+ − P− ] + [P+ − P− , ( (P+ − P− )]) 8 5 4 ˜ ,( + 1 −i H ([D(zk )( , D(zk )∗ ] + [D(zk ) , (D(zk )∗ ]) . (324) 2 k 3 2 The quantum dynamical semigroup exp L˜B t will be one of the main ingredients in the computations of the fluorescence spectrum; therefore, we need to study its properties and, in particular, its equilibrium state.

276

Alberto Barchielli

The Parameters

x, y, z γ

First of all we need to summarize all the parameters which enter the model and to introduce some shorthand notations. We already started to give all quantities in units of the natural linewidth |α|2 ; for instance, we wrote λ = αΩ eiδ λ+ in (309), so that Ω 2 becomes an adimensional measure of the laser intensity. Then, we define x :=

ν − ω0 , |α|2

y := B/|α|2 , z := (ω − ω0 ) /|α| , γ˜ , γ := |α|2 2

q

z˜

ε, P⊥

δ± , s, g± ∆g, b, Γ 2

reduced frequency,

(325a)

reduced laser bandwidth,

(325b)

reduced detuning,

(325c)

reduced instrumental width,

(325d)

It is also useful to introduce the shorthand notation γ+y q := + i(x − z) 2

(326)

and the shifted detuning parameter z˜ := z − Ω 2 ε ,

(327)

ε := ImS + λ+ |P⊥ S − λ+ , P⊥ := 1l − |1, 1; +11, 1; +1| ;

(328) (329)

where

here Ω 2 ε plays the role of an intensity dependent light shift. It is also useful to define δ± := δ± (1; +1) , s := δ+ − δ− , (330) ± g± := P⊥ S − 1l λ+ , ∆g := g+ − g− , (331) 1 1 1 + y + Ω 2 ∆g2 + sin2 s − i z˜ + Ω 2 sin 2s , (332) b := 2 4 2 2 2 Γ 2 := 1 + y + Ω 2 ∆g + Ω 2 2 + 2y + 2Ω 2 ∆g + Ω 2 sin2 s . (333) We have to ask |ε| < +∞, g± < +∞, for ∆θ ↓ 0; roughly speaking, S ± must introduce small corrections even when the norm of λ+ diverges. The Equilibrium State By inserting the explicit expressions of all the quantities appearing in the timeindependent Liouvillian (324) and by using the shorthand notations just introduced, after some computations we obtain

Quantum Continual Measurements −2

|α|

L˜B [(] = −P+ (P+ − bP+ (P− − bP− (P+ +

1

277

Qm (Q∗m

m=−1

5 1 4 + Ω ei(δ+2δ− ) Q∗1 ( + e−i(δ+2δ− ) (Q1 2 5 1 4 i(δ+2δ ) − Ω P (Q∗1 + e−i(δ+2δ ) Q1 (P . e 2 =±

(334)

2 3 2 ˜ has a unique For |α| > 0, Ω > 0, the quantum dynamical semigroup exp Lt equilibrium state with support2 in the 3 linear span of |F+ , F+ , |F− , F− : for any ˜ initial state ρ0 , limt→+∞ exp LB t [ρ0 ] = ρ∞ . We skip proofs and computations and give the final expression for ρ∞ : F+ , F+ |ρ∞ |F+ , F+ = Ω 2 Re d ,

F− , F− |ρ∞ |F− , F− = 1 − Ω 2 Re d , (335a)

F+ , F+ |ρ∞ |F− , F− = F− , F− |ρ∞ |F+ , F+ = Ω exp [i (δ + 2δ− )] d , (335b) 1 + y + Ω 2 ∆g2 + sin2 s + i 2˜ z − Ω 2 sin s cos s . (335c) d= 4˜ z2 + Γ 2 5.3 The Detection Scheme Heterodyne Detection The spectrum of our two-level atom can be scanned by using the balanced heterodyne scheme (Sect. 3.5 and Fig. 3). We take a monochromatic laser of frequency ν as local oscillator and consider a measuring apparatus which spans a small solid angle with the vertex in the atom and not containing the forward direction in order that the light of the stimulating laser does not hit directly the apparatus. This means that we are in the case of eqs. (201)–(216). The measurement scheme produces an output current t

ˆ t) = k I(ν, h;

ˆ s) , ˜ h; e−˜γ (t−s)/2 dQ(ν,

(336)

0

ˆ s) is the stochastic process associated to the compatible quantum ˜ h; where Q(ν, observables 5 t 4 ˆ ˆ dA† (s) + eiνs h|z ˆ j dAj (s) , e−iνs zj |h Q(ν, h; t) = (337) j j

0

ν ∈ R is the frequency of the local oscillator, γ ! > 0 is an instrumental width, ˆ ∈ Z, h ˆ = 1. Any information on the k = 0 is a proportionality constant and h ˆ We assume that localization and on the polarization of the detector is contained in h. ˆ is given by the detector spans a small solid angle, so that h

ρ∞

278

Alberto Barchielli

(θ , φ ) ˆ , φ ) = 1Ξ$ e(θ , φ ), h(θ |Ξ|

(338)

where Ξ is a small solid angle around the direction (θ, φ), Ξ ↓ {(θ, φ)}, |Ξ| sin θ dθ dφ and e is a complex polarization vector, |e(θ , φ )| = 1. Moreover, we assume that the transmitted wave does not reach the detector, i.e. Ξ and the laser solid angle of (310) are disjoint: Ξ ∩ {θ ∈ [0, ∆θ], φ ∈ [0, 2π)} = ∅; in the limit of infinitesimal angles we have simply that Ξ is a small solid angle around the direction (θ, φ) with θ > 0. In particular this gives ˆ + = 0 . h|λ

(339)

Then, the generator (209) of the characteristic operator associated to the process ˆ s) becomes ˜ h; Q(ν, κ2 Kt (f ; κ)[(] = L f (t) [(] − ( + iκ [Z(f ; t)( + (Z(f ; t)∗ ] , (340) 2 where, by eqs. (143), (147), L f (t) is the generator of the dynamics Υ (f ; t, s) and is given by eqs. (312)–(314), while Z(f ; t) is given by eq. (210), which now becomes

1 iνt ˆ ˆ Z(f ; t) = e h|1, m; +1Qm + h|(S − 1l)f (t)P . (341) α m=−1

=±

By using the explicit expression (307) of f (t) and the stochastic unitary operators UW (t) (318) we get 2 4 53 √ ˆ W (t) , Z(f ; t) = exp −i (ω − ν) t + BW (t) UW (t)∗ D(h)U (342) where D(·) is defined in eq. (319). By defining Υ˜ (t, s)[(] := UW (t)Υ (f ; t, s) [UW (s)∗ (UW (s)] UW (t)∗ ,

(343)

eqs. (321), (323) give dΥ˜ (t, s)[(] =

4 5 5 i√ 4 B P+ − P− , Υ˜ (t, s)[(] dW (t) + L˜B Υ˜ (t, s)[(] dt , (344) 2

with L˜B given by eq. (324). The Power Spectrum As the power of a current is proportional to the square of the current itself, the expression T 4 5 ˆ = lim k1 ˆ t)2 dt P (ν, h) Eρ0 I(ν, h; (345) T →+∞ T 0


