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Particles and Nuclei: Volume 1, Part 2 PDF

196 Pages·1995·6.022 MB·English
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PARTICLES AND NUCLEI Volume 1,. Part 2 PARTICLES AND NUCLEI Volume 1, Part 1 Elastic Scattering of Protons by Nucleons in the Energy Range 1-70 Ge V V. A. Nikitin Probability Description of High-Energy Scattering and the Smooth Quasi-potential A. A. Logunov and O. A. Khrustalev Hadron Scattering at High Energies and the Quasi-potential Approach in Quantum Field Theory V. R. Garsevanishvili, V. A. Matveev, and L. A. Slepchenko Interaction of Photons with Matter Samuel C. C. Ting Short-Range Repulsion and Broken Chiral Symmetry in Low-Energy Scattering V. V. Serebryakov and D. V. Shirkov CP Violation in Decays of Neutral K-Mesons S. M. Bilen'kii Nonlocal Quantum Scalar-Field Theory G. V. Efimov Volume 1, Part 2 The Model Hamiltonian in Superconductivity Theory N. N. Bogolyubov The Self-Consistent-Field Method in Nuclear Theory D. V. Dzholos and V. G. Solov'ev Collective Acceleration of Ions E. I. N. Ivanov, A. B. Kuznetsov, A. Perel'shtein, V. A. Preizendorf, K. A. Reshetnikov, N. B. Rubin, S. B. Rubin, and V. P. Sarantsev Leptonic Hadron Decays E. I. Mal'tsev and I. V. Chuvilo Three:Quasiparticle States in Deformed Nuclei with Numbers between 150 and 190 (EfT) K. Va. Gromov, Z. A. Usmanova, S.1. Fedotov, and Kh. Shtrusnyi Fundamental Electromagnetic Properties of the Neutron Yu. A. Aleksandrov Volume 2, Part 1 Self-Similarity, Current Commutators, and Vector Dominance in Deep Inelastic Lepton-Hadron Inter actions V. A. Matveev, R. M. Muradyan, and A. N. Tavkhelidze Theory of Fields with Nonpolynomial Lagrangians M. K. Volkov Dispersion Relationships and Form Factors of Elementary Particles P. S. Isaev Two-Dimensional Expansions of Relativistic Amplitudes M. A. Liberman, G.1. Kuznetsov, and Va. A. Smorodinskii Meson Spectroscopy K. Lanius Elastic and Inelastic Collisions of Nucleons at High Energy K. D. Tolstov PARTICLES AND NUCLEI N. N. Bogolyubov Editor-in-Chief Director, Laboratory for Theoretical Physics Joint Institute for Nuclear Research Dubna, USSR / A Translation of Problemy Fiziki Elementarnykh Chastits i Atomnogo Yadra (Problems in the Physics of Elementary Particles and the Atomic Nucleus) Volume 1, Part 2 ® CONSULTANTS BUREAU • NEW YORK-LONDON • 1972 Editorial Board Editor-in-Chief N. N. Bogolyubov Associate Editors A. M. Baldin Nguen Van Heu V. G. Solov'ev Secretary I. S. Isaev K. Aleksander N. Kroo D. I. Blokhintsev R. M. Lebedev V. P. Dzhelepov M. M. Lebedenko G. N. Flerov M. G. Meshcheryakov I. M. Frank I. N. Mikhailov V. G. Kadyshevskii S. M. Polikanov Kh. Khristov Shch. Tsitseika A. Khrynkevich A. A. Tyapkin The original Russian text, published by Atomizdat in Moscow in 1971 for the Joint Institute for Nuclear Research in Dubna, has been revised and corrected for the present edition. This translation is published under an agreement with Mezhdunarodnaya Kniga, the Soviet book export agency. PROBLEMS IN THE PHYSICS OF ELEMENTARY PARTICLES AND THE ATOMIC NUCLEUS PROBLEMY FIZIKI ELEMENTARNYKH CHASTITS I ATOMNOGO YADRA n p06J1eMbi IjJH3HKH 3J1eMeHTapHblX 'faCTH~ H aTOMHoro HApa Library of Congress Catalog Card Number 72-83510 ISBN-13: 978-1-4684-7661-3 e-ISBN-13: 978-1-4684-7659-0 DOl: 10.1007/978-1-4684-7659-0 © 1972 Consultants Bureau, New York Softcover reprint of the hardcover I st edition 1972 A Division of Plenum Publishing Corporation 227 West 17th Street, New York, N. Y. 10011 United Kingdom edition published by Consultants Bureau, London A Division of Plenum Publishing Company, Ltd. Davis House (4th Floor), 8 Scrubs Lane, Harlesden, London NWlO 6SE, England All rights reserved No part of this publication may be reproduced in any form without written permission from the publisher CONTENTS Volume 1, Part 2 Eng'/Russ. The Model Hamiltonian in Superconductivity Theory-N. N. Bogolyubov ........... . 