{"id":4329,"date":"2013-03-20T19:09:13","date_gmt":"2013-03-20T15:09:13","guid":{"rendered":"http:\/\/ellphi.lebedev.ru\/?p=4329"},"modified":"2013-04-05T15:17:11","modified_gmt":"2013-04-05T11:17:11","slug":"1984-en","status":"publish","type":"post","link":"http:\/\/preprints.lebedev.ru\/?p=4329","title":{"rendered":"1984 En"},"content":{"rendered":"

A.D. Linde , <\/em>
\n\u2116 8<\/strong> QUANTUM CREATION OF INPLATIONARY UNIVERSE
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> |\u0410\u043d\u043d\u043e\u0442\u0430\u0446\u0438\u044f|<\/a>\n

It is shown that the process of quantum creation of the universe in a wide class of elementary particle theories with a large probability leads to the creation of the exponentially expanding (Inflationary) universe, which after expansion 28 acquires the else l \u2265 10 \u0441\u043c. ---------------------------<\/div>\n<\/p>\n

\u0410.\u0412. \u0412\u0438\u043d\u043e\u0433\u0440\u0430\u0434\u043e\u0432 , <\/em> \u0412.\u0424. \u041a\u043e\u0432\u0430\u043b\u0435\u0432 , <\/em> \u0418.\u0412. \u041a\u043e\u0436\u0435\u0432\u043d\u0438\u043a\u043e\u0432 , <\/em> \u0412.\u0412. \u041f\u0443\u0441\u0442\u043e\u0432\u0430\u043b\u043e\u0432 , <\/em>
\n\u2116 9<\/strong> \u041c\u041e\u0414\u0410 \u0428\u0415\u041f\u0427\u0423\u0429\u0415\u0419 \u0413\u0410\u041b\u0415\u0420\u0415\u0418, \u0412\u041e\u0413\u041d\u0423\u0422\u042b\u0415 \u041f\u041e\u0412\u041e\u0420\u041e\u0422\u041d\u042b\u0415 \u0417\u0415\u0420\u041a\u0410\u041b\u0410 \u0418 \u0420\u0415\u0417\u041e\u041d\u0410\u0422\u041e\u0420\u042b \u0414\u041b\u042f \u0418\u0417\u041b\u0423\u0427\u0415\u041d\u0418\u042f \u041c\u042f\u0413\u041a\u041e\u0413\u041e \u0420\u0415\u041d\u0422\u0413\u0415\u041d\u041e\u0412\u0421\u041a\u041e\u0413\u041e \u0414\u0418\u0410\u041f\u0410\u0417\u041e\u041d\u0410
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> |\u0410\u043d\u043d\u043e\u0442\u0430\u0446\u0438\u044f|<\/a>\n

The geometrooptical and wave theory of X-ray propagation across the smooth cylindrical surface has been developed. The angular and spectral pro? parties of the X-ray concave mirrors are considered. On the basis of Maxwell equations the structure of the electromagnetic field near the mirror surface is determined. The frequencies and decrements of the X-ray eigen modes sliding across the concave cylindrical surface are found. If the absorption is negligeable, the quality factor, Q, of the resonator (as well as the mirror reflectivity) is connected with the effect of the wave penetration into the dielectric media at the angles smaller than the critical angle of the total external reflection. ?or calculation of the mirror parameter the available experimental data are used. ---------------------------<\/div>\n<\/p>\n

A.B. Goncharov , <\/em> A.D. Linde , <\/em>
\n\u2116 11<\/strong> CHAOTIC INFLATION OF SUPERGRAVITY
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> |\u0410\u043d\u043d\u043e\u0442\u0430\u0446\u0438\u044f|<\/a>\n

A new realization of the chastic inflation scenario is suggested in the context of N=1 supergravity. ---------------------------<\/div>\n<\/p>\n

T.V. Danilova , <\/em> A.D. Erlykin , <\/em> S.K. Machavariani , <\/em>
\n\u2116 14<\/strong> THE USAGE OR SMALL EAS EXPERIMENTAL DATA OR THE CALLBRATION OR THE MODELOF THE COSMIC RAY PROPAGATION THROUGH THE ATMOSPHERE. THB RBSULTS OF SIMULATIONS AND COMPARISON WITH THE EXPERIMENT
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> |\u0410\u043d\u043d\u043e\u0442\u0430\u0446\u0438\u044f|<\/a>\n

In the first part of this work \/1\/ the characteristics of models were described which were accepted in simulation of extensive air showers. Below the simulation results are presented for small EAS, observed at the Mountain level. ---------------------------<\/div>\n<\/p>\n