279

is the mean output power in the long run; k1 > 0 is a suitable constat with the dimensions of a resistance, it is independent of ν, but it can depend on the other features ˆ gives the power spectrum obof the detection apparatus. As a function of ν, P (ν, h) ˆ in the case of the choice (338) it is the spectrum observed served in the “channel h”; around the direction (θ, φ) and with polarization e. Let us pospone the computations of the mean power and let us start by giving and discussing its final expression: ˆ = P (ν, h)

ˆ = Σ(ν; h)

1 2π

+∞

4πk2 k1 k2 k1 ˆ , + Σ(ν; h) γ˜ γ˜

(346)

2 4 53 γ +B)/2+i(ν−ω)]t ˆ ∗ eK1 t D(h)ρ ˆ ∞ dt e−[(! Tr D(h)

0

+ c.c., (347) K1 [(] = L˜B [(] − BP+ (P− + BP− (P+ ,

(348)

c.c. means “complex conjugated”. 9 – The term k2 k1 γ˜ is independent of ν and, for this reason, can be seen as a white noise contribution to the power spectrum. It is due to the detection scheme, but it cannot be eliminated; its origin can be traced to the canonical commutation relations of the fields and, so, it is of a quantum origin. It is known as shot noise. ˆ is positive because it is the expectation of the square – The mean power P (ν, h) ˆ is positive. Therefore, of a real quantity, but it can be shown that also Σ(ν; h) ˆ Σ(ν; h) can be separated from the shot noise and can be interpreted as the fluˆ To prove the positivity of Σ(ν; h) ˆ one orescence spectrum in the channel h. needs to go back to expressions in which the quantum fields appear explicitly; see Section 3.1.3 of [28]. – The normalization of Σ(ν; h) in (346) has been chosen in such a way that

+∞

−∞

3 2 ˆ dν = Tr D(h) ˆ ∗ D(h)ρ ˆ ∞ , Σ(ν; h)

(349)

With this choice, the total strength of the spectrum is the asymptotic rate of ˆ indeed, we have emission of photons in the “channel h”;

+∞

−∞

1 TrH⊗Γ N out (Phˆ ; T )s , T →+∞ T

ˆ dν = lim Σ(ν; h)

(350)

ˆ Also for this result we refer to where Phˆ is the orthogonal projection on h. Section 3.1.3 of [28]. – The state ρ∞ is the unique equilibrium state of the quantum dynamical semigroup exp(L˜B t) and it is given in eqs. (335).

280

Alberto Barchielli

– In quantum optics it is often stated that the emission spectrum is the Fourier transform of the two-times quantum correlation function of the dipole operator. This is indeed the structure appearing in eq. (347) if we interprete the operator D(·), defined in eq. (319), as an effective dipole operator. This is reasonable because a dipole operator has to take into account not only the two levels remained in the description, but also the full structure of the atom and the operator S − 1l is indeed a track of this structure. Let us note that the effective dipole operator appears also in the Liouvillian L˜B and, so it contributes to the spectrum also through ρ∞ and K1 . – The semigroup exp[K1 t] is trace preserving, but not positivity preserving, while L˜B is a bona-fide Liouvillian, because it can be written in the Lindblad form; this peculiar structure of the quantum correlation function appearing in (347), while not explicitly formulated, was already found in [68]. By putting in evidence the terms with B we can write K1 [(] −

B B B ( = L˜0 [(] − P+ (P+ − P− (P− + BP+ (P− . 2 2 2

(351)

Let us sketch now the computations which bring to eqs. (346)–(348). First step. By particularizing the formula for the second moments (216) to our case we get t s2 5 k2 2 −˜ γt 2 ˆ 1−e + 2k ds1 ds2 e−˜γ (2t−s1 −s2 )/2 Eρ0 I(ν, h; t) = γ˜ 0 0 4 53 2 4 √ ˆ ∗ Υ˜ (s1 , s2 ) ρ˜(f ; s2 )D(h) ˆ ∗ × Ec ei[(ω−ν)(s1 +s2 )+ B(W (s1 )+W (s2 ))] Tr D(h) 2 4 53 √ ˆ ∗ Υ˜ (s1 , s2 ) D(h)˜ ˆ ρ(f ; s2 ) + ei[(ω−ν)(s1 −s2 )+ B(W (s1 )−W (s2 ))] Tr D(h) 5 + c.c. . (352) 4

Second step. The dynamics Υ˜ (t, s) depends on the Wiener process only through the increments W (τ ) − W (s), s ≤ τ ≤ t, and, so, the conditional expectation i√B(W (t)−W (s)) c Υ˜ (t, s)Fsc is non random and coincides with the expectation E e √ Ec ei B(W (t)−W (s)) Υ˜ (t, s) . Recall that Fsc is the σ-algebra generated by W (τ ), τ ∈ [0, s]; see S3’ for this notation. By eq. (344) and the classical Itô’s formula we get

√ i B(W (t)−W (s))

d e

√ 1 ˜ Υ (t, s)[(] = i B [P+ − P− , ·] + 1l dW (t) 2 4 √ 5 B + K1 − 1l dt ei B(W (t)−W (s)) Υ˜ (t, s)[(] ; 2

(353)

this gives √ Ec ei B(W (t)−W (s)) Υ˜ (t, s)Fsc = e−B(t−s)/2 eK1 (t−s) .

(354)


281

Similarly, we get √ Ec e2i BW (s) ρ˜(f ; s) = e−2Bs eK2 s [ρ0 ] ,

(355)

with K2 = K1 −

B [P+ − P− , ·] , 2

(356)

or, more explicitly, 1 3 ˜ K2 [(] − 2B( = L0 [(] − 2B P+ (P+ + P− (P− + P− (P+ + P+ (P− . 4 4 (357) By inserting these results into eq. (352) we get t s2 5 k2 2 −˜ γt 2 ˆ 1−e + 2k ds1 ds2 e−˜γ (2t−s1 −s2 )/2 Eρ0 I(ν, h; t) = γ˜ 0 0 2 2 4 53 B ˆ ∗ eK1 (s1 −s2 ) eK2 s2 [ρ0 ]D(h) ˆ ∗ × ei(ω−ν)(s1 +s2 )− 2 (s1 +3s2 ) Tr D(h) 4 2 53 B ˆ L˜B s2 [ρ0 ] ˆ ∗ eK1 (s1 −s2 ) D(h)e + ei(ω−ν)(s1 −s2 )− 2 (s1 −s2 ) Tr D(h) 3 + c.c. . (358) 4

Third step. By using the new variables of integration τ = s1 − s2 , s = s2 , we get 4 5 2 ˆ t)2 = k 1 − e−˜γ t + 2k2 [a1 (t) + a2 (t) + a3 (t) + c.c.] , (359) Eρ0 I(ν, h; γ˜ t t−τ 4 53 2 τ B ˆ ∞ , ˆ ∗ eK1 τ D(h)ρ dτ ds e−˜γ (t−s− 2 )+[i(ω−ν)− 2 ]τ Tr D(h) a1 (t) := 0

0

t

a2 (t) :=

(360a) t−τ

dτ 0

a3 (t) :=

0

t

dτ 0

0

t−τ

ds e−˜γ (t−s− 2 )+[i(ω−ν)− 2 ]τ 2 53 4 ˆ ∗ eK1 τ D(h)e ˆ L˜B s [ρ0 − ρ∞ ] , (360b) × Tr D(h) τ

B

τ B ds e−˜γ (t−s− 2 )+[i(ω−ν)− 2 ]τ 4 53 2 ˆ ∗ eK1 τ eK3 (ν)s [ρ0 ]D(h) ˆ ∗ , (360c) × Tr D(h)

K3 (ν) := 2[i(ω − ν) − B] + K2 .

