SCIENTIFIC ABSTRACT TERNOV, I.M. - TERNOVENKO, N.M.

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December 31, 1967
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SCIENTIFIC ABSTRACT
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S 07/56 - 2 A -:z - xe '7 1 On the Problem of the Covariant Determination of the Spin-pseudovector It further holzls that . k F7-87V Cos 6'P k Y 1-0, ' sin 6, 1 0 ~2 - 0 ~ ~3 - ks, ~4 - ikal several special cases are investigated. There are 7 references, 6 of which are Soviet. ASSOCIATION: Moskovskiy gosudarstvennyy universitet (Moscow state University) SUBMITTED: October 27, 1958 Card 2/2 TMOV, I.M.; TLTIIANDV. V.S. Effect of vacuum fluctuations on the polarization of electrons moving in a magnetic field. Zhur.el-spA teor.fiz. 37 no.4-- 1137-1139 0 159. OIRA 13 -.5 1. Moskovskly gosudarstvewiyy universitet. (Electrons) (Magnetic fields) 9(3),24(4) AUTHORS: Ternov, I. M,, Tumanov, V. S. SOV/20-124-5-21/62 TITLE-. On the Radiation of a Polarized Electron (Ob izluchenii poly- arizovannogo avetyashchegosya elektrona) PERIODICAL: Doklady Akademii nauk SSSR, 1959, Vol 124, Nr 5, pp 1038-1041 ('USSR) ABSTRACT: The authors investigated the radiation of a polarized rela- tivistic electron in a constant and homogeneous magnetic field. In this connection it is useful to demand that the wave function of the electron moving in the magnetic field A - 0 be a solution of the = -(1/2)yH, A = (1/2)xH, A x z Y Dirac equation and, besides, an eigenfunction of the operator of the spin Iro ction on the kinetic momentum: CC + -'P- A)~ It is useful to make such a P)+ - 6(-V C selection of the wave function because the orientation of the spin of the electron with respect to the direction of its motion in a magnetic field remains conserved. The steady solution of the Dirac equation in the system of coordinates Card 1/3 r, 1, z is explicitly written down. An expression for the On the Radiation of a Polarized Electron SOV/20-124-r-21/62 polarized radiation of the electron at its spontaneous tran- sition from the initial to another state in written down. The matrix elements of the Dirac matrices are proportional to certain Laguerre-functions. The authors above all estimate the intensity of radiation at transitions with approximation of the polarization of spin, The intensity of the radiation which is connected with depolarization is much lower than the corre- sponding value for transitions with conservation of polariza- tion. For the investigation of the angular distribution of radiation intensity the usual approximation of matrix elements must be carried out, and the above-mentioned expression for the intensity of the polarized radiation of the electron must be summated with respect to all harmonics and radial transi- tions. Next, rather long expressions are derived also for the integral intensity of radiation. The p6larization of the electron manifests itself already in the terms of the order of magnitude -P , although the radiation with the re-orienta- tion of spin is of the order *-2. The authors thank 11rofessor A. A. Sokolov and Professor D.' D. Ivanenko for discuosing the problem and its results. There are 7 Soviet references. Card 2/3 On the Radiation of a Polarized Electron SOV/20-1124-5-21/62 ASSOCIATION: Moskovskiy gosudarstvennyy universitet im. M. V. Lomonosova (Moacow State University imeni h. V. Lomonosov) PRESENTED: October 31, 1958s by N. 11. Bogolyubov, Academician SUBMITTED: October 24, 1958 Card 3/3 69-45 3 S/139/6o/ooo/ol/027/041 $13 0 E032/E4 III AUTHORS% Ternov, I.M. and Tumanov, V,,S. TITLE *. '_0_n__th-e-1Td1-t-u~f Polarized Electrons in a Magnetic Fielak PERIODICAL: Izvestiya vysshikh uchebnvkh zavedeniy, Fizika, 1960, Nr 1, PP 155-163 (USSR) ABSTRACT-. It is well known that the effect of electromagneti,~l fields on the motion of a polarized electron beam , an, in the general case, be reduced to a change rn-the momentum and the direction of the spin vector. In the case of a purely magnetic field, this change takes place