T.V. Danilova , <\/em> A.D. Erlykin , <\/em>
\n\u2116 15<\/strong> THE USAQE OP SMALL EAS EXPERIMENTAL \u041f\u0410\u0422\u0410 FOR THE CALIBRATION OP THE MODEL OP THE COSMIC RAY PROPAGATION THROUGH THE ATMOSPHERE. DESCRIPTION OP MODELS
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> <\/p>\n

V.P. Silin , <\/em>
\n\u2116 23<\/strong> THE ADVANOESIN THE THEORY OF THE PLASMA ION ? SOUND TUBULENSE
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> |\u0410\u043d\u043d\u043e\u0442\u0430\u0446\u0438\u044f|<\/a>\n

The ion-sound turbulence (IST) theory results obtained from the analytical solution of kinetic equations for ion-sound waves and plasma electrons are reviewed. Some applications of the IST theory are indicated. ---------------------------<\/div>\n<\/p>\n

N.G. Basov , <\/em> A.F. Plotnikov , <\/em> V.N. Selesnev , <\/em>
\n\u2116 30<\/strong> OPEBATIVE OPTOELECTROHIC MEMORY OF A LARGE CAPAC1TY
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> <\/p>\n

V.L. Ginsburg , <\/em> V.S. Ptuskin , <\/em>
\n\u2116 35<\/strong> ON GAMMA-RADIATION OF MAGELLANIC CLOUDS AND OF SUPERNOVA REMNANTS-POSSIBLE ANTIPROTON SOURCES IN THE GALAXY
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> |\u0410\u043d\u043d\u043e\u0442\u0430\u0446\u0438\u044f|<\/a>\n

Badiation of Magellanic Clounds is discussed in view of the nearest perspectives of observation gamma-astronomy. Expected gamma-ray fluxed are compared according to metagalactic and galactic theories of the cosmic ray origin. The best way to disprove metagalactic models is found to be determining the ratio of gamma-radiation fluxes from SMC and LMC. Gamma-luminosity of the young supernova remnats which can generated many antiprotons is estimated. It is shown that such remnants must have a relatively short phase with a very powerful gamma-radiation. ---------------------------<\/div>\n<\/p>\n

A.I. Andryshin , <\/em> A.E. Kazakov , <\/em>
\n\u2116 38<\/strong> THE DECAY OF AUTOIONIZING ATOMIC STATE IN THE BESONANCE ELECTROMAGNETIC FIELDS
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> |\u0410\u043d\u043d\u043e\u0442\u0430\u0446\u0438\u044f|<\/a>\n

The decay of the autoionizilng state (AS) is considered in the presence of the resonance electromagnetic field (e.m.f.) connecting AS with other level (descrets or autoionizing). It is shown that this process can be characterised by two decay constants which depend on frequency, intensity and polarisation of the a.w.f. One of this constants is always more or of the order of the field free autoionizing width of AS. But if the e.m.f. parameters obey some conditions the other decay constant can be much smaller than the field free AS width. In this case a life-time of AS in the e.a.f. is a whole can be much more than the field free lifetime of AS. In means that there la a partial stabilization of AS. The AS lifetime increasing is connected with a destructive interference between the autoionizing and ionizing transitions. But there are always the «noninterfering» transitions due to which the stabilization never can be absolute and a long living part of AS population la rather small. ---------------------------<\/div>\n<\/p>\n

A.M. Danaevsky , <\/em> S.V. Pashkov , <\/em>
\n\u2116 59<\/strong> Monte Carlo method with weights non equaled to one and cascade simulation
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> |\u0410\u043d\u043d\u043e\u0442\u0430\u0446\u0438\u044f|<\/a>\n

The Monte Carlo method of events generation with weights non-equal to one is suggested for the atmospheric cascades simulation. The exact formulae for distributions, average values and errors, to be necessary for the statistical processing of weighted event* are derived. The use of the method leads to decrease of the com?puter time, required for the events simulation about 100 times and greater. This fact provides one with ample opportunity of the quantitive investigation of events characteristics sensitivity to the model parameters, that was unreal up to now. ---------------------------<\/div>\n<\/p>\n

E.S. Fradkin , <\/em> A.A. Tseytlin , <\/em>
\n\u2116 67<\/strong> QUAHTUM EQUIVALENCE OF DUAL FIELD THEOEIES
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> |\u0410\u043d\u043d\u043e\u0442\u0430\u0446\u0438\u044f|<\/a>\n

