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Non-Relativistic Quantum Electrodynamics PDF

201 Pages·1982·10.479 MB·English
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NON-RELATIVISTIC QUANTUM ELECTRODYNAMICS NON-RELATIVISTIC QUANTUM ELECTRODYNAMICS W. P. Healy Department of Mathematics Royal Melbourne Institute of Technology Melbourne, Victoria Australia 1982 ACADEMIC PRESS A Subsidiary of Harcourt Brace Jovanovich, Publishers LONDON NEW YORK PARIS SAN DIEGO SAN FRANCISCO SAO PAULO SYDNEY TOKYO TORONTO ACADEMIC PRESS INC. (LONDON) LTD 24/28 Oval Road, London NW1 7DX United States Edition published by ACADEMIC PRESS INC. 111 Fifth Avenue, New York, New York 10003 Copyright © 1982 by ACADEMIC PRESS INC. (LONDON) LTD All Rights Reserved No part of this book may be reproduced in any form by photostat, microfilm, or any other means without written permission from the publishers Healy, W. P. Non-relativistic quantum electrodynamics. 1. Quantum electrodynamics I. Title 537.6 QC680 LCCCN 82-71002 ISBN 0-12-335720-9 Typeset and printed by The Universities Press (Belfast) Ltd. Preface Non-relativistic quantum electrodynamics is the theory of the interaction of photons and slowly moving charged particles, such as those found in atoms and molecules under normal laboratory conditions. In recent years there has been a resurgence of interest in this subject, due in part to the development of lasers and their use as spectroscopic tools for investigat­ ing a variety of physical and chemical phenomena. This book presents a systematic account of non-relativistic quantum electrodynamics and is aimed at theoretical physicists, applied mathematicians and physical chemists who have some knowledge of classical electrodynamics and of Dirac’s formulation of ordinary quantum mechanics. The theory is derived by the method of canonical quantization and is thus related to classical electrodynamics through Bohr’s correspondence principle. This method seems the most natural and easiest to use in a non-relativistic context and, historically, is the one by which the electro­ magnetic field was first quantized. It is true that the description of the spin of the charged particles does not emerge automatically from the resulting formalism, but this can, if desired, be added on in an ad hoc fashion, as in non-relativistic quantum mechanics. The canonical formula­ tion of classical electrodynamics in the Coulomb gauge is dealt with at some length, as are the transformations of the energy and momentum densities of the system. Particular attention is drawn to the inversion of the relations defining the electromagnetic potentials that may be achieved by taking certain line integrals over the fields. These path-dependent potentials are interesting in their own right, but do not appear to be widely known. Moreover, they are closely associated with the path- dependent polarization and magnetization fields that occur in the multi­ polar form of the Hamiltonian, which is related to the more standard minimal-coupling form through the unitary transformation that was first carried out by E. A. Power and S. Zienau. The interpretation of this transformation is still, even now, a subject of debate in the literature. It is hoped that the treatment given here will show (i) that the correct canonical variables and consistent equations of motion are obtained by interpreting the transformation as the quantum analogue of a classical VI PREFACE canonical transformation and (ii) that the partitioning (for the purposes of perturbation theory) of the multipolar Hamiltonian is intrinsically path- dependent, due to the path-dependence of the polarization and magne­ tization fields. This can be regarded as a kind of gauge dependence. The gauge invariance of physical results, however, is demonstrated for some cases. The summation convention is used, so that a repeated Latin suffix always implies a sum. References are listed alphabetically according to the surname of the author at the end of each chapter. They are cited in the text by author name and year of publication. A list of physical constants, some theorems in vector analysis, a note on longitudinal and transverse vector fields and two operator identities appear in Appendices A, B, C and D, respectively. The reader is referred to these where necessary in the body