SCIENTIFIC ABSTRACT KHALATNIKOV, I.M. - KHALDEYEV, O.D.

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SCIENTIFIC ABSTRACT
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N A I- 47-IV K6 v, , T. M 4 AUTHORS: Abrikosov, A. A., KhalatnikOv, I- M- 56-1-28/~6 TITLE: The Scattering of Light in a Fermi Flvid (Hasseyaniye eveta Y Fermi-zhidkouti) PERIODICAL: Zhurnal Eksperimentalinoy i Teoreticheskoy Fizikip 19581 Vol. 34t Nr 1p pp. 198-2o3 (USSR) ABSTRACT: The present paper determines the distribution of the scattered light to the angles and to the frcquencies. According to Landau (reference 1) oscillations of a certain type which are designated as "zero sound" can spread in a Fermi fluid at suffigiently low temporaturcs. Even at a temperature of 0,010 a frequency of more than loo cycles is needed for the immediate observation of zero soundt which renders the performance of such an experiment very difficult* But an indirect method can also be saggested whiob consists of the observation of tho Rayleigh scattering of light in liquid He3. The observation of the freqaancy distribution of the scattered light principally makes possible the measurement of the speed of zero sound. Besides, the scattering of the light in a Fermi fluid has a number of Card 113 specific features, wherefore the theoretical investigation The Scattering of Light in a Fermi Fluid 56-i-2e/56 of this phenomenonp especially of i;he distribution of the intensities to the frequencies, is of interest. Due to the very small polarizability of the helium-atoms it may be assumed that the dielectric constant changes due to the fluctuation of density. In the ranE:e of those temperature* and frequencies where >.kT applies the quantum effects must be taken into account in the averaging of all possible fluctuations. But for this purpose only the knowledge of the purely classical case is needed and then a certain corrective factor has to be introduoed. The fluctuation of the "random force" contained in the kinetic equation is determined by the method suggested by Rytov (reference 5)9 .Landau and Lifshits (reference 6). After the solution of this equation the fluctuations of the distribution function can then also be determined. The kinetic equation used here for the case of the Fermi fluid is oxylicitly written down. The authors are furthermore only interested in the case that the collisions can be diaregard.ed. In this connection the exact form of the shook integral doea not have to be known. But the velocity of modification of the entropy has to be determined. The course of the cclculatlon is followed Card 2/3 stel? by step. In this manner formulae for the caloulation The Scattering of LiCht in a Fermi Fluid 56-l-W56 13 followed atep by step. In this maLner for-iulae for the calculation of the fluctuations of the distribution function are found. Finally the formi:aa found for the distribution of the scattered light to the angles and frequencies is explicitly written dorn. The frequency spectriun consists of a central part E.nd of two sharp lines. The central part corresponds to the Doppler broadening of the main line. There are 9 references, 7 of w:..ich are Slavic. ASSOCIATION: Institute for Physical Problems All USSR (In5titut fizicheakikh problem Akademii nauk SSSR) SUBIMITTED: July 3o, 1957 AVAILABLE: Library of Congress Card 3/3 7z ~................... ~5-1 -37./),- ikav T T Yk .:uw.,r-;oi;uctor in a f'-iPh-11-'rvquenc:: ?~.,AA (_:;ver~h.-;rovo'!aik v v,~s:!,och,-,stctno.,,1 polF..) ;.;-i1O,ACALr 'Zhurnql oksper,imontallnoy i tcor~_'.tichos~,oy fiziki, 1958, Vol . 