(360d)

282

Alberto Barchielli

The a1 term becomes a1 (t) =

1 γ˜

t

0

4 γ˜ 5 γ ˜ γ ˜ B dτ e− 2 τ − e− 2 t e− 2 (t−τ ) e[i(ω−ν)− 2 ]τ 2 4 53 ˆ ∗ eK1 τ D(h)ρ ˆ ∞ × Tr D(h) (361)

and in the limit it gives 4 53 2 B+˜ γ 1 +∞ ˆ ∞ . (362) ˆ ∗ eK1 τ D(h)ρ dτ e[i(ω−ν)− 2 ]τ Tr D(h) lim a1 (t) = t→+∞ γ˜ 0 The a2 term becomes

t

a2 (t) =

B ˆ ∗ dτ e[i(ω−ν)− 2 ]τ Tr D(h)

0

×e

K1 τ

γ ˜ γ ˜ − e− 2 t e− 2 (t−τ ) [ρ0 − ρ∞ ] ; γ˜ + L˜B

˜B (t−τ )− γ˜ τ L 2

ˆ e D(h)

(363)

˜

because limt→+∞ eLB t [ρ0 − ρ∞ ] = 0, we get lim a2 (t) = 0 .

(364)

t→+∞

Similarly, the a3 term becomes

t

a3 (t) =

i(ω−ν)− B τ ] [ ˆ ∗ 2 dτ e Tr D(h)

0

× eK1 τ

γ ˜

γ ˜

γ ˜

eK3 (ν)(t−τ )− 2 τ − e− 2 t e− 2 (t−τ ) ˆ ∗ [ρ0 ]D(h) γ˜ + K3 (ν)

;

(365)

then, at least almost everywhere in ν, 1 lim t→+∞ T

0

T

γ 1 T i(ω−ν)− B+˜ τ ] [ ˆ ∗ 2 a3 (t)dt = lim dτ e Tr D(h) t→+∞ T 0 1 eK3 (ν)(T −τ ) − 1l K1 τ ∗ ˆ ◦ [ρ0 ]D(h) ×e = 0. γ˜ + K3 (ν) K3 (ν)

(366)

By inserting all these results into (345) we get the expression (346)–(348) for the power spectrum. 5.4 The Fluorescence Spectrum In order to get an explicit expression for the spectrum (347), we need to solve the pseudo–master equation σ(t) ˙ = K1 [σ(t)] with the initial condition σ(0) = ˆ ∞ . We already said that the equilibrium state ρ∞ is supported by the two D(h)ρ extreme states


|1 = |F+ , F+ ,

|2 = |F− , F−

283

(367)

and one can check that all the operations involved in (347) leave the span of |1, |2 invariant; so, we can forget all the other states in H and we are left with formulae involving 2 × 2 matrices. Let us use the Pauli matrices 01 00 1 0 , σ− = , σz = ; (368) σ+ = 00 10 0 −1 with this notation we have in particular P± =

1 2

(1 ± σz ) and

ˆ = αΩeiδ h|1, ˆ 1; +1 D1 + h|g ˆ + P+ + h|g ˆ − P− , D(h) 1 −iδ D1 := e σ− − ieiδ+ sin δ+ P+ − ieiδ− sin δ− P− , Ω ⎞ ⎛ Ω exp [i (δ + 2δ− )] d Ω 2 Re d ⎠. ρ∞ = ⎝ 1 − Ω 2 Re d Ω exp [−i (δ + 2δ− )] d

(369) (370)

(371)

The Angular Distribution of the Spectrum ˆ the states To obtain the angular dependence of the spectrum, let us introduce for h h± concentrated around (θ, φ) and with right/left circular polarization, given by equation (338) with e = e± , where ⎛ ⎞ i sin φ ∓ cos θ cos φ exp(iφ) ⎝ −i cos φ ∓ cos θ sin φ⎠ . (372) e± (θ, φ) = √ 2 ± sin θ Then, we can introduce the two angular spectra Σ± (x; θ) :=

1 Σ(ν; h± ) , |∆Ξ|

(373)

which, by the cylindrical symmetry of the problem, do not depend on φ; recall that x is linked to ν by eq. (325a). Then, we have Ω 2 +∞ −qt e Tr D± (θ)∗ eK1 t [D± (θ)ρ∞ ] dt + c.c., (374) Σ± (x; θ) = 2π 0 3 1 (1 ± cos θ) D1 + g (θ; ±)P , (375) D± (θ) := ± 4 2π =± h± |g g (θ; ±) := $ . |∆Ξ|

(376)

The functions g (θ; ±) depend on S , but after all they are free parameters of the theory: they are square integrable θ-functions, satisfying the constraint

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Alberto Barchielli

π

sin θ [(1 + cos θ) g (θ; +) − (1 − cos θ) g (θ; −)] dθ = 0 ,

(377)

0

coming from the orthogonality of g to |1, 1; +1, see (331). Then, by integrating over the whole solid angle, one gets the total spectrum π 2π Σ(x) = dθ sin θ dφ Σ+ (x; θ) + Σ− (x; θ) = Σ(ν; hk ) , (378) 0

0

k

where {hk } is any c.o.n.s. in Z. When one has g = 0, as in the usual case, one gets Σ± (x; θ) =

3 8π

1 ± cos θ 2

2 Σ(x) .

(379)

For g = 0 the x and θ dependencies do not factorize. In the experiments one measures something proportional to Σ+ (x; θ) + Σ− (x; θ) for θ around π/2; this quantity fails to be proportional to Σ(x) only by the presence of some terms which we expect to be small and which are not qualitatively different from the other terms in Σ(x). So, for simplicity, we shall study only the total spectrum (378). The Total Spectrum By choosing in (378) a basis with h2 = ∆g−1 ∆g , (380a) −1/2 ∆g2 g− − ∆g|g− ∆g , h3 = ∆g−1 g− 2 ∆g2 − |∆g|g− |2 (380b) h1 = |1, 1; +1,

we get the final expression of the total spectrum Ω2 1 v3 + ieiδ− sin δ− + iΩ 2 v1 e−is sin s d − ie−iδ− sin δ− 2π q − iΩ 2 {Re d}eis sin s + e−iδ− sin δ+ Ω 2 c1 sin s − ieis c3 1 g− g− + Ω 2 {Re d}∆g + Re d + id eis sin s u3 + iΩ 2 u1 e−is sin s + q 2 Ω ∆g g− + Ω 2 d1 ∆g v1 + c.c. , + Ω 2 ∆g|g+ c1 − Ω 2 d ∆g2 u1 + q (381) ⎞ ⎛ ⎞ ⎛ ⎛ ⎞ Re d 0 0 1 1 1 ⎝1⎠ , c = ⎝ d ⎠, u = ⎝0⎠ , (382) v= 2 (K + q) K +q K +q 1 1 d