in such a way that the component of' the spin vector in the direction of motion is conserve(L The situation is however complicated by the interaction of the electron with the electromagnetic vacuum, This leads to an additional energy which should be included in the generalized Dirac equation. A consideration of the effect of the vacuum inter-action energy shows that in the non-relatiViStLC Aj)j)r0XtMati0n, the electron has a vacuum magnetic moment (in addition to the Bohr magnoton) Card 1/3 so that the Hamiltonian in the generalLzed Dirac 1-f 4r,4-- A I I - S/139/60/000/01/027/o4i E032/Elii4 On the Motion of Polarized Electrons in a Magnetic Field equation for an electron in the magnetic field is of the form given by Eq (3), The presence of the additional vacuum moment leads to the fact that the change in the momentum vector and in the spin direction, when the electron moves in a magnetic field, is such that the spin component in the direction of motion is no longer an integral of motion, since the operator (uP) no longer commutes with the Hamiltonian of' the generalized Dirac equation. In this way, the original polarization of the electron beam gradually changes with time, The vacuum intelraction plays the major part in the change in the polarization since the kinematic (non-vacuum) part of the magnetic moment is automatically taken into account by the Hamiltonian given by Eq (2) and has no effect on the polarization, The vacuum corrQctiott to the Dirac equation (Eq (3) ) in the form of an additional field moment is only significant in the non-relativistic approximation, The relativistic problem must he Card 2/3 considered separately and this is done in 50MC detail in 69i~ ~' 3 S/139/60/000/01/027/041 E032/E414 On the Motion of Polarized Electrons in a Magnetic Field the present paper. The treatment given holds up to ultra-relativistic electron velocities, The derivation is given of radiational corrections to the Dirac equation, and the effective energy of interaction of an electron with vacuum is computed, An estimate is also given of the change in the orient-ation of the electron spin vector which is due to the vacuum interaction,, The discussion is concluded with an example in which the electron moves in a direction perpendicular to the magnetic field. Acknowledgement is made to Professor A.A,Sokolov for disc-iision of the results obtained. There are 10 referen,_*,-r, 0 of which are Soviet and 4 English, ASSOCIATIONtMoskovskiygosuniver.4i.tet imeni M.V.Lomono1jova (Moscow State University imeni M,V,Lomonosov SUBMITTEDs July 234 1959 Card 3/3 S/139/0/000/0i/o/jo/oli 1 F AUTHORS, Voroblyev. A.A., and Ternov, JL'Q -391 TITLE- lilt ernati_9nal Confnr ince on Hi-i-h-ener-gy Partic-le AcceloriAtors and on.- 1X_UUU'11La"o11 A PERIODICAL: Izvestiya vysshikh uctiebny1ch zaveder?iv, Fizi1ra. 1960, Nr 1, pp 2~6 - 2111 (USSR) ABSTRACT: The conference was opened by the Chairman of CERIN, Dr. Rnker, At the first session four papers were read on the necessity of building new high-energy accelerators. Ono of these papers was read by Professor Panovskiv, who argued that large accelerators give no information i-rhich could not be obtained from cosmic rays,, The evening session on September 14 and two sessions on September 15 were occupied by twenty-one papers on extension of the accelerator energies towards higher values. During these sessions papers -ere prezented by Kolomenskiy, V~P. Dmitriyevskly (descriptxon of a 12 MeV cyclotron i-n Dubno, which uses spatial variation of the magnetic f.Leld) and Cardl/4 ~X S/139/6o/ooo/oi/oWo4i International Conference on tiigii-L-iiergyF-'P"Da'r~'L2~o' Accelerators and on Nuclear-physics Instrumentation V.I. Zamolodchtkov (description of a 1.5 m cyclotron with azimuthal variation of the magnetic field), The morning sess-ion on September 15 included 7 papers on acceleration of charge5 in plasmas,.IL-I among the3e were pApers by Rodionov, Academician I.F. Kvartskhava (experimental LtivestigatiOnS Of f)I-OdUCtI.On and acceleration of