35 , fir 1 , pp. d6-~-275 (11;;3H) ABTZHACT: Bardeen, Cooper and Schrieffer (;3arLiin, Kup~r, Shriffcir) L*'C-- volopel a microscopical theor,11 of sun,-,rc:onductiv!t.'- ('~+?f In the present paper the question is investigated as to how superconductors behave in variable wcak ficids, and a new (not local) equation is derived, which describes the connec- tion between current ani ficli insteal of the eauation of the phenomenological theory by F. and G. London. Also the au-3s- tion of the depth of penetration of a weak stat4c field intD massive suporconductors and their lepenlence on temperaturp is dealt with. In the pr~,sent paper the riut~iora investip--~te the behavior of superconductors in high-fruouoncy fiel,,3 ani derive an equation describinF this behavior. 7'h._~ parer is subdivided into 4 sections. lihe first deals the quttinry.,- Carj 1/2 up of an equntion for the current in surjcrcon,~!.uctoro , 1!f ii". W A :3uDcrconductor in a Bigh-Froquency Fic14 OOV,156- 35- 1 - 37/-5,~ -1~ in dependL-nce on A(x); soction two Jpals with Pippard's limiting case, and section tnree deals with London's doijain (vk>A(O). In this case, only the ratio between T and & changes) and Ci is always large with respect to these two quanti- ties. The formulas written down in the present paper permit a Card 2/3 detailed comparison of theory with numerous experimental data. The Analysis of Experimental Data on the surface SOV/56-37-1-29/64 Impedance of Superconductors In the range of very high frequencies cj>>, no experimental data have become known.up to date*-rLhe causes of disagreement between the experimental date and the values of impedance cal- culated by the now theory of superconductivity have not yet been clarified. There are 3 figures and 6 references, 3 of which are Soviet. ASSOCIATION: Institut fizicheakikh problem'Akademii nauk SSSR (Institute of Physical Problems of the Academy of Sciences, USSR) SUBMITTED: February 3, 1959 Card 3/3 Amcs t TrTLI: Tbo pirsh AII.VaIV. Ca.r.-ooo on the "is. of La- (5-Y. wP#W';iiiiiyi Go_hVh.ftiF. p0 Trin. miattkit 21':W ~ FUZOVICALt rspekti rigicbeskim naux, 1)5), Tal 67, wr 4. pp 743-750 (MR) A1S'TXACT_- This Comfor.sq. took piece fr" O"s WL~21 to 1,19".b.r 1 .1 T%11J.Ij It v.@ orgeals#4 by the Otfol..iye $331 (N;*r$..mt of Phymica- *60.04%1.4 Balsa... or the A0.1-il f 3.1.nCes, MR). the a-doftlys. ... k ar..La.koy SSR (Le.I.My of SC100C.S. STU:Im.k.T. m), .04 %be 7billookly -1- "r Its% U. Stella& (Tbilisi St.%* University tacml The Cdxf~=- --a all-nJed *air at-0 3CO OP-ai-1101- ft*a Th Llol, R"-. Kharlkov, tiyq,, Lentgred, 3-r4la,wk, ad bar *111" -0 -all .2 by - Duab.r of y"ag Chit-.* :.*-prvt*xt working In the MR. About 50 lectures were deliver- -.4 *blc& "" 4J,14.d cc.rilng %a r.**.,.h f1#10. - Ir. jV2rAj2ZjyctivLtr. f3 lectures *are 1.11verod an this of wbicu- S** va" *xp*rInez%&I and the *%hers tbqor*tl. "I. Reports " exp.rl.watal I.vwtleallmg f,~pr:COndU livity re dell"rOA by TV. T. ass"In sni ".. F. &: n _k h r (LP*P) Zd 1. 1. Uvar1l.i-1jr kIPPI. The r.rc.r Im *Irv. r. she _41at. *let* in t'.Vexystals of pure C4rd Slit Ila, Us letter asasu,rej the tts=al conductivity of different. ly Nkmp*d OrlOutatO4 cylindrical CallIna smepltg at 4.2'9. 1 . N. 'al.'. _111h. bdh.wlcr 01 "p.maaduct~ in the hiCh-frequency, field. T. L. Cio~turg &at J,, - ~Zk"11 ~~ (?IAN) dealt ith the 4-4 Clasbarg discuso.4 --1-C other thi". the part pl.jr.d b7 floCIV.11m. in ph... tramallion. of lb * a.0 cord lgind. W. Llfghtts (nnl) shoved th.t it folio.