Σ(x) =


285

⎞

⎛

1 −1/2 −1/2 K = ⎝ Ω 2 eis cos s b + y 0 ⎠ . Ω 2 e−is cos s 0 b − y

(383)

By integrating over the reduced frequency x, we get the strength of the total spectrum [cf. (349)] +∞ 2 |α|2 Σ(x) dx = |α|2 Ω 2 {Re d} 1 + Ω 2 sin2 δ+ + 1 − Ω 2 Re d −∞ 3 × sin2 δ− + g− 2 + Re d e2iδ− − 1 + Ω 2 {Re d}g+ 2 . (384) 2 Let us recall that |α|9 is the natural line width, Ω 2 is proportional to the laser intensity, z = (ω − ω0 ) |α|2 is the reduced detuning, y = B/|α|2 is the reduced laser bandwidth, Ω 2 |α|2 ε is an intensity dependent shift, x = (ν − ω0 ) /|α|2 and γ=γ !/|α|2 are the reduced frequency and the reduced instrumental width, respectively, and q = i(x−z)+(γ + y) /2, s = δ+ −δ− , ∆g = g+ −g− . Let us note that ε, 2 δ± , g± , g+ |g− are parameters linked to the S ± scattering matrices, satisfying the two constraints g+ |g− ≤ g+ g− , (385a)

∆g = 0 ⇒ ε = 0 ;

(385b)

apart from this relation ε is an independent parameter of the model. One can check that the spectrum Σ(x) is invariant under the transformation: x → −x , δ± → −δ± ,

z → −z , ε → −ε , g− |g+ → g+ |g− .

(386a) (386b)

The case S ± = 1l Let us recall that the usual model, with only the absorption/emission process, corresponds to δ± = 0, g± = 0, ε = 0, z = z˜, s = 0. In this case we obtain 4Ω 2 Ω2 1 v3 d + 2v3 + Σ(x) = Re d + c.c. , (387) 2π q N 1 + y + 2iz , Γ 2 = (1 + y)(1 + y + 2Ω 2 ) , 4z 2 + Γ 2 9 v3 = [2 + γ + y + 2i (x − z)] [1 + γ + 4y + 2i (x − 2z)] N ,

(389)

N = 4Ω 2 [1 + γ + 2y + 2i(x − z)] + [2 + γ + y + 2i (x − z)] × [1 + γ + 4y + 2i (x − 2z)] (1 + γ + 2ix) .

(390)

d=

(388)

Now, the spectrum Σ(x) is invariant under the transformation: x → −x ,

z → −z .

(391)

286

Alberto Barchielli 0.18

0.18 2

(a) 0.15

2

(b)

W =3, y = 0

W =3, y = 0.5

0.15

0.12

0.12

0.09

0.09

0.06

0.06

0.03

0.03

0

0 -7

-3.5

0

3.5

7

0.18

-7

-3.5

0

3.5

7

0.18 W2=3, y = 1

(c) 0.15

W2=3, y = 4

(d) 0.15

0.12

0.12

0.09

0.09

0.06

0.06

0.03

0.03

0

0 -7

-3.5

0

3.5

7

-7

-3.5

0

3.5

7

Fig. 8. The spectrum Σ(x) × 100 for laser bandwidths y = 0, 0.5, 1, 4 and γ = 0.6, Ω 2 = 3, z = 0.

Plots Let us end by presenting some plots of the spectrum with various choices of the parameters. Let us consider only the resonant case (no detuning: z = 0) and let us take γ = 0.6 for the reduced instrumental width; let us recall the in our units the natural line width is 1. In all the plots we compare the spectrum predicted by the usual model (dashed lines), in which only the absorption/emission channel is present, with the spectrum predicted by the modified model (solid lines), in which both the absorption/emission channel and the direct scattering channel are present. The usual model is characterized by δ± = 0, g± 2 = 0, ε = 0, while as an example of modified model we choose δ+ = −0.03, δ− = 0.13, g+ 2 = 0.0045, g− 2 = 0.0055, g+ |g− = −0.004 + i × 0.002, ε = −0.001. In Figs. 8, 9, 10 we consider three laser intensities Ω 2 = 3, 28, 50 and four laser bandwidths y = 0, 0.5, 1, 4. Our choice of the parameters for the modified model is such that for a monochromatic laser in resonance (Fig. 1(a)) the modified spectrum is not quantitatively too different from the usual one, but its asymmetry is clear. The differences between the two cases are enhanced by the presence of the bandwidth. In Fig. 11 we have considered a stimulating laser in resonance with a very large bandwidth y = 50 and four levels of intensity: Ω 2 = 5, 15, 30, 60. The instrumentals width is again γ = 0.6.

Quantum Continual Measurements 0.1

287

0.1 W2=28, y = 0

(a)

0.08

0.06

0.06

0.04

0.04

0.02

0.02

0 -10

-5

0

5

W2=28, y = 0.5

(b)

0.08

10

0.1

0 -10

-5

0

5

10

0.1 W2=28, y = 1

(c)

0.08

0.06

0.06

0.04

0.04

0.02

0.02

0 -10

-5

0

5

W2=28, y = 4

(d)

0.08

10

0 -10

-5

0

5

10


0.15

0.15 2

(a) 0.12

0.12

0.09

0.09

0.06

0.06

0.03

0.03

0 -15

-10

-5

0

5

10

15

0.15

0 -15

W =50, y = 0.5

-10

-5

0

5

10

15

0.15 2

(c)

0.12

0.09

0.09

0.06

0.06

0.03

0.03

-10

-5

0

5

10

2

(d)

W =50, y = 1

0.12

0 -15

2

(b)

W =50, y = 0

15

0 -15

W =50, y = 4

-10

-5

0

5

10

15


288

Alberto Barchielli 0.07 0.06

0.07 2

(a)

W =5, y = 50

0.06

0.05

0.05

0.04

0.04

0.03

0.03

0.02

0.02

0.01

0.01

0 -15

-10

-5

0

5

10

15

0.07 0.06

2

(b)

0 -15

W =15, y = 50

-10

-5

0

5

10

15

0.07 W2=30, y = 50

(c)

0.06

0.05

0.05

0.04

0.04

0.03

0.03

0.02

0.02

0.01

0.01

0 -15

-10

-5

0

5

10

15

0 -15

W2=60, y = 50

(d)

-10

-5

0

5

10

15

Fig. 11. The spectrum Σ(x) × 100 for laser bandwidth y = 50 and γ = 0.6, Ω 2 = 5, 15, 30, 60, z = 0.

Acknowledgments Work supported in part by the European Community’s Human Potential Programme under contract HPRN-CT-2002-00279, QP-Applications, and by Istituto Nazionale di Fisica Nucleare, Sezione di Milano. The author is indebted to Franco Fagnola e Matteo Gregoratti for discussions ´ and suggestions and to Stephane Attal for the invitation to the stimulating “Ecole d’été de Mathématiques 2003” in Grenoble.

