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Theory and Applications of Moment Methods in Many-Fermion Systems PDF

509 Pages·1980·28.247 MB·English
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Theory and Applications of Moment Methods in Many-Fermion Systems Theory and Applications of Moment Methods in Many-Fennion Systems Edited by B.J. Dalton Ames Laboratory Iowa State University Ames, Iowa S.M. Grimes Lawrence Livermore Laboratory Livermore, California J. P. Vary AND S. A. Williams Ames Laboratory and Department of Physics Iowa State University Ames, Iowa PLENUM PRESS · NEW YORK AND LONDON Library of Congress Cataloging in Publication Data International Conference on Theory and Applications of Moment Methods in Many Fermion Systems, Spectral Distribution Methods, Iowa State University, 1979. Theory and applications of moment methods in many fermion systems. Sponsored by the Physics Department, Iowa State University, and others. Includes index. 1. Fermions-Spectra-Congresses. 2. Spectral energy distribution-Congresses. 3. Many-body problem-Congresses. 4. Moments method (Statistics)-Congresses I. Dalton, W. Bill J., 1940- II. Iowa State University of Science and Tech nology, Ames. Physics Dept. III. Title. QC793.5.F427I57 1979 539.7'21 80-21054 ISBN-13: 978-1-4613-3122-3 e-ISBN-13: 978-1-4613-3120-9 DOl: 10.1007/978-1-4613-3120-9 Proceedings of the International Conference on Theory and Applications of Moment Methods in Many-Fermion Systems - Spectral Distribution Methods, held at Iowa State University, Ames, Iowa, September 10-14, 1979. ©1980 Plenum Press, New York A Division of Plenum Publishing Corporation 227 West 17th Street, New York, N.Y. 10011 Softcover reprint of the hardcover 1st edition 1980 All righ ts reserved No part of this book may be reproduced, stored in a retrieval system, or transmitted, in any form or by any means, electronic, mechanical, photocopying, microftlming, recording, or otherwise, without written permission from the Publisher PREFACE The first international conference on "Theory and Applications of Moment Methods in Many-Fermion Systems" was held September 10 - 13, 1979 at Iowa State University. Manuscripts of the invited talks presented at this conference are the contents of this volume. These manuscripts were prepared and delivered to the editors by the authors; the responsibility for any errors in scientific con tent is theirs. While we, the editors, have made every effort to keep this volume as free from typographical errors as possible, we accept responsibility for such errors as do occur, even those which may be mistaken for scientific error. All but one of the invited talks given at the conference are reported here; those authors apparently felt unable to provide the editors with manuscripts. The editors. who also served as the organizing committee, would like to express appreciation to the sponsors of this con ference: Physics Department, Ames Laboratory, Energy and Mineral Resources Research Institute, and the Graduate College, all of Iowa State University, the National Science Foundation, and the U. S. Department of Energy. Their generosity both in terms of funding and support made the conference possible. We should also like to express our gratitude to the Interna tional Advisory Committee whose prestige lent support to the con ference and whose advice in topic selection was invaluable. Those members were: R. Arvieu Grenoble, France C. Bender Lawrence Livermore Laboratory J. B. French University of Rochester W. Fowler California Institute of Technology R. Gordon Harvard University J. N. Ginocchio Los Alamos Scientific Laboratory J. Huizenga University of Rochester A. Merts Los Alamos Scientific Laboratory J. C. Parikh Ahmedabad, India C. Quesne University Libre de Bruxelles, Belgium v vi PREFACE S. Raman Oak Ridge National Laboratory R. R. Whitehead University of Glasgow, Scotland S. S. H. Wong University of Toronto, Canada lye are also grateful to all the participants in this conference; credit for its success is theirs. Finally, we express profound gratitude to our secretary, Mrs. Pat Thiede, who took care of all the conference logistics, smoothly handled all the problems of the conference, and typed all of the manuscripts. Throughout, she had to deal with the editors which required the patience of a saint. B.J. Dalton S.M. Grimes J.P. Vary S.A. Williams CONTENTS Elementary Principles of Spectral Distribution ..... 1 J.B. French Limits of Thermodynamic Models for Nuclear Level Densities . . .. •••• 17 S.M. Grimes Statistical Properties from High Resolution Proton Resonance Reactions • . . • . . 33 G. E. Mitchell Nuclear Level Densities in Astrophysics 61 S.E. Woosley Astrophysical Opacities and Moment Methods in the Interpretation of Spectral Observation in Atomic Spectra 81 A.L. Merts Special Topics in Spectral Distributions . . . . . . . . . 91 J.B. French On the Averages of Operators in Finite Fermion Systems . • . • . 109 J.N. Ginocchio Moment Techniques in Atomic and Molecular Scattering Theory • • . . . . • • . 129 William P. Reinhardt The Representative-Vector Method for Calculating Operator Moments . . . • . . . • . . . . . 151 S.D. Bloom and R.F. Hausman, Jr. vii viii CONTENTS Phenomenological Approach to Nuclear Level Densities ••.••.