* frm the =01..ft %be In conall,rallam of 1b. whl.o- ire, wy-*wuls thatt In ;xLacLple, the 4xistenci of su;ra. 80,04mclars is possible which or* supra-comiuctive only vith- in a Zimilet z*mg~ of temporoturo (&ad act at all %~;4ratures Va.." the critical at ) 3 T C "', &Ad T. Z. Irwala ("I) int-stlf.'-d :1,; vy of rap".Pd..1-re by .*-* of the 4~pmrskmxem %bat are oat very over absolute T. %yka, ad 1. 9. C-r--i-b (FTI Al 33311) a;-k. t" 0 r -0 , 'b '?a ~r& in-Me-Ta"dary between the and ao~l pbsoo.. D. ~. Zuoarev and Tu. A Tetrigarnikov, (!*-etec~etich..kly LamItto 1T ~l Z~iM-ui-.ks fS,,R) dealt ith Card 4/11 1bsrmWrVs=Icx of the -praconluctive *%&%a [Pr4ohllch-model)p Toloneh*~ (ml) 1a'.9%jCmt*4 the probjec of colle.ij,. "elt.tiam. 1. . -prm,onductcr. n. T. Shirko, (Ob"jra1in*anyy juslitut y.l.rzjth lvoloio~vsl: It.%. of 'fuel*" ICh .;s:nx b.ul of :.at,.Ia -1 toa4Vt%.rP. Th. probl** of of St. Coul aab I; vwrallan Was dISCUS944 by Cb*.I' Ch-u~hsien "'I 4%1-htio 107 1 ILI LI S/030/60/000/011/005/026 s-6 o fa B021/BO59 AUTHOR: Khalatnikov, I.M., Professor TITLE: Problems in Low-temperature Physics PERIODICAL: Vestnik Akademli nauk SSSR, 1960, No. 11, pp~ 28-35 TEXT: Low-temperature physics includes a large number of phenomena of which superfluidity, superconductivity, antiferromagnetism, and galvano.- magnetic phenomena in metals are particularly emphasized. Superfluidity in helium was discovered by P. L. Kapitsa in 1938. Temperature dependence of the thermodynamic quantities of helium were explained by L. D. Landau by the existence of a minimum in the energy spectrum. Fluid helium, consisting of He4 isotopic atoms and obeying Bose statistics, exhibits the property of superfluidity. At present, research of the properties of liquid helium is concentrated to the properties of the liquid He3 isotope. This field is regarded presently as the most promising area of research. The phenomenon of superconductivity had been discovered by Kamerlingh-Onnes 50 years ago, but has been explained only in the last few years. Superconductivity of me- tals is distinguished not only by vanishing resistivity, but also by extraordinary magnetic properties. The energy spectrum of superconductive Card 1/2 86229 Problems in Low-temperature Physics 3/030/60/000/011/005/026 B021/BO59 metals has, among others, also been explained by the Soviet acientist N. N. Bogolyubov on the basis of a system of Fermi electrons. The young scientist L. P. Gor1kov, who investigated the excitation spectrum by means of field quantum theoretical methods is also mentioned. Galvanomagnetic properties of metals have been investigated during the last years at the Institut fizicheskikh Problem Akademii nauk SSSR (Institute for Physical Problems of the Academy of Sciences USSR) and at t'~_e_ iziko-tekhnicheskiy institut Akademii nauk USSR (Institute of_Physics and Technology of the Academy of Sciences UkrSSR). The dependence of res4stivity, heat conduc- livity and other electrical characteristics of met;ls on magnitude and direction of a magnetic field were the subject of 'Investigations for the purpose of explaining the electron spectTum. The energy spectrum of the excitation of antiferromagnetics has not been obtained so far. Achieve- ments may be attained by co-operation of experimental and theoretical physicists. There is I figur,3. Card 212 j _&V S/056/60/039/01/19/029 B006/BO63 AUTHORS: Lifohitag Ye. N,, Khalatnikovt I._ M. TITLE: On the Singularities of Cosmo ngigal-Solutions of the Gravitational Equations. "P PERIODICAL: Zhurnal eksperimentallnoy i teoreticheskoy fiziki, 19609 Vol. 39t No- 1(7), PP- 149-157 TEXT: The usualloy applied cosmological solution of the Einstein gravi- tational equation is based on the assumption of an entirely homogeneous and isotropic mass distribution in space though this assumption is at Most approximately satisfied. In the present paper, the authors wanted to clarify as to how far the properties of the solution and, above all, the occurrence of time singularities are connected with this assumption. 