1 301 The Self-consistent-Field Method in Nuclear Theory -R. V. Dzholas and V. G. Solov'ev ............ , ............................ . 53 390 Collective Acceleration of Ions-I. N. Ivanov, A. B. Kuznetsov, E. A. Perel'shtein, V. A. Preizendorf, K. A. Reshetnikov, N. B. Rubin, S. B. Rubin, and V. P. Sarantsev . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 71 391 Leptonic Hadron Decays - E. I. Mal' tsev and I. V. Chuvilo .................... . 105 443 Three-Quasiparticle states in Deformed Nuclei with Mass Numbers between 150 and 190 - K. Ya. Gromov, Z. A. Usmanova, S. I. Fedotov, and Kh. Shtrusnyi. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 159 525 Fundamental Electromagnetic Properties of the Neutron-Yu. A. Aleksandrov ...... . 170 547 THE MODEL HAMILTONIAN IN SUPERCONDUCTIVITY THEORY N. N. Bogolyubov A system of fermions with attraction described by the model Hamiltonian in superconduc tivity theory with separable interaction is considered. Asymptotically exact estimates (as V - 00) for the minimal eigenvalue of the Hamiltonian, correlation functions, and Green's functions are obtained. § 1. Statement of the Problem The simplest model system considered in superconductivity theory is characterized by a Hamiltonian in which only the interaction between particles having opposite momenta and spins is retained: H -- .~..;. T(t)a,+ af- 2VI .,~. A(f)A(j , )a,+ a+_, a_f, a,., (1.1) f f. f' where j = (p, s), s = ±1; p is the momentum vector. For fixed v= L3, 2lt PZ=L nz, nx' ny, nz are integers; -j = (-p, -s). Finally, TV) = (p2/2m)-!l, where!l > 0 is the chemical potential, -Ill J'B(S) for I :: ~~, A(f) = ( o I ::- Ill>~; for E (s) = ± I, J = const. The application of the Bardeen-Cooper-Schrieffer method [1] and the method of compensation of dan gerous diagrams leads to the identical result in the case given. Moreover, in [2] it was shown that a Ham iltonian of the type (1.1) is of great methodological interest, since here we have one of the very few com pletely solvable problems in statistical physics. In the paper mentioned it is established that for this problem we may obtain an asymptotically exact (for V - 00) expression for the free energy. This result was found there in the following manner. The Hamiltonian (1.1) was partitioned into two parts Ho and H1 in a special manner. The problem with the Hamiltonian Ho was solved exactly. Perturba tion theory was used to consider the effect of H1• It was shown that any n-th term of the corresponding ex panSion becomes asymptotically small for V-oo, in connection with which it was concluded that the effect of H1 may in general be neglected after the transition in the limit V-oo. Of course, reasoning of this kind ,. Joint Institute for Nuclear Research, Dubna. Translated from Problemy Fiziki Elementarnykh Chastits i Atomnogo Yadra, Vol. 1, No.2, pp.301-364, 1971. Cl1972 Consultants Bureau, a division of Plenum Publishing Corporation, 227 West 17th Street, New York, N, Y. 10011, All rights reserved, This article cannot be reproduced for any purpose whatsoever without permission of the publisher. A copy of this article is available from the publisher for $15.00. 