plarnas), Academician (coherent shock acceleration of ring plasmas), A.N. Lebedev and A.A, Kolomenskiv (theory of stochastic acceleration and accumulation): A.A. Vorob~vpv dreur the attention of the conforence T.0 tile Absence Of PIT)erS On inj ec t ion. The morning session on September 16 was devoted to fundamental limitations of accelerator4j. 7 Among the papers presented at this session there were communications from D.G. Koshkarev (theory of non-linear problems of betatron oscillations and particles losses in resonances); V.V- Vladimi-rskiv (space-charge limitations), Card2/4 Lebedev, Finkel,shteyn and Veksler~ 6'4~,A 0- S/139/60/000/01/0110/0"1 International Conference on Accelerators and on Nuclear-physics Instrumentation Another group of papers dealt with departure from cyclic acceleration of electrons due to radiat-i.on and quantum of f (3c. 1, t3 (A.N. 1.0)4~dov and D.G. Komhkarov in this group). At the evening session on September 16, twelve papers were presented which described technical details of high- energy accelerators. The 7 BeV proton synchrotron in Moscow and % planned 50 BeV synchrophasotron i.n Serpukhov were descri.bed by V.V, Vladimir6kly. Engineer_Zinov~y*v -described -)0, 90 and 200 'MeV linear electron accelerators, constructed at UFT1. A.A. Voroblyev- read a paper on "The Theory of Cyclic Waveguide, El.ectrcn Ar~celerator,3", based on his own work and that of A.N. Didenko, Ye.S, Kovalenko and 13,N.Morozov, At the morning sessicn on September 17, devoted LC Card3/4 ztt, M 1~ !W- MITI S/139/60/ooo/01/040/041 International Conference an H_igh-energEY2%1dR21a Accelerators and on Nuclear--physics Instrumentation production, extraction and high-energy machines, papers (formation of a meson beam Dubno synchrophasotron) and kmicrowave separation of separation of particles in were read by S.V. Chuvilo of 7 BeV/c momentum in the by Professor Panovskiy particles). ASSOCIATIONS: Moskovskiy gosuniversitet irieni M.V. Lomonosova (Moscow StatE University imeni M. V. Lomonosov) Toms kx;7~o_f -it ek-lin L c lies ki y institut imeni S.2,L Kirova (Tomsk Polytechnical. Institute imeni S.1M. Kir SUBMITTED- December 11, 1959 Card 4/4 ACCESSION NR: AP4041444 s/0188/64/000/003/0101/0103 AUTHOR: Sokolov, A. A.; Te=ov. I. X.; Loskutov, YU. X. TITLE: The problem of radiation damping of betatronic oicillations SOURCE: Moscow. Universitet. Vestnik. SeriYa 3. Fizika, astronomiya, no- 3, 1964, ICI-103 TOPIC TAGS: betatron, betatronic oscillation, cyclic accelerator, radiation damp- ing, quantum theory, cyclic electron accelerator, electron accelerator, electron radiation, electron oscillation, electron motion, parabolization ABSTRACT: After the demonstration of the influence of quantum fluctuations of radiation on the movement of electrons In a cyclic accelerator, the development of the quantum theory of electron movement acquired theoretical and practical signi- ficance. Recently, in a paper by S. A. Kheyfets and Yu. F. orlov (ZhETF, 45, 1225, 1963), an attempt was made to obtain not only fluctuation activation of betatronic oszillations, but also classical damping using a nonrelativistic approximation in addition to the quantum method. These authors feel that one cannot obtain radia- tion damping In elthor the classical.case or the quantum case because quadratic terms in rand dr are neglected in the equations of movement, i.e. "paraboliza- ,Card_, 1/3 d-t ACCESSION NR: Ap4o41444 tion" of the potential energy describing the betatronic oscillations is carried out. The present authors then point out that."parabolizatioWl of the potential energy actually takes place In both the classical and quantum calculations. Never- theless, in spite of the assertions of S. A. Kheyfets and Yu. F. Orlov, with the help of the classical theory the authors at once found an expression fo5 radiation damping: x+ 0~x_ q x+j i-They then review'their previous work on the application of quantum theory to the excitation of betatronic oscillations, and show that the criticism of Kheyfets and Orlov