'This problem can be tackled most successfully by studying the general properties of the solutions to gravitational equations in the neighborhood of singularities. Theeiistence of such solutions is assumed. Two particular classes of these solutions are given. One of them is a generalization of Card 1/2 S/056/60/059/003/032/045 Boo6/Bo63 AUTHORS: Lifshits, Ye. M., Khalatnikov~ I. M. TITLE: Singularities of the Cosmo.logical Solutions of Gravitatio- nal Equations..kvi PERIODICAL; Zhurnal eksperimentalinoy i teoreticheskoy fiziki, 1960, Vol. 39, No. 3119), pp. 600-808 TEXT: The sub-classe8 of cosmological solutions of gravitational equa- tions derived in Ref. 1 (Part I of the present paper) usually have singularities. The question as to whether the existence of singularities is a general property of cosmological rjolutions, irrespective of the as- sumptions made for the distribution ef matter and the field of gravity, has not been solved as yet. The solution of this problem is related to the existence or non-existence of a general solution of gravitational equations. Thus, the authors were confronted with the following problem: Within the region of a singularity that is assumed to exist, the form of the broadest class of solutions to gravitational equations is to be found, and conclusions are to be drawn as to the universal character of Card 1/2 88445 8/05 60/039/006/037/063 '~'O: 5-30c) Boo6yzoO AUTHORSt Bekarovich, I. L.9 Khalatnikovj-.I--X, TITLE: Theory of the UP tea Theraal Discontinuity on the Interface Between Liquid Hsi and a Solid PERIODICALs Zhurnal eksperisontallnoy i tooretiohookoy fiziki, 1960, Vol. 39, No. 6(12), pp. 1699 - 1712 TEXT: Heat transfer between liquid He II and the surrounding solid is accompanied by a temperature jump which in related to the complicated temperature exchange between He II and the phonons of the solid. A similar effect is displayed by He3 where the surface of the solid performs small vibrations, and the moved liquid carries away a small amount of energy. Nonetheless, a temperature jump occurs on the boundary. A theoretical description of this effect is presented here. The authors used liquid He3 which was in conlact with the vibrating surface of a solid. At low temperatures, liquid He can be regarded an a Fermi fluid, and its condition is characterized by an excitation distribution function which Card 1/3 4:1~ T 3 Theory of the Kapites, Thermal Discontinuity 8/056/60/85"06/037/063 on the Interface Between Liquid He3 and a B006/BO63 Solid an satisfies the equation of motion 7 .1 an -aL - -~n at . I(n) (n - distribu- t ar ap ap ar tion functionj F, - excitation energy which is a function of n; IN - collision integrall p - momentum). It may be assumed that all points of the body surface oscillate in phase. Therefore, the distribution function is only a function of the normal to the surface z. n is not equal to 110+nV where n 0 is the equilibrium Fermi function at absolute zero; thus, F- - &0 + f(p,pQnj(p')dp' and f(p,p') - 6t(p)/6n(p'). Spherical coordinates, G and %, are introduced (e is the angle between p and zi is the azimuthal angle), /4,is substituted for cos 9, and the coordinates