1 cannot pretend to mathematical rigor, but it should nevertheless be underlined that in statistical physics problems still cruder devices are often used. For example, approximate methods based on selective sum mation of "principal terms" (in some sense) of the perturbation-theory series are very widely used; here the remaining terms are discarded even though they do not vanish even for V- 00. Doubts of the validity of the results of [2] also arise in connection with the fact that various attempts I-I at using conventional Feynman diagram techniques (without allowance for "anomalous pairings" at a-f' I-I a2:f at. to which canonical 11-, v-transformation leads) did not yield the expected result. Furthermore, based on the summation of a certain class of Feynman diagrams, Prange [3] obtained a solution which dif fered in principle from the solution obtained in [1. 2] and assumed that the latter papers were wrong. In [4] a study was made of a chain of linked equations for the Green's function without the use of per turbation theory. It was shown there that the Green's function for the Hamiltonian Ho satisfied this entire chain of equations for the exact Hamiltonian H = Ho + Hl with an error of order 1/V. This substantiates the results of [2] and reveals the "inefficiency" of the correction H1• However, one can also dwell on the purely mathematical point of view. As soon as we have fixed the Hamiltonian, say in the form (1.1), we have an already fully defined mathematical problem which should be rsolved rigorously without any "physical assumptions." In this case, the approximate expressions satisfy the exact equations with an error of order 1/V, and we should estimate the difference between the most exact and approximate expressions. Having in mind complete parity in the problem of the behavior of a dynamic system having the Hamil tonian (1.1), we shall take precisely such a purely mathematical viewpoint in this paper. We shall study the Hamiltonian (1.1) at a temperature () = 0 and demonstrate rigorously that the rela tive difference (E-Eo) lEo between the lowest energy levels Hand Ho' and likewise between the correspond ing Green's functions, tends to vanish for V - 00; we shall obtain estimates for the order of decrease. Based on .methodological concepts it is convenient to cons ider a somewhat more general Hamiltonian containing terms which represent sources of creation and annihilation of pairs: 3f=.v., .T(f) a,+ a,-'Y~~- 2A -(f)( a_,a,+a,+ a+_I) -2V1 ~~,,.. <f) ,1. . (t')a ,+ a+_I a_I' a,., (1.2) " '0 l' where v is a parameter which we shall assume to be greater than or equal to zero. Let us note that the case v < 0 need not be considered, since it can be reduced to the case v> 0 by a trivial change in the gauge of the Fermi operators: + . + a, --+ -1 a, . Let us emphasize the fact that the case v >0 will be considered exclusive of those notions that it is of in terest in understanding the situation in the actual case v = o. For the investigation undertaken we shall not need those specific properties of the functions ?.(f), T(f) of which we spoke above. It will be quite sufficient if the following general conditions are satisfied: 1) the functions ?.(f) and T(f) are real, piecewise continuous, and have the ~ymmetry conditions A(-f)= -AU); T (-f) = T (f); 2) ?.(f) is uniformly bounded throughout the entire space, and T(f)-oo for Ifl-oo; 3) ~ ~ IA(f)I~const for V-oo; V I 2 4) lim J..- ~ A' (f) > I for sufficiently small positive x. v .... oo 2V f YA2 (f) x+ T' (f) Let us represent ;;e (1.2) in the form (1.3) where (1.4) (1.5) Here u is a certain complex number. Let us note that if u is determined from the condition for the minimum of the least eigenvalue {ffo, while {f{l is discarded, we arrive at the well-known approximate solution which was considered in [1,2,4]. Here our problem will consist in finding the estimates for the deviation of the minimal eigenvalues 3(0, J£ and for the deviation of the corresponding Green's functions. Let us show that these deviations will vanish in the process of the transition in the limit V- 00.