concerning the origin of classical damping cannot be applied to the ultra- 'stic case of "free!' betateonic oscillations. Atte tion is'-drawn, in this relativi n connection, to the work of Gutbrod (Zs. f. Phys., 168, )77, 1962). Taking into account all the terms of the analysis, one can obtain the following expression for the change in.the quantum number s; dl 48 -/_3 Rla%0 (I - q)y- (2) where WkI Is the classical 'expression for the energy'being radiated In a unit of Cwd 2/3 ACCESSION NR: AP4041444 time. In conclusion, the authors remark that the quantum fluctuations of the radius have great practical significance. in this regard, If the first quantum term in the right hand side of equation (2), corresponding to the quantum fluctu- ations, Is neglected, then the square of the amplitude of the radial fluctuAtions rapidly vanishes in the presence of relatively large energies. Acutally- however, the amplitude.of the vertical or axial oscillations tends toward a sm4II positive limit. It also follows that the effect of classical damping begins to decrease at' energies on the order of 400-600 Mev. The article is followad by a brief rebuttal by S. A.,-Kheyfets. Orig. art. has: 9 formulas. ASSOCIATION: Kafedra tooratichaskoy fiziki Moskoviskogo universiteta (Department, I of Theoretical Physics, Moscow University) SUBMITTED: 07Dec63 ENCL: 00 SUB CODE: NP NO REF SOV: 007 OTHER: 003 Crd 3/3 --431MM T 17 1 T IT. ~T~ ~T ACCESSION NR: AP4043800 S/0188/G4/000/004/OOGZ/0070 AUTHOR: Ternov 1. At., Bagrov, V. G., Rzayev, R. A. TITLE: Influence of synchrotron radiation of electrons on their spin orientation SOURCE: Aloscow, Universitet. Vestnik. Seriya 3. Mika, astronornlya, no. 4, 1964, 62-70 TOPIC TAGS: electron, magnetic field, synchrotron radiation, electron spin, electron spin polarization, electron spin orientation ABSTRACT: The influence of an electromagnetic field on the movement of a polarized beam of electrons generally leads to a change in both the momentum vector of the particles and their spin orientation. In the case of a magnetic field which Is uniform in space and consLant in time this change occurs in such a way that the state of polarization of the electron spin, determined relative to the direction of motion of the electron and relative to the direction of the external magnetic field, doesnotchango with time. During motion in a magnetic field an electron becomes a source of extremely strong clectromag- netic radiation which can lead to a change in the orientation of electron spin. In this article the author considers the problein of the behavior of electron spin during synchrot- rorvgdiation. Two states of polarization are investigated: relative to the directioa of Cord ACCESSION NR: AP4043800 motion (longitudinal) and relative to the direction of the magnetic field (for practical purposes transverse). Expressions are derived for the wave functions, followed by an analysis of the probability of spontaneous transitions. In his exposition of the formulas characterizing spectral distribution, the author cites dy F. AC 'R 0 + U? where F is dependent on the state of polarization of thb electron spin. The state of longitudinal polarization is F- - (2 (1 + ~Iylj (x) dx, (2) (3) F" ~10'2K% (y) - X~,, (x) dx) where arrows indicate transitions corresponding to spin flipping and without change ,,in spin orientation (4). These formulas show that transition probability is gonerall 4 E1/2 / (that Is, independent of the inItial state of polarization. In the case E, whenUi). Cord 2/5 ACCESSION NR: AP4043800 spin flipping is expressed in terms proportional to the square of the Planck constant 112. The state of polarization along a magnetic field Is (4) T". 2 (1 + ZY) (x)) dx + VyW% (y) - C. (2 + jV) (5) Y'(I(,/.(Y) t;K%(tM- where the arrows indicate retention of polarization and change of polarization (spin flipping). The results differ appreciably from the preceding case: dependence on initial spin state enters into both expressions. Limiting the problem to the region of energies E