Motivated by the study of ultraviolet properties of different versions of supergravities we discuss duality transformations at the quantuai level. Using the background field method we prove on shell quantum equivalence for several pairs of dual field theories known to be classically equivalent. The examples considered include duality in chiral model, duality of scalars and second rank antisymmetric gauge tensors, vector duality and duality of the Einstein theory with coamological term and the Eddington-Schrodinger theory. ---------------------------<\/div>\n<\/p>\n

A.N. Lesnov , <\/em> V.I. Man»ko , <\/em> S.M. Chumakov , <\/em>
\n\u2116 70<\/strong> HIGH ENERGY AND COSMIC RAYS PHYSICS
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> |\u0410\u043d\u043d\u043e\u0442\u0430\u0446\u0438\u044f|<\/a>\n

The explicit solitons solutions for dynamioal systems with sl(2,R) algebra as the continuous component of internal symmetry algebra of these systems are found by means of scalar L -A pair formalism. ---------------------------<\/div>\n<\/p>\n

I.A. Batalin , <\/em> G.A. Vikovisky , <\/em>
\n\u2116 76<\/strong> EXISTENCE THEOREM FOR GAUGE ALGEBRA
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> |\u0410\u043d\u043d\u043e\u0442\u0430\u0446\u0438\u044f|<\/a>\n

A general gauge action is defined by postulating minimum of its properties, necessary for the existence of loop expansion in the quantum theory. The structure of the general gauge algebra is derived from these postulates. The proof of existence of the structure functions, lacking in previous works, is given. The question of uniqueness is also completely cleared up. Some unsolved problems are discussed is connection with the Covariant-Quantization Conjecture. ---------------------------<\/div>\n<\/p>\n

O.D. Dalkarov , <\/em> V.A. Karmanov , <\/em>
\n\u2116 77<\/strong> SCATTERING OP LOW ENERGY AHTIPROTONS FROM NUCLEI 12C AND 16O
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> |\u0410\u043d\u043d\u043e\u0442\u0430\u0446\u0438\u044f|<\/a>\n

The differential cross-sections for elastic scattering and cross-sections for exitation of nuclear level by low energy antiprotons from carbon and oxigen nuclei are calculated. Theoretical curves agree with experimental data at 46.8 MeV which have been obtained at LEAR. We predict the differental cross-seotlons for nuclear level exitation with definite spin projection of exited nucleus. They determine an angular ? — quanta distributions in (p,p?) reactions on nuclei. ---------------------------<\/div>\n<\/p>\n

V.V. Dodonov , <\/em> V.I. Man»ko , <\/em> V.V. Semjanov , <\/em>
\n\u2116 78<\/strong> THE DENSITY MATRIX OF THE CANONICALLY TRANSFORMED MULTI-DIMENSIONAL IN THE FOCK BASIS
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> <\/p>\n

R.E. Kallosh , <\/em>
\n\u2116 79<\/strong> GEOMETY OF 11-DIMENIONAL SUPERGRAVITY
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> <\/p>\n

A.I. Nikishov , <\/em>
\n\u2116 81<\/strong> SYMMETRY IN PION SYSTEM
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> |\u0410\u043d\u043d\u043e\u0442\u0430\u0446\u0438\u044f|<\/a>\n

The pion system with fixed number of pions H \u0430\u043f\u0439 fixed charge \u0429 is considered. The isospin functions for 3- and 4-pion systems are given. The are characterized b\u0443 the total isospin T, its projection T3=Q and are the base functions of the Young-Ymanouchi irreducible orthogonal representation of the permutation groups Sn. It is shown how from the total wave function of a given S (or a superposition of a few functions of different T) there follow relations between amplitudes, each of which is characterized by e. particular way of attachment of each charge to the particular momentum. (For definiteness we assume that the quantum numbers other than charge are moments). The squared amplitudes in same cases uniquely determine the weight with which an elementary lave function, characterized by an irreducible representation of Sn, enters into the total wave function. The existence of compound-resonances described by the elementary wave functional is suggested (i.e. N-plon resonances labled by an irreducible representation of Sn and other quantum numbers). For a given \u043echarge content (I.e. for fixed numbers N+, N-, N0 of ?+, ?-, and ?0 correspondingly) we find tee numb\u0435\u0433 of times each irreducible representation is contained in the representation realized by the products of one — pion charge functions. ---------------------------<\/div>\n<\/p>\n