•••• 167 G. Reffo Stieltjes-Tchebycheff Moment-Theory Approach to Photoeffect Studies in Hilbert Space 191 P.W. Langhoff Polynomial Expansions and Transition Strengths •••••••••• 213 J.P. Draayer Moment Methods and Lanczos Methods • . • • • • • • • • •• 235 R.R. Whitehead Spectral Distributions and Symmetries 257 . C. Quesne Calculation of Spin Cutoff Parameters using Moment Techniques •••.••••• 273 S.M. Grimes Group Symmetries and Information Propagation • • • • • •• 287 J.P. Draayer Level Densities in Nuclear Physics • • . . • • • • . . •• 307 M. Beckerman Spectral Methods Applied to Ising Models . • • • • • • •• 327 B. DeFacio, C.L. Hammer, and J. Ely Schrauner The Partition Function as a Laplace Transform of a Positive Measure in the Strength Parameter • . . . . • • • 363 D. Bessis Application of Spectral Distributions in Effective Interaction Theory • • • 371 B.D. Chang Beta Decay and Strength Distributions 389 J.C. Hardy Study of Effective Interactions and Models in Nuclei Using the Moment Method • • • 405 Jitendra C. Parikh CONTENTS ix Realistic Hamiltonians for No-Core Moment Methods Studies • . • . . . . . 423 J.P. Vary Fixed-J Moments: Exact Calculations 437 C. Jacquemin Radial Densities of Nuclear Matter and Charge Via Moment Methods . . • •• .• . • 451 B.J. Dalton Sum Rules, Strength Distributions and Giant Resonances ...•••••.•.•. 463 O. Bohigas Part ic ipant s 499 Index 505 ELEMENTARY PRINCIPLES OF SPECTRAL DISTRIBUTIONS J. B. French Department of Physics and Astronomy University of Rochester Rochester, N.Y. 14627 I. INTRODUCTION It is a common observation that as we add particles, one by one, to a "simple" system, things get steadily more and more com plicated. For example if the system is describable in shell-model terms, i.e., with a model space in which m particles are distributed over N sinrle-particle states, then, as long as m« N, the dimen- l:) sionality increases rapidly with particle number. On the other hand, for the usual (l+2)-body Hamiltonian, the (m~2)-particle spectrum and wave functions are determined by operators defined in the one-particle space (for the single-particle energies) and the two-particle space (for the interactions). We may say then that the "input" information becomes more and more fragmented as the particle number increases, the fixed "amount" of information being distributed over more and more matrix elements. On the other hand there arise also new simplicities (Fig. 1) whose origin is connected with the operation of statistical laws. There is a "macroscopic" simplicity corresponding to ¢e fact that the smoothed spectrum takes on a characteristic shape1 defined by a few parameters (low-order moments) of the spectrum. There is a "microscopic" simplicity corresponding to a remarkable spectral rigidity2 which extends over the entire spectrum and guarantees us that the f1ucutuations from uniformity in the spectrum are small and in many cases carry little information. The purpose of spectral-distribution theory, as applied to these problems, is to deal with the complexities by taking advantage of the simplicities. 2 J. B. FRENCH To make clear what we mean by a "spectral distribution" we consider a few examples: 1) H-Eigenvalue Distribution: PE(x) defines the density of eigen values of H acting in the model space; for finite spaces we take JPE(x)dx = 1 so that a dimensionality factor d(m) is needed for the true state density I(x). Then the moments of PE are ~ = JPE(x)xPdx= <HP>m where, for any operator G, d(m)x<G>m:: «G»m is the trace of G over the model space (or over the m-particle space as the case may be). From the standpoint of statistical mechanics PE(x) and the partition function Z(8) are related by Laplace transformation, and therefore carry the same information; PE(x), which is to s~me extent measurable, is more convenient for us. From p, aA a 6un~on 06 the p~met~ 06 the ~y~tem, we should be able to determine most things of interest about the system, just as one can from the par tition function. The complete evaluation is in general out of the question but we shall be able to calculate a smoothed version of p, and deal with the deviations by introducing an appropriate ensemble. Thus P = Psmoothed + Pfluctuation (1) in which our main interest will be in the first term, for which we shall drop the subscript label. From the smoothed density we can, as first done by Ratchiffl , recover a (smoothed) spectrum by re placing the smoothed distribution function F(x) = JXp(z)dz by a staircase function with jumps of magnitude d-l at x values for which F is half-integral; an example is given in Fig. 1. An obvious extension is called for if the spectrum has known degeneracies. 2) Expectation-value Distributions: We might be interested in the expectation value of an operator K in the ~amiltonian eigenstates, i.e. in <~E K ~E> = K(E) say, or of H in J eigenstates, etc. The second example would come up in dealing with the J-decomposition of the level density. Figure 1. The upper fieure shows a computer histogram of a (ds)12, J=T=O spectrum for a "realistic" Hamiltonian. The di mensionality is 839. The bins are 1.7 MeV wide, and the Gaussian values are indicated by oval points. The lower figure shows a comparison between the exact shell-model spectrum and the smoothed spectrum generated by using a four-moment distribution. Two segments of the spectrum are shown, for levels 1-23 and 503-524. In each case the exact spectrum is to the left.

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