are measured in units of the nean free path (I - 9 0'01 with w'r-tco (r-j - oscillation frequency) one obtains cquation (8): i4j1rF 3i1j'TF 3 irInF + 0 90 - I - 1 41- 2 cos~(plt . Next, az 1+F - 7-+Fl Min 1 -+F I" 0 1 the suitable boundary conditions ate determined. When substituting for ~(z,,a) at z-0, one obtains equation (15):1/ - -Pouz -Pou t- -~v 008~, Card 2/3 88445 Theory of the Kapitea Thermal Diso3ntinuity 8/056/60/039/006/037/063 on the Interface Between Liquid He and a B006/BO63 Solid and the condition for reads Iq (/.L-)djv- - -p u /3. The solution f, n a 7 +~1 0 Z to (8) is divided into two parts (proportional to u Z and ut) according to the two terms of (15). The solution corresponding to perpendicular surface oscillations is called the longitudinal solution, while that corresgbnaixg to tangential surface oscillations is called the transverse solution. The two types of solutions are discussed, and several relations are derived for diffuse reflection in both cases. Thereupon, mirror reflection is studied, in which case a solution is obtained through a Fourier expansion. Finally, several formulas are presented for the thermal resistance of the boundary, which is proportional to T,3. Academician L. D. Landqu Is thanked for discussions. V. A. Fok is mentioned. There are I figure and 5 references: 4 Soviet and 1 US. ASSOCIATION: Institut fizicheskikh problem Akademii nauk SSSR (Institute of Physical Problems, Academy of Soienoes USSR) SUBMITTED: June 13, 1960 Card 3/3 BEKAREWICII, I.L.j KILUATNIKOV I.M, Phenomenological deduction of the equations of vortex motion for He II. Zhur.ekspA teor.fiz. 40 no.3:920-925 Mr 161. (MIRA 14-8) 1. Ins%Ltut fizicheskikh problem Akademii nauk SSSR. (Vortex motion) (Helium) POKROVSKIYI? V.L.; XMIATVIKOV~ I.M. Superbarrier reflection of high-energy particles# Zhure ekspo i teoro fiz. 40 no.6:1713-1719 Je 161. (MIRA 14:8) 1. Institut fizicheskikh problem AN SSSR. (Particles (Nuclear physics)) ",fN al, V 25204 S/056/61/040/006/025/031 B108/B209 AUTHORS: Lifshits, Ye. M., Sudakov, V. V., Khalatnikov, 1. M. TITLEt Singularities of cosmological solutions of gravitation equations. III PERIODICALt Zhurnal eksperimentallnoy i teoreticheskoy fiziki, v- 40, no. 6t 1961, 1847-1855 TEXT: In earlier papers (Refs. 1,2s ZhETF, a, 149, 1960; ZhETF, 12, 800, 1960), Ye. M. Lifshits and I. M. Khalatnikov studied the form of the cosmological solution of gravitation equations near a point with time singularity. The general solution of gravitation equations with a fictitiotr singularity may be represented (by a proper choice of a synchronous reference system) in a form in which the singularity is synchronous for the entire space. Such a solution must contain eight arbitrary solutions of the three spatial coordinates: 1) four "physically different" functions, necessary to establish the gravitational field at a certain initial moment, 2) one function determining the initial hyper- Card 1/3 25204 S/056/61/040/006/025/031 Singularities of cosmological... B108/B209 surface in the geometrical structure, 3) three functions related to the requirement that the conditions g 00 ' -11 goa . 