N.G. Basv , <\/em> N.E. Bykovsky , <\/em> V.V. Ivanov , <\/em> Yu.V. Senatsky , <\/em> G.V. Sklizkov , <\/em>
\n\u2116 86<\/strong> FORMATION OF THE POPULATION INVERSION AT PULSED SELECTIVE PUMPING OF NEUDUMIUM LASER ACTIVE ELEMENTS
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> |\u0410\u043d\u043d\u043e\u0442\u0430\u0446\u0438\u044f|<\/a>\n

A possibility of selective pumping of an Nd: glass laser by means of electron-beam exited semiconductor laser radiation has been considered. The systems providing the concentration of semiconductor laser radiation may allow pumping of active elements with the efficiency related to stored population inversion up to \u2264 5%, and a pulse repetition rata up to \u2248 1 Rs. The modeling experiment has been made on exciting the laser oscillation in glass samples with Nd34 ion concentration of 4-8x10cm-3 by means of a 2 ns Nd-laser second-harmonic pulse. Experiment and numerical calculations allow to estimate the relaxation times of the excitation from pumped bands to ---------------------------<\/div>\n<\/p>\n

V.V. Dodonov , <\/em> V.I. Man»ko , <\/em> D.L. Osipov , <\/em>
\n\u2116 91<\/strong> THE QUASI-CLASSICAL BQUILIBHIOM WIGHBR DISTRIBUTI0N FUNOTION OF AH ELECTRON GAS IH A HOH-UNIFORM ELECIRO-MAGNETIC FIELD
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> |\u0410\u043d\u043d\u043e\u0442\u0430\u0446\u0438\u044f|<\/a>\n

Quantum corrections up to order ? are found for the equilibrium distribution function of ah electron gas in a non-uniform electromagnetic field in the case of Boltzmann statistics. The quantum corrections are also found for the classical free energy. ---------------------------<\/div>\n<\/p>\n

R.J. Glauber , <\/em> V.I. Man»ko , <\/em>
\n\u2116 96<\/strong> DAMPING AND FLUCTUATIONS IN SYSTEMS OP C0UPLKD QUANTUM FORCED OSCILLATORS
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> |\u0410\u043d\u043d\u043e\u0442\u0430\u0446\u0438\u044f|<\/a>\n

A damping and an equilibrium under the influence of random?ly fluctuating driving forces of different magnitudes state in terms of P-distribution function are obtained for a system of N coupled forced harmonic oscillators contained in a heat bath which is a system of different heat baths with different temperatures interacting with every of oscillators. ---------------------------<\/div>\n<\/p>\n

V.G. Denisova , <\/em> A.K. Managadze , <\/em>
\n\u2116 101<\/strong> Overlapping effect of neighbouring electron-photon cascades in gamma-families and its influence on gamma-family characteristics.
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> <\/p>\n

V.S. Titov , <\/em> B.V. Somov , <\/em>
\n\u2116 110<\/strong> Magnetic reconnection in a high-temperature plasma of solar flares.
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> <\/p>\n

B.V. Somov , <\/em> V.S. Titov , <\/em>
\n\u2116 111<\/strong> Magnetic field dissipation in a high-temperature plasma pf solar flares.
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> |\u0410\u043d\u043d\u043e\u0442\u0430\u0446\u0438\u044f|<\/a>\n

A simple self-consistent model of a high-temperature turbulent current sheet (HTCS) is oonsidered. The anomalous character of plasma conductivity in a sheet is assumed to be due to gradient instabilities. The possibility of a low threshold of their excitation is demonstrated on an example of temperature-drift instability. Application of the HTCS model to the «hot» or «main» phase of a solar flare is discussed. The model consistently explains the observed properties of this phase. ---------------------------<\/div>\n<\/p>\n

A.S. Babichenko , <\/em> A.E. Shabad , <\/em>
\n\u2116 127<\/strong> Infrared singularities in Quantum Statistics Summed to Confinement.
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> <\/p>\n

Yu.I. Skrynnikov , <\/em> Luigi.. Nocera , <\/em> V.. Somov , <\/em>
\n\u2116 129<\/strong> Hard X-rays bremsstrahlung produced by electrons escaping a high-temperature thermal source in a solar flare.
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> <\/p>\n

A.D. Mironov , <\/em> V.. Puhryghin I , <\/em> I.I. Royzen , <\/em>
\n\u2116 130<\/strong> Qcdapproach to the inelastic diffraction with large transfers of transverse momenta.
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> <\/p>\n

