SCIENTIFIC ABSTRACT PAFOMOV, V.YE. - PAGAVA, G.D.

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CIA-RDP86-00513R001238720018-9
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S
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100
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January 3, 2017
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August 1, 2000
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December 31, 1967
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SCIENTIFIC ABSTRACT
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PAFOMOV, V-ye- Izv. vys-,--ucheb zav; Transient radiation in the-case of oblique- (14115:7) radiofiz. 5 n0-394&01489 '62- nst tut imenj p.p.jabodeva AN SSSR. 1, FizicheskiY i (Faectrowmetic waves ,~-~Ov ~Iv - Y~- - ng throUgh DlatOG, Zb=f Radiation from a charged particle movi (MIRA 13:12) eksp. i teor. fiz. 39 no. 1:134-137 11 16o. 1. Fizicheskiy institUt imeni P.N. Lebedeva AN SSSR- (Blectron optics) 84701 S/02 60/133/006/003/016 0 J/-? R 2-) B019YB054 AUTHOR: Pafomov, V, Yes. TITLE: Influence of Multi le Soatte-4-- on Transition Radiation PERIODICAL: Doklady Akademii nauk SSSR, 1960p Vol. 133, No. 6, PP. 1315-1316 TEXT: In the introduction, the author briefly explains the generation of transition radiation during the motion of charged particles through the interface.of two media. He points to the increase in energy of transition radiation which in the relrAivistio case is proportional to the incTease in energy of particles, and describes the production of transi- tion radiation quanta. He studies the motion of a point charge through the surface separating a medium from the vacuum; he proceeds from formula (1) for the amplitude of the spherical wave field of transition radiation. Here$ the field amplitude is proportional to the path length difference of the coherent interaction of particles with the waves in the vacuum and in the mediumt which depends on the angle between the direction of wave propagation and the direction of motion of particles. With the use Card 1/3 84701 Influence of Multiple Scattering on Transition B/020/60/133/006/003/016 Radiation B019/BO54 2 2N/m, 0 G) E/Po2, and Co # , E 2E2.4,.)4L, of the definitions 6) 0 47te or - 0 6 or a where E is the total energy of particlesp E 9 - 21410 evv ji -the rest mass of the particles, and L the unit of radiation length, as well as Et 0 2)3/E2, (6)0 L/O)-(Ao a the author derives a formula for the cases B smaller than Ef, formula (7) for E >> El, formula (8) for E > El, and a formula for the spectral densities of the radiation energy for B - El. Prom these investigations it appears, among other things, that for frequencies 6j< Wor the field of transition radiation is mainly formed on the way in the vacuum. Thus, multiple scattering does not reduce the probability of emission of transition quanta. Multiple scattering is of considerable importance if, on the way s V - C/W(F,/pe 2)2 of the coherent interaction of particles with the waves in the vacuum, the particles move out under the angle 0 - go 2/Eq In this case, new frequenciesq for which G) < Q < (j * holds, appear in the spectrum. Further, El is the particle or or Card 2/3 84701 Influence of Multiple Scattering on Tranaition 8/020/60/133/006/003/016 Radiation B019/BO54 energy at which or r There are 5 Soviet references. ASSOCIATION: Fizioheskiy institut im. P. N. Lebedeva Akademii nauk SSSR (Institute of Physics imeni P. N. Lebedev of the Academy of Sciences, USS ) PRESENTED: April 14, 1960, by D. V. Skobelltsyn, Academician SUBMITTED: Maroh 30, 1960 Card 3/3 SOV/26-58-12-2/44 AUTHOR: Pafomov, V.Ye., Candidate of Physical and Mathematical Sciences TITLE: An Outstanding Discovery of Soviet Physicists (Vydayushche- yesya otkrytiye sovetskikh fizikov) A Contribution to the Award of the Nobel Prize for Physics for 1958 to P.A. Che- renkov, I.Ye. Tamm and I.M. Frank (K prisuzhdeniyu nobelev- skoy premii. po fizike za 1958 9- P.A. Cherenkovu, I.Ye. Tammu i I.M. Franku) PERIODICAL: Priroda, 1958, Nr 12, Pp 11-14 (USSR) ABSTRACT: The article sketches briefly in popular language the Cherenkov effect. Ye.M. Brumberg and S.I. Vsvilov did preliminary re- search. The successful development of this work by P.A. Cherenkov, I.Ye. Tamm and I.M. Frank led to their receiving the Nobel Prize for physics for 10,56. There are 2 diagrams and 3 photos. ASSOCIATION: Fizicheskiy institut im. P.N. Lebedeva AN SSSR, Moskva (The Physics Institute imeni P.N. Lebedev, AS USSR, Moscow% Card 1/1 PAFOMDV, V. Yo., Uand Phys-Math Sol -- (diss) /The theory of Vavilov-Cherenkov radlationonisotrop-la media in the vresence of 11mItations," Moso 1958. 7 PP. (Acad Sol USSR, Phys Inst Im. P. N. Lebedev), 125 copies. Bibliogr at end of UxUR text (15 titles). (KL, 9-58, 113) 21(7) AUTHORS: Agranovich, V. If., Pafomov, V. Ye.9 QOV/56-36-1-z2/62 Rukhadze, A. A. ------- TITLE: On the Cherenkov Radiation of an Electron Moving in a Kedium With Spatial Dispersion (0 cherenkovskom izluchenii elektrona, dvizhushchegosya v srede s prostranst7ennoy dispersiyey) PERIODICAL: Zhurnal eksperimentallnoy i teoreticheskoy fiziki, 1959, Vol 36, Nr 1, pp 238-243 (USSR) ABSTRACT: The present paper deals with Vavilov-Cherenkov radiation in an isotropic gyrotropic medium in consideration of spatial dispersion. The formula for the total losses, which corresponds to this case, is written down. In consideration of spatial dispersion, Cherenkov radiation propagates on the surface of cones with the aperture angle-~i. The next chapter of this paper deals with the distribution of intensities over these cones. The formula for the total intensity of Cherenkov radiation here takes the form of a sum of the intensities distributed over the individual Cherenko-i cones. For a more intense study of the distribution of the intensity of Cherenkov radiation, the author investigates several possibilities of Card 1/4 taking the spatial dispersion of the medium into account, For On the Cherenko7 Radiation of an Electron Moving in a Medium With Spatial Dispersion frequency ranges which are fax from the eigenfrequencies of the medium it is possible to determine the solution for the decomposition of "direct" dispersion. Within this frequency range it holds uniquely that - n2 ((J) = F_ (4J)/(l +o( (60)), and Cherenkov radiation will be 0 distributed over the surface of a single cone. In the domains near the eigenfrequencias of the medium, spatial dispersion may be of essential influenoe and in this case a development of the "inverse" dispersion must be used. Assuming that the condition F_ 21A] 0 Cherenkov radiation is distributed over one cone, but with 13