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Index of Volume III

F (T ) fixed points set, 167 Λ configuration, 258 ω-continuous, 123 σ-finite von Neumann algebra, 163 σ-weakly continuous groups, 113 Absorption, 272 Adapted process, 214 regular, 214 stochastically integrable, 215 unitary, 219 Adjoint pair, 217 Affinities, 19, 49, 56 Annihilation, creation and conservation processes, 213 Antibunching, 264 Araki’s perturbation theory, 11 Bose fields, 213 Broad–band approximation, 229 CAR algebra, 26 even, 28 CCR, 148, 211 Central limit theorem, 20 Characteristic functional, 235 operator, 235 Classes of bounded elements left, 127 right, 127 Classical quantum states, 126 Cocycle property, 220 Coherent vectors, 210

Completely positive map, 89 semigroup, 90 Conditional expectation, 122, 167 ψ-compatible, 122 Continual measurements, 230 Correlation function, 20, 47 Counting process, 263 quanta, 230 Current charge, 36, 45, 55 heat, 17, 36, 45, 55 output, 248 Dark state, 267 Davies generator, 97 Decoherence –induced spin algebra, 143 environmental, 119 time, 125 Demixture, 225 Density operator, 27 Detailed Balance Condition, 92 AFGKV, 93 Detuning parameter, 261 shifted, 276 Direct detection, 247 Dynamical system C∗, 5 W ∗ , 94 weakly asymptotically Abelian, 11

294

Index of Volume III

Effective dipole operator, 280 Emission, 272 Entropy production, 9, 18, 19, 24, 39, 44, 46, 55 relative, 9 Ergodic generator, 114 globally, 114 Exclusive probability densities, 251 Experimental resolution , 139 Exponential domain, 210 vectors, 210 Exponential law, 29, 37 Fermi algebra, 26 Fermi Golden Rule, 54, 76 analytic, 76 dynamical, 76 spectral, 76 Fermi-Dirac distribution, 27 Field quadratures, 213, 231 Fluctuation algebra, 21 Fluorescence spectrum, 279 Flux charge, 36, 45, 55 heat, 17, 36, 45, 55 Fock space, 26, 210 vacuum, 210 Form-potential, 194 Friedrichs model, 40 Gauge group, 26 Gorini-Kossakowski-Sudershan-Lindblad generator, 141 Harmonic operator, 184 Heterodyne detection, 252 balanced, 254 Indirect measurement, 230 Infinitely divisible law, 239 Input fields, 232 Instrument, 244 Interaction picture, 222 Isometric-sweeping decomposition, 133 Ito table, 215 Jacobs-deLeeuw-Glicksberg splitting, 136

Jordan-Wigner transformation, 31 Junction, 15, 35 Kinetic coefficients, 19, 25 Kubo formula, 20, 25, 50, 56 Laser intensity, 276 Level Shift Operator, 73 Lindblad generator, 90 Linear response, 18, 25 Liouville operator, 227 Liouvillean -Lp , 8 -ω, 8, 28 semi–, 96 perturbation of, 11 standard, 8 Localization properties, 237 Møller morphism, 11, 15 Mandel Q-parameter, 249 Markov map, 89 Master equation, 227 Modular conjugation, 28 group, 39 operator, 28 Narrow topology, 166 NESS, 8, 43 Nominal carrier frequencies, 228 Onsager reciprocity relations, 20, 25, 50, 56 Open system, 14 Operator number, 26 Output characteristic operator, 240 Output fields, 232 Pauli matrices, 30 Pauli’s principle, 29 Perturbed convolution semigroup, 151 of promeasures, 151 Poisson, 153 Phase diffusion model, 225, 273 Photoelectron counter, 248 Photon scattering, 272 Picture Heisenberg, 89

Index of Volume III Schrödinger, 89 Standard, 89 Pointer states, 123 continuous, 139 Poissonian statistics sub–, 250 super–, 250 Polarization, 228 Potential operator, 195 Power spectrum, 279 Predual space, 164 Promeasure, 149 Fourier transform of, 150 Quantum Brownian motion, 155 Quantum dynamical semigroup, 91, 122 on CCR algebras, 153 minimal, 167 Quantum Markovian semigroup, 22, 52 irreducible, 186 Quantum stochastic equation, 225 Quasi–monochromatic fields, 228 Rabi frequencies, 261 Reduced characteristic operator, 241 dynamics, 244 evolution, 122 Markovian dynamics, 122 Representation Araki-Wyss, 28 GNS, 5, 27 semistandard, 95 standard, 94 universal, 6 Reservoir, 14 Response function, 248 Rotating wave approximation, 228 Scattering matrix, 41 Semifinite weight, 121 Semigroup C0 -, 112 C0∗ -, 113 one-parameter, 112 recurrent, 199 transient, 199 Sesquilinear form, 164 Shelving effect, 257

electron, 258 Shot noise, 279 Singular coupling limit, 141 Spectral Averaging, 83 Spin system, 31, 138 State, 5 chaotic, 14 decomposition, 6 ergodic, 5, 28 factor, 8 factor or primary, 27 faithful, 163 invariant, 5, 27, 163 KMS, 8, 19, 27, 28 mixing, 5, 28 modular, 8, 27 non-equilibrium steady, 8, 43 normal, 163 primary, 8 quasi-free gauge-invariant, 27, 31, 35 reference, 3, 9 relatively normal, 5 time reversal invariant, 15 States classical, 225 disjoint, 6 mutually singular, 6 orthogonal, 6 quantum, 225 quasi-equivalent, 7, 27, 44 unitarily equivalent, 7, 27, 44 Subharmonic operator, 184 Superharmonic operator, 184 Test functions, 235 Thermodynamic FGR, 24, 56 first law, 17, 24, 37 second law, 18, 24 Tightness, 166 Time reversal, 15, 42 TRI, 15 Two-positive operator, 127 Unitary decomposition, 130 V configuration, 258 Van Hove limit, 22, 50 Von Neumann algebra

295

296

Index of Volume III

enveloping, 5 universal enveloping, 6 Wave operator, 41 Weak Coupling Limit, 22, 50, 77

dynamical, 76 stationary, 76 Weyl operator, 211 Wigner-Weisskopf atom, 40

Information About the Other Two Volumes

Contents of Volume I

References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . XII Introduction to the Theory of Linear Operators Alain Joye . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 2 Generalities about Unbounded Operators . . . . . . . . . . . . . . . . . . . . . . . . . . . . 3 Adjoint, Symmetric and Self-adjoint Operators . . . . . . . . . . . . . . . . . . . . . . . 4 Spectral Theorem . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 4.1 Functional Calculus . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 4.2 L2 Spectral Representation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 5 Stone’s Theorem, Mean Ergodic Theorem and Trotter Formula . . . . . . . . . 6 One-Parameter Semigroups . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .

1 1 2 5 13 15 22 29 35 40

Introduction to Quantum Statistical Mechanics Alain Joye . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1 Quantum Mechanics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1.1 Classical Mechanics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1.2 Quantization . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1.3 Fermions and Bosons . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 2 Quantum Statistical Mechanics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 2.1 Density Matrices . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 3 Boltzmann Gibbs . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .

41 42 42 46 53 54 54 57 67

Elements of Operator Algebras and Modular Theory Stéphane Attal . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1.1 Discussion . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1.2 Notations . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 2 C ∗ -algebras . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .

69 70 70 71 71


299

2.1 First definitions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 71 2.2 Spectral analysis . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 73 2.3 Representations and states . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 79 2.4 Commutative C ∗ -algebras . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 83 2.5 Appendix . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 84 3 von Neumann algebras . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 86 3.1 Topologies on B(H) . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 86 3.2 Commutant . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 89 3.3 Predual, normal states . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 90 4 Modular theory . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 92 4.1 The modular operators . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 92 4.2 The modular group . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 96 4.3 Self-dual cone and standard form . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 100 References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 105 Quantum Dynamical Systems Claude-Alain Pillet . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 107 1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 107 2 The State Space of a C ∗ -algebras . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 110 2.1 States . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 110 2.2 The GNS Representation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 119 3 Classical Systems . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 123 3.1 Basics of Ergodic Theory . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 123 3.2 Classical Koopmanism . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 127 4 Quantum Systems . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 130 4.1 C ∗ -Dynamical Systems . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 132 4.2 W ∗ -Dynamical Systems . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 139 4.3 Invariant States . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 141 4.4 Quantum Dynamical Systems . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 142 4.5 Standard Forms . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 147 4.6 Ergodic Properties of Quantum Dynamical Systems . . . . . . . . . . . . . . 153 4.7 Quantum Koopmanism . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 161 4.8 Perturbation Theory . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 165 5 KMS States . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 168 5.1 Definition and Basic Properties . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 168 5.2 Perturbation Theory of KMS States . . . . . . . . . . . . . . . . . . . . . . . . . . . . 178 References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 180 The Ideal Quantum Gas Marco Merkli . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 183 1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 184 2 Fock space . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 185 2.1 Bosons and Fermions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 185 2.2 Creation and annihilation operators . . . . . . . . . . . . . . . . . . . . . . . . . . . . 188 2.3 Weyl operators . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 191

300


2.4 The C ∗ -algebras CARF (H), CCRF (H) . . . . . . . . . . . . . . . . . . . . . . . . 194 2.5 Leaving Fock space . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 197 3 The CCR and CAR algebras . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 198 3.1 The algebra CAR(D) . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 199 3.2 The algebra CCR(D) . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 200 3.3 Schrödinger representation and Stone – von Neumann uniqueness theorem . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 203 3.4 Q–space representation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 207 3.5 Equilibrium state and thermodynamic limit . . . . . . . . . . . . . . . . . . . . . 209 4 Araki-Woods representation of the infinite free Boson gas . . . . . . . . . . . . . . 213 4.1 Generating functionals . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 214 4.2 Ground state (condensate) . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 217 4.3 Excited states . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 222 4.4 Equilibrium states . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 224 4.5 Dynamical stability of equilibria . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 228 References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 233 Topics in Spectral Theory Vojkan Jakˇsić . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 235 1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 236 2 Preliminaries: measure theory . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 238 2.1 Basic notions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 238 2.2 Complex measures . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 238 2.3 Riesz representation theorem . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 240 2.4 Lebesgue-Radon-Nikodym theorem . . . . . . . . . . . . . . . . . . . . . . . . . . . 240 2.5 Fourier transform of measures . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 241 2.6 Differentiation of measures . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 242 2.7 Problems . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 247 3 Preliminaries: harmonic analysis . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 248 3.1 Poisson transforms and Radon-Nikodym derivatives . . . . . . . . . . . . . . 249 3.2 Local Lp norms, 0 < p < 1. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 253 3.3 Weak convergence . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 253 3.4 Local Lp -norms, p > 1 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 254 3.5 Local version of the Wiener theorem . . . . . . . . . . . . . . . . . . . . . . . . . . . 255 3.6 Poisson representation of harmonic functions . . . . . . . . . . . . . . . . . . . 256 3.7 The Hardy class H ∞ (C+ ) . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 258 3.8 The Borel transform of measures . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 261 3.9 Problems . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 263 4 Self-adjoint operators, spectral theory . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 267 4.1 Basic notions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 267 4.2 Digression: The notions of analyticity . . . . . . . . . . . . . . . . . . . . . . . . . . 269 4.3 Elementary properties of self-adjoint operators . . . . . . . . . . . . . . . . . . 269 4.4 Direct sums and invariant subspaces . . . . . . . . . . . . . . . . . . . . . . . . . . . 272 4.5 Cyclic spaces and the decomposition theorem . . . . . . . . . . . . . . . . . . . 273 4.6 The spectral theorem . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 273


301

4.7 Proof of the spectral theorem—the cyclic case . . . . . . . . . . . . . . . . . . . 274 4.8 Proof of the spectral theorem—the general case . . . . . . . . . . . . . . . . . 277 4.9 Harmonic analysis and spectral theory . . . . . . . . . . . . . . . . . . . . . . . . . 279 4.10 Spectral measure for A . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 280 4.11 The essential support of the ac spectrum . . . . . . . . . . . . . . . . . . . . . . . . 281 4.12 The functional calculus . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 281 4.13 The Weyl criteria and the RAGE theorem . . . . . . . . . . . . . . . . . . . . . . . 283 4.14 Stability . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 285 4.15 Scattering theory and stability of ac spectra . . . . . . . . . . . . . . . . . . . . . 286 4.16 Notions of measurability . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 287 4.17 Non-relativistic quantum mechanics . . . . . . . . . . . . . . . . . . . . . . . . . . . 290 4.18 Problems . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 291 5 Spectral theory of rank one perturbations . . . . . . . . . . . . . . . . . . . . . . . . . . . . 295 5.1 Aronszajn-Donoghue theorem . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 296 5.2 The spectral theorem . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 298 5.3 Spectral averaging . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 299 5.4 Simon-Wolff theorems . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 300 5.5 Some remarks on spectral instability . . . . . . . . . . . . . . . . . . . . . . . . . . . 301 5.6 Boole’s equality . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 302 5.7 Poltoratskii’s theorem . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 304 5.8 F. & M. Riesz theorem . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 308 5.9 Problems and comments . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 309 References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 311 Index of Volume-I . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 313 Information about the other two volumes Contents of Volume II . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 318 Index of Volume II . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 321 Contents of Volume III . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 323 Index of Volume III . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 327

Index of Volume I

∗-algebra, 72 morphism, 77 C ∗ -algebra, 71 morphism, 77 C0 semigroup, 35 W ∗ -algebra, 139 ∗-derivation, 132 µ-Liouvillean, 143 Adjoint, 6 Algebra ∗, 72 C ∗ , 71 Banach, 72 von Neumann, 88 Analytic vector, 32, 136, 202 Approximate identity, 84 Aronszajn-Donoghue theorem, 297 Asymptotic abelianness, 229 Baker-Campbell-Hausdorff formula, 193 Banach algebra, 72 Birkhoff ergodic theorem, 125 Bogoliubov transformation, 200 Boltzmann’s constant, 57 Boole’s equality, 302 Borel transform, 249, 261 Bose gas, 140, 145, 177 Boson, 53, 186 Canonical anti-commutation relations, 190 Canonical commutation relations, 50, 190, 192 Canonical transformation, 43