G.N. Birich , <\/em> Yu.I. Bogdanov , <\/em> S.I. Kanorskii , <\/em> I.I. Sobelman , <\/em> V.N. Sorokin , <\/em> I.I. Struk , <\/em> E.A. Yukov , <\/em>
\n\u2116 136<\/strong> Optical rotation on 648nm transition in atomic bismuth vapor.
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> <\/p>\n

I.M. Dremin , <\/em> V.I. Yakovlev , <\/em>
\n\u2116 141<\/strong> Particles with heavy quarks and long-flying cascades in cosmic rays.( Tien-shaw effect).
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> <\/p>\n

I.I. Sobelman , <\/em> A.V. Vinogradov , <\/em>
\n\u2116 150<\/strong> OF THE PROBLEM OF EXTREME UV AND X-RAY LASER
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> <\/p>\n

I.M. Dremin , <\/em> D.T. Madigontin , <\/em> V.A. Saakyan , <\/em>
\n\u2116 152<\/strong> Heavy quark hadrone and ionisation curves of cascades In a matter
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> |\u0410\u043d\u043d\u043e\u0442\u0430\u0446\u0438\u044f|<\/a>\n

The abundant production of charmed particles at high energies explains the origin of long-flying cascades observed in cosmic ray studies? The conclusion is derived from an analy?tic solution of simplified kinetic equations and is confirmed by computer calculations of more rigorous equations, the charmed particles production cross section at SFS-collider energies should be about 5 mb par nucleon. ---------------------------<\/div>\n<\/p>\n

F.M. Saradzhev , <\/em>
\n\u2116 168<\/strong> Instanton configurations in Minkowski space-time.
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> |\u0410\u043d\u043d\u043e\u0442\u0430\u0446\u0438\u044f|<\/a>\n

We oonetruct self- and antlselfdual SU(2)’t Hooft type solutions to the Jang-Mills equations in Minkowski space-time. Configurations of topological number +2 are singled out. ---------------------------<\/div>\n<\/p>\n

V.I. Mazhukin , <\/em> A.A. Samokhin , <\/em>
\n\u2116 170<\/strong> Radiation-induced vaporization kinetiks from a surface into vaguum.
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> |\u0410\u043d\u043d\u043e\u0442\u0430\u0446\u0438\u044f|<\/a>\n

Vaporization kinetics from a surface Into vacuum la investigated for various transient heating regimes due to intense Irradiation of the surface. One-dimensional theoretical model of the process includes heat conduction into the (surface, vapor flux through a Knudsen layer, and vapor flow without plasma formation. «Transient vaporization kinetics turns out to be more complicated than it was assumed previously. Results of numerical calculations show that there are transient solutions of the nonlinear vaporization problem with a constant value of the flow Mach number M = 1 at the outer edge of the Knudsen layer. Evolution of M depends strongly on variation of radiation intensity. ---------------------------<\/div>\n<\/p>\n

E.A. Akhundova , <\/em> V.V. Dodonov , <\/em> V.I. Man’ko , <\/em>
\n\u2116 175<\/strong> The quasi-classical propagator of a quantum particle ina uniform field in a half space.
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> <\/p>\n

A.M. Dunaevsky , <\/em> S.V. Pashkov , <\/em>
\n\u2116 187<\/strong> Scaling violation and large Ptjets on EC gamma-families data
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> <\/p>\n

V.P. Silin , <\/em> V.T. Tikhonchuk , <\/em>
\n\u2116 192<\/strong> DOUBLE SIMULATED SCATTERING AND THE DEVELOPMENT OF THE THEORY OF PARAMETRICINSTABILITIES IN PLASMAS
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> |\u0410\u043d\u043d\u043e\u0442\u0430\u0446\u0438\u044f|<\/a>\n

The coherent structure of electromagnetic fields in plasmas in reason of for the new features of parametric instabilities . Such coherent structure connected with the reflection surface of the electromagnetic waves produces the distributed feedback. Because of this feedback the number of the interacting electromagnetic waves in the processes of the stimulated scattering is twice more than usually. Such double stimulated scattering processes are connected with absolute parametric instabilities. The examples of double simulated Mandel?shtam-Brillouing scattering, double combination (Raman) scattering and parametric decay are discussed. ---------------------------<\/div>\n<\/p>\n

S.M. Apenko , <\/em> Yu.E. Losovik , <\/em>
\n\u2116 196<\/strong> On the Quantization of the Hall Conductivity In Two Dimensions
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> |\u0410\u043d\u043d\u043e\u0442\u0430\u0446\u0438\u044f|<\/a>\n

The Hall conductivity is expressed in terms of classical drift trajectories In the high-H limit. The general connection of \