0 (1) for the metric tensor (Refs. 1,2) permit any transformation of the spatial coordinates without involving time. The arbitrary choice of the spatial. coordinates may be used to bring the first terms of the expansion for the m6trios near the singularity into a form in which the spatial differential length is given by the formula 2 6 a b 2 2 2 a 3 'dx a dx dx + (t -1) a & + 2 (t -0 a3 dx dx (5), dl godxo' ab 33 x3 a. where the indices a,b assume the values 112; the quantities a ab ta 3a 9a 30 are functions of all three ooorainates. These statements, together with the results of Refs. 1 and 2 lead to the o6noluaion that the presence of a time singularity is not a necessary property of cosmological models in the general relativity theory, and that the general case of arbitrary distribution of matter and gravitational field does not lead to such a singularity. The authors thank Academioian D. L. Landau and Card 2/3 252o4 3/056/61/040/006/025/031 Singularities of cosmological... B108/B209 L. P. Pitayevskiy for discussions. There are 3 Soviet-bloc references. ASSOCIATION: Institut fizicheskikh problem Akademii nauk SSSR (Institute of Physical Problems of the Academy of Sciences USSR) SUBMITTEDt January 259 1961 Card 3/3 S/030/62/000/002/007/008 11101/11110 AUTUOR: Khalatnikov, I. M., Doctor of Physics and Mathematics TITLE: New studies in the field of low-temperature physics PERIODICAL: Akademiya nauk SSSR. Vestnik, no. 2, 1962, 111 - 112 T E XT :This is n report on the VIII Congress oil Low- tempera Lure Physics held in Kiyev on October 13-20, 1961, by the Nauchnyy sovet Do fizike nizkikh temoeratur,Otdeleniya fiziko-matematicheskikh nauk Akademii nauk SSSR (Scientific Council of Low-temperature Physics of the Department of Physics and Mathematics of the Academy of Sciences USSR). This Scientific Council has been working for eight years. Tile conference was attended by scientists of Moscow, Leningrad, Khar1kov, Kiyev, Sverdlovsk, Tbilisi, and other places. The following papers and r3sulto are mentioned; Tunnel passages of electrons through0a dielectric lying between superconducting metal (Al, In, Sn, Pb) at 0.1 K. Superconducting modification of Bi, the suDerconductivity of Bi II being discovered with a transition temperature of'3.920K at 25,000 kg/cM2. Effect of electron scattering due to spin-orbit interaction on Night's shift in superconductors. Experimental investigation Card 1/3 S/030/62/000/002/007/008 New studies in the field of ... B101/B110 of superfluidity of demixed phases of He3_He4 solutions. Investigatio?) of the scattering of gamma quanta and slow neutrons in Fermi fluid (He to find the zero sound predicted by L. D. Landau. Piezomagnetic effect in siderite monocryntzil;t antiferromagnetic resonance in IAnCO and CoCO 3' The properties of 1114.3I-In alloy between room temperature and 1.3 K were studied to prove the coexictence of ferromagnetiam and antiferromagnetism below 20XK- I'vIleasurements of the magnetic heat capacity of carbonatee of transition metals between 60 and 1-50K shoived that the magnetic heat capacity (spin waves) in MnCO 3 exceeded that of the lattice by one order of magnitude. No spin waves were observed in FeCO 5" Theoretical study of quantum oscillations of complex electroconductivity in perpendicular magnetic and electric fields, and of the de Haas - van Alphen effect for electrons in the inetal. Theoretical prediction of a new type of oscillation of the ultrasonic absorption coefficient of metals in a magnetic field, which had already been proved experimentally in Zn monocrystals.. Development of the thoory of cyclotron retionnneo j.n metalo. E;e. 1) e r I 1:,,e n t 0 concerning the galvanomagnetic properties of Pb showed that the Fermi Card 2/3 S/030/62/COO/002/007/008 New studies in the field of ... B101/B110 level in Pb consisted of two equal parts with opposite signs. Thermo- maUnctic and galvanomagnetic effects in InAu, lnSb, and ~,,alvanoma(',netic effects in Al and In at low temperatures were