* § 2. The General Properties of the Hamiltonian 1. In this section we shall establish certain general properties of the model Hamiltonian ;;e (1.2). Let us consider the occupancy numbers nj = ajaj and let us show that the differences nj-o._j are integrals of motion. Actually, and likewise therefore, Consequently, ddt (n, (I) - n_, (I)) = O. (2.1) 2. Let us show that for the wave function <D .Yt', corresponding to the least eigenvalue of the Hamil tonian ;;e, we may place (2.2) for any j. In order to prove this let us assume the opposite. Since (nj-n-j) commutates with;;e (and with one another) one can always choose <D.1t' in such a way that it is an eigenfunction for all these operators: * Recently papers have appeared [7-12] in which new methods have been developed for finding asymptotically exact expressions for multitemporal correlation functions (Green's functions) in the case of arbitrary tem e. peratures Estimates were likewise constructed for finding expressions for the free energies in model systems of the BCS type which are exact for v-co. Based on an analysis and generalization of the papers, it was possible to formulate a new prinCiple-the minimax principle [12]-for an entire class of model prob lems in statistical physics. 3 Let us use Ko, K_, K+, respectively to denote the ensemble of subscripts f for which (n,-n_,) cD.:ft' = 0, f E Ko; (n,-n_,- I)CD.rt=O, f EK+; (n,-n_,+ 1) cD.rt =0, f EK-. This assumption can be reduced to the proposition that the sets K+, K_ are not empty and that* for any function cp. Further we shall require that cp satisfy the additional conditions (2.3) Let us note now that if f E K+, then nf =1 , I1-f =0 , while if f E K_, then nf =0 ; n_f =1 . Therefore, cD.rt may be represented in the form of the direct product where while cI>Ko is a function of only those nf for which f E Ko: cDx.=F( ... n, ... ); (cDt,cDx) = 1, fEKo' Let us note further that a_, a, 6 (n,- 1) 6 (n_,) = 0; a_, at 6 (n,) 6 (n_,- 1) = 0; at a~t 6(n,-I) 6(n_f)=0; at a~f b(nf) 6(n_f-l)=O, and therefore that if f E K+ for K_. Consequently, And thus, * The symbol <cI>*w> will be used to denote the scalar product of the functions cI> and w. 4 --V1 "~" """ A(f)A(f,) a,+ a+_ ,a_"ar }cDK"/, 2 fEKo,'EK, 0 Let us now partition the set K+ + K_ into two sets in such a way that Q+ will include those subscripts j from K+ + K _ for which T(f) 2: 0, while Q_ will include those subscripts from K++ K_ for which T(f)< o. In view of the symmetry of T(f) = T(-j) the subscript j will always be included in Q+ and Q_ simultaneously with -j. We have +/"< DK. 'II "~" T (t)nf- -\I "~" /1i oU ) (a_f a,+ a+f a+_ f) fEK, 2 fEK, Let us now construct the function q; likewise in the form of a simple product, having placed where (Here it is preclsely essential that j belong to Q+ or Q_ simultaneously with -j.) For such a function As is evident, On the other hand, the method of construction of q; satisfies all of the additional conditions (3), and we have arrived at a contradiction with Eq. (2). Thus, our statement has been proved. From the statement (2.2) it follows, in particular, that the total momentum for cD 3t' is equal to zero: (2.4) As is evident from what has been said earlier, the eigenfunction cJ> for the least eigenvalue :Je may always be sought in the class of functions q; which are governed by the additional conditions (2.3). Let us note that for this special class of q; satisfying the conditions (2.3) the Hamiltonian :Je may be expressed in terms of Pauli amplitudes. Let us consider the operators bf = a_f af; b+f = a+f a+_ f' 5

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