Cantor set, 310 CAR, CCR algebra CARF (h), 195 CCRF (h), 195 quasi-local, 198 simplicity, 199, 200 uniqueness, 199, 200 CAR-algebra, 134, 172 Cayley transform, 8 CCR-algebra, 140, 145, 177 Center, 118 Central support, 118 Chaos, 186 Character, 83 Chemical potential, 58 Commutant, 89 Condensate, 217 Configuration space, 42 Conjugation, 10 Contraction semigroup, 37 Critical density, 227 Cyclic subspace, 22, 295 vector, 22, 195, 273 Deficiency indices, 8 Density matrix, 55, 114, 290 Dynamical system C ∗ , 132 W ∗ , 139 classical, 124 ergodic, 125, 156 mixing, 127, 156

Index of Volume I quantum, 142 Ensemble canonical, 60 grand canonical, 63 microcanonical, 57 Entropy Boltzmann, 57 Enveloping von Neumann algebra, 119 Essential support, 281 Evolution group, 29 Exponential law, 203 Factor, 118 Faithful representation, 80 Fermi gas, 134, 172 Fermion, 53, 186 Finite particle subspace, 192 Finite quantum system, 133 Fock space, 186 Folium, 119 Free energy, 61 Functional calculus, 16, 25, 281 G.N.S. representation, 82 Hahn decomposition theorem, 240 Hamiltonian, 290 Hamiltonian system, 43 Hardy class, 258 Harmonic oscillator, 50, 205 Heisenberg picture, 51 Heisenberg uncertainty principle, 49, 290 Helffer-Sjöstrand formula, 17 Hille-Yosida theorem, 37 Ideal left, 84 right, 84 two-sided, 84 Ideal gas, 185 Indistinguishable, 186 Individual ergodic theorem, 125 Infinitesimal generator, 35 Internal energy, 58 Invariant subspace, 22, 272 Invertible, 73 Isometric element, 75

303

Jensen’s formula, 259 Kaplansky density theorem, 111 Kato-Rellich theorem, 285 Kato-Rosenblum theorem, 287 Koopman ergodicity criterion, 129 Koopman lemma, 128 Koopman mixing criterion, 129 Koopman operator, 128 Lebesgue-Radon-Nikodym theorem, 240 Legendre transform, 62 Liouville equation, 43 Liouville’s theorem, 43 Liouvillean, 128, 143, 150, 161, 168 Lummer Phillips theorem, 38 Mean ergodic theorem, 32, 128 Measure absolutely continuous, 240 complex, 239 regular Borel, 238 signed, 239 space, 238 spectral, 274, 280, 295 support, 238 Measurement, 48 simultaneous, 49 Measures equivalent, 280 mutually singular, 240 Modular conjugation, 96 operator, 96 Morphism ∗-algebra, 77 C ∗ -algebra, 77 Nelson’s analytic vector theorem, 32 Norm resolvent convergence, 27 Normal element, 75 Normal form, 143 Observable, 42, 46, 123, 290 Operator (anti-)symmetrization, 187 closable, 5, 268 closed, 2, 268 core, 31, 268

304

Index of Volume I

creation, annihilation, 50, 188 dissipative, 37 domain, 2 essentially self-adjoint, 7 extension, 2 field, 192 graph, 3, 268 linear, 2 multiplication, 14, 273 number, 186 positive, 271 relatively bounded, 12, 285 Schrödinger, 47 self-adjoint, 7 symmetric, 5 trace class, 286 Weyl, 193 Partition function, 61, 64 Pauli’s principle, 54, 191 Perturbation theory rank one, 295 Phase space, 42 Planck law, 226 Poisson bracket, 44 Poisson representation, 256 Poisson transform, 249 Poltoratskii’s theorem, 262, 304 Positive element, 78 linear form, 80 Predual, 90 Pressure, 58 Quantum dynamical system, 142 Quasi-analytic extension, 16 RAGE theorem, 284, 290 Reduced Liouvillean, 161 Representation, 80 Q-space (CCR), 207 Araki-Woods, 224 faithful, 80 Fock, 203 GNS, 120 GNS (ground state of Bose gas), 221 Quasi-equivalent, 206 regular (of CCR), 201 ¨ Schrdinger, 204

Resolvent, 3 first identity, 4, 268 norm convergence, 27 set, 3, 268 strong convergence, 194 Resolvent set, 73 Return to equilibrium, 127, 230 Riemann-Lebesgue lemma, 241 Riesz representation theorem, 240 Schrödinger picture, 51 Sector, 186 Self-adjoint element, 75 Simon-Wolff theorems, 300 Spatial automorphism, 133 Spectral averaging, 299 Spectral radius, 74 Spectral theorem, 23, 274, 298 Spectrum, 3, 73, 83, 268 absolutely continuous, 278 continuous, 278 essential, 284 point, 268 pure point, 278 singular, 278 singular continuous, 278 Spin, 53 Standard form, 148 Standard Liouvillean, 150, 168 Standard unitary, 149 State, 81, 198 absolutely continuous, 155 centrally faithful, 118 coherent, 52 disjoint, 119 equilibrium, 124 extremal, 159 factor, 231 faithful, 110, 117 gauge invariant, 173, 212 generating functional, 214 Gibbs, 210 ground (Bose gas), 220 invariant, 141 KMS, 169, 210 local perturbation, 228 mixed, 54 mixing, 232 normal, 92, 112

Index of Volume I orthogonal, 119 pure, 46, 56 quasi-equivalent, 119 quasi-free, 147, 173, 212 relatively normal, 119, 198 tracial, 96 Stone’s formula, 282 Stone’s theorem, 30 Stone-von Neumann uniqueness theorem, 205 Strong resolvent convergence, 194 Support, 117 Temperature, 58, 61 Thermodynamic first law, 58 limit, 184, 197 second law, 58 Topology σ-strong, 111 σ-weak, 87, 111 strong, 86

uniform, 86 weak, 86 weak-, 139 Trotter product formula, 33 Unit, 72 approximate, 84 Unitary element, 75 Vacuum, 186 Von Neumann density theorem, 111 Von Neumann ergodic theorem, 33, 128 Wave operators, 286 complete, 286 Weyl (CCR) relations, 193 Weyl commutation relations, 140 Weyl quantization, 47 Weyl’s criterion, 283 Weyl’s theorem, 286 Wiener theorem, 241, 255

305

Contents of Volume II

Ergodic Properties of Markov Processes Luc Rey-Bellet . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 2 Stochastic Processes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 3 Markov Processes and Ergodic Theory . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 3.1 Transition probabilities and generators . . . . . . . . . . . . . . . . . . . . . . . . . 3.2 Stationary Markov processes and Ergodic Theory . . . . . . . . . . . . . . . . 4 Brownian Motion . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 5 Stochastic Differential Equations . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 6 Control Theory and Irreducibility . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 7 Hypoellipticity and Strong-Feller Property . . . . . . . . . . . . . . . . . . . . . . . . . . . 8 Liapunov Functions and Ergodic Properties . . . . . . . . . . . . . . . . . . . . . . . . . . References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .

1 1 2 4 4 7 12 14 24 26 28 39

Open Classical Systems Luc Rey-Bellet . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 2 Derivation of the model . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 2.1 How to make a heat reservoir . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 2.2 Markovian Gaussian stochastic processes . . . . . . . . . . . . . . . . . . . . . . . 2.3 How to make a Markovian reservoir . . . . . . . . . . . . . . . . . . . . . . . . . . . 3 Ergodic properties: the chain . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 3.1 Irreducibility . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 3.2 Strong Feller Property . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 3.3 Liapunov Function . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 4 Heat Flow and Entropy Production . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 4.1 Positivity of entropy production . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 4.2 Fluctuation theorem . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 4.3 Kubo Formula and Central Limit Theorem . . . . . . . . . . . . . . . . . . . . . . References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .

41 41 44 44 48 50 52 56 57 58 66 69 71 75 77


307

Quantum Noises Stéphane Attal . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 79 1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 80 2 Discrete time . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 81 2.1 Repeated quantum interactions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 81 2.2 The Toy Fock space . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 83 2.3 Higher multiplicities . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 89 3 Itô calculus on Fock space . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 93 3.1 The continuous version of the spin chain: heuristics . . . . . . . . . . . . . . 93 3.2 The Guichardet space . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 94 3.3 Abstract Itô calculus on Fock space . . . . . . . . . . . . . . . . . . . . . . . . . . . . 97 3.4 Probabilistic interpretations of Fock space . . . . . . . . . . . . . . . . . . . . . . 105 4 Quantum stochastic calculus . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 110 4.1 An heuristic approach to quantum noise . . . . . . . . . . . . . . . . . . . . . . . . 110 4.2 Quantum stochastic integrals . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 113 4.3 Back to probabilistic interpretations . . . . . . . . . . . . . . . . . . . . . . . . . . . 122 5 The algebra of regular quantum semimartingales . . . . . . . . . . . . . . . . . . . . . . 123 5.1 Everywhere defined quantum stochastic integrals . . . . . . . . . . . . . . . . 124 5.2 The algebra of regular quantum semimartingales . . . . . . . . . . . . . . . . . 127 6 Approximation by the toy Fock space . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 130 6.1 Embedding the toy Fock space into the Fock space . . . . . . . . . . . . . . . 130 6.2 Projections on the toy Fock space . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 132 6.3 Approximations . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 136 6.4 Probabilistic interpretations . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 138 6.5 The Itô tables . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 139 7 Back to repeated interactions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 139 7.1 Unitary dilations of completely positive semigroups . . . . . . . . . . . . . . 140 7.2 Convergence to Quantum Stochastic Differential Equations . . . . . . . . 142 8 Bibliographical comments . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 145 References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 145 Complete Positivity and the Markov structure of Open Quantum Systems Rolando Rebolledo . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 149 1 Introduction: a preview of open systems in Classical Mechanics . . . . . . . . . 149 1.1 Introducing probabilities . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 152 1.2 An algebraic view on Probability . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 154 2 Completely positive maps . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 157 3 Completely bounded maps . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 162 4 Dilations of CP and CB maps . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 163 5 Quantum Dynamical Semigroups and Markov Flows . . . . . . . . . . . . . . . . . . 168 6 Dilations of quantum Markov semigroups . . . . . . . . . . . . . . . . . . . . . . . . . . . 173 6.1 A view on classical dilations of QMS . . . . . . . . . . . . . . . . . . . . . . . . . . 174 6.2 Towards quantum dilations of QMS . . . . . . . . . . . . . . . . . . . . . . . . . . . 180 References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 181

308


Quantum Stochastic Differential Equations and Dilation of Completely Positive Semigroups Franco Fagnola . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 183 1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 183 2 Fock space notation and preliminaries . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 184 3 Existence and uniqueness . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 188 4 Unitary solutions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 191 5 Emergence of H-P equations in physical applications . . . . . . . . . . . . . . . . . . 193 6 Cocycle property . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 196 7 Regularity . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 199 8 The left equation: unbounded Gα β . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 203 9 Dilation of quantum Markov semigroups . . . . . . . . . . . . . . . . . . . . . . . . . . . . 208 10 The left equation with unbounded Gα β : isometry . . . . . . . . . . . . . . . . . . . . . . 213 11 The right equation with unbounded Fβα . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 216 References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 218 Index of Volume-II . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 221 Information about the other two volumes Contents of Volume I . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 224 Index of Volume I . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 228 Contents of Volume III . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 232 Index of Volume III . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 236

Index of Volume II

Adapted domain, 114 Algebra Banach, 156 von Neumann, 157 Algebraic probability space, 154 Banach algebra, 156 Brownian interpretation, 107 Brownian motion, 13 canonical, 14 Chaotic expansion, 106 representation property, 106 space, 106 Classical probabilistic dilations, 174 Coherent vector, 96 Completely bounded map, 162 Completely positive map, 158 Conditional expectation, 173 Conditionally CP map, 170 Control, 24 Dilation, 208 Dilations of QDS, 173 Dynkin’s formula, 21 Elliptic operator, 27 Ergodic, 8

Fock space toy, 84 multiplicity n, 90 Gaussian process, 13 Generator, 7 Gibbs measure, 45 Hörmander condition, 27 Independent increments, 13 Initial distribution, 5 Integral representation, 85 Itô integrable process, 99 integral, 15, 99 process, 16 Lyapunov function, 21 Markov process, 4 Martingale normal, 105 Measure preserving, 8 Mild solution, 217 Mixing, 9 Modification, 13 Normal martingale, 105

Feller semigroup strong, 7 weak, 7 First fundamental formula, 186

Obtuse system, 90 Operator process, 185

310

Index of Volume II

Operator system, 156

Regular quantum semimartingales, 128

Poisson interpretation, 107 Predictable representation property, 105 Probabilistic interpretation, 87, 107 p-, 88 Probability space algebraic, 154 Process, 2 distribution, 3 Gaussian, 13 Itô integrable, 99 Ito, 16 Markov, 4 strong, 20 modification, 13 operator, 185 adapted, 111 path, 3 stationary, 7 Product p-, 89 Poisson, 108 Wiener, 108

Sesqui-symmetric tensor, 91 Spectral function, 48 State normal, 155 Stationary increments, 13 Stinespring representation, 164 Stochastic integral, 15 quantum, 115 Stochastically integrable, 185 Stopping time, 21 Strong Markov process, 20 Structure equation, 107

Quantum dynamical semigroup, 170, 208 minimal, 210 Quantum Markov semigroup, 170, 208 Quantum noises, 111 Quantum probabilistic dilations, 174, 180

Uniform topology, 156 Uniformly continuous QMS, 170

Tensor sesqui-symmetric, 91 Topology uniform, 156 Total variation norm, 12 Totalizing set, 205 Toy Fock space, 84 multiplicity n, 90 Transition probability, 5

Vacuum, 96 von Neumann algebra, 157

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