investigated. Anisotropy of the effective massea in Al was found by cyclotron rooonatice, and the Fermi velocities and Lhe effective, electron masses in Sri wore measurod. Analysis of the dimension effect of the electric resistance in metals to ascertain the free path of electrons. Prediction for semiconductors of a new resonance type on band carriers caused by the electric vector of a high-frequency field at low temperatures. Spectroscopic study of the resonance effect in wurtzite-type semiconductors at helium temDerature led to the determination of the tensor of the effective masses. Hall effect and magnetic resistance of Ge in strong magnetic fields at low temperatures. Determination of the spin-spin and spin-lattice relaxation times in metal by "spin echo". Nuclear magnetic resonance in Tl with natural and enriched isotope content. Moessbauer effect of 23.8 kev gamma quanta on Sn 119 nuclei. Further reports dealt with low-temT)erature research, structure of strength, and polymorphous conversions at low temperatures. Card 3/3 Or 2111,1 ~j 4~ F, 45 -- 4% "R N, ABRIKOSOV, A.A., doktor fiziko-matematicheakikli nauk; K-HALATNIKOV I.M. doktor fiziko-matematicheskikh nauk, prof. Aca4emician Lev Davidovich Landau. Fiz.v shkole 22 no.1:2l-z7 ja-F 162. (11M 15 -.3) (Landau., Lev Davidovich., 1908-) AERIKOSOVv A.A., doktor fisika--mat6maticheakikh nauk, prof.' KHAIATNIWV I doktor fiziko-matematicho5kikh naukj prof ~a S~=etry of the world. Fiz,v shkole 22 no.5t4-13 B-0 162, WRA l5sl2) (Particlea (Nuelear physics)) (Symetry) TAMK, I.Ye., akademik; ABRIKOSOV, A.A., doktor fiz.-matem.nauk; KHALATNIKOV I.M., doktor fir.-matem.nauk Nobel prize wi=er foi 1962. Test.AN SSSR 32 no.12:63-67 D 162. (KERA 15,12) (Undgu, lav Davidovicbp 1908-) I S/056 62/'043/'00,'z,/'O,r5/063 B 1 04X1 02 AUTHORS: Patashinskiy, A. Z., Pokrovskiy, V. L., Khalatnikov, i. TITLE: Regge poles in nonrelativistic quantum mechanics P-_--R!CD I CAL: Zhurnal eksperimental'noy i teoraticheskoy fiziki, v. 43, no. 3(g), 1562, 1117-1119 'i_- Ii method of examining the position of the poles in the complex Momentu~n *planelfor a lar(,e class of potentials was worked out. - This method iq cloo'l-1.1y related to that previously established by V. L. Pokrov3kiy and nikov (ZhETF, 40, 1713, 1961). The ronanulytical potential 1. i~.:. Khalat U U, < 0 for r a is s tudied on t,',.e basis of a semi- 0. claosical approximation to Schr6difieer's radial equation. From the equations X,J', (xl)lj.(x.) xH(,"'(x)1II,( 11 (x), x2jal = 2niE, /a'= 2m (E - U(~). (3) Card 1/3 5/0:i6 '62/043/M/059/063 Reje Ie poles i noLrllelativis'ti c. B104YB 102 it is conclud that three series of ales exist. Tha first series is to tVieft- of Vj~ X, ~,Fig. 1), tho second in the unpar semiplane abovo tho il point x atymptotically approacIning the line Im -1 at U < E < 0. T h,~ 0 third sorieg is missing when U 0 E < 0, but approximately symmnetric -~-Ath h c o n d :3 o r i e u wh e n '"' > 0 . Ar, analytical potential V(r) 'aiiving singularitles in the complex momentum plane is examined. 'tiller, --->>U0 the Doles are-near to those values of I at which the level lir~e has two ;:.oints of inverpion,ir V~ej/k and r (Fig. 2). There are twe. oeries of poles in 1 2 the UDP4~ s Iem1plane. The first series extends to the left and downward of i ; ,, 1 2 the po nt q~= kr , k = 2mT.1, approaching the real axis asymptotically. Th,_ 0 second s'drie6 ~is situated right. and left of the point, 9 = kr 0 where the asymptotO,s Im(V - kr )~n/ln(n), Re(~ - kr )-In,(V - kr')/ln(n). The 0 0 0 i Position !of the poles in the case of-minU (r)< E