of the book. The problems that are given at the end of many sections are meant to illustrate the theory, and in some cases to develop it further. The work leading to this book was mostly carried out in the Research School of Chemistry, Institute of Advanced Studies, and the Department of Applied Mathematics, Faculty of Science, at the Australian National University. Some of the last section of Chapter 7 is based on work done in collaboration with Dr. R. G. Woolley. I am very grateful to Professor D. P. Craig of the Research School of Chemistry for suggesting and encouraging the project and to Mrs B. Hawkins of the Department of Applied Mathematics for typing the manuscript. W. P. Healy Melbourne March 1982 Contents Preface v Chapter 1 Introduction 1.1 Non-relativistic theory 1 1.2 Planck’s radiation law 2 1.3 Einstein’s A and B coefficients 5 1.4 Uncertainty relations 8 Chapter 2 The Classical Equations of Motion 2.1 Maxwell-Lorentz theory 14 2.2 C, P and T symmetries 16 2.3 Vector and scalar potentials 20 2.4 Gauge transformations 23 2.5 The Coulomb gauge 27 2.6 Energy and momentum balance 31 Chapter 3 Canonical Formalism 3.1 Discrete systems—particles 38 3.2 Continuous systems—fields 43 3.3 Transverse fields 47 3.4 Canonical formulation of electrodynamics in the Coulomb gauge 50 3.5 Conservation of energy and momentum; Noether’s principle 55 Chapter 4 Canonical Quantization 4.1 Introduction 61 4.2 Equations of motion 63 4.3 Photons 68 4.4 Product space for the coupled systems 83 4.5 The free field 86 Chapter 5 Symmetries and Conservation Laws 5.1 Relations between observers 96 5.2 Linear and antilinear operators 100 5.3 Continuous symmetries 102 5.4 Discrete symmetries 108 vüi CONTENTS Chapter 6 Interaction of Photons and Atoms 6.1 Approximations 119 6.2 Emission, absorption and scattering of radiation 123 6.3 Line width and level shift 138 Chapter 7 Path-dependent Electrodynamics 7.1 Introduction 147 7.2 Polarization and magnetization fields 149 7.3 Line integral Lagrangians 156 7.4 The multipolar Hamiltonian 162 7.5 Applications 169 Appendices A Values of Physical Constants 177 B Theorems in Vector Analysis 178 C Longitudinal and Transverse Vector Fields 183 D Operator Identities 185 Subject Index 187 Chapter 1 Introduction 1.1 Non-relativistic theory Quantum electrodynamics is the fundamental theory of the interaction of radiation and charged particles. It is founded on the hypothesis that the behaviour of the electromagnetic field under the influence of its micros­ copic sources is governed by the laws of quantum mechanics as well as by the Maxwell-Lorentz equations. The theory was first established by Dirac (1927) and its modern version, due mainly to Tomonaga, Schwinger, Feynman and Dyson, complies fully with the requirements of special relativity. Indeed any theory of the pure radiation field based on the source-free Maxwell-Lorentz equations must be relativistically covariant, even though it might not be expressed in a form that makes this evident. Quantum electrodynamics has, however, a well defined non-relativistic limit in so far as the motion of the sources is concerned. The non- relativistic theory is of an approximate character but involves a much simpler formalism than its relativistic counterpart. Moreover, it is applica­ ble to a wide range of problems in physics and chemistry, particularly in the areas of spectroscopy, laser physics and intermolecular forces. The conditions under which non-relativistic quantum electrodynamics provides an accurate description of phenomena will first be determined. It is assumed that the charged particles move at such low speeds (in the inertial frame of a fixed observer) that their masses can be considered as constant and equal to their rest masses. More specifically, since the relativistic mass of a particle with speed v and rest mass m0 is m0(l — v2/c2)~112, we require that vie« 1, c being the speed of light in vacuo.t This inequality generally holds for the motion of atomic particles. Thus the root mean square speed v of the electron of a hydrogen-like ion in a state with principal quantum number n is (Pauling and Wilson 1935) 27rZe2/nh, where Ze is the nuclear charge and h is Planck’s constant. If Z = 1 and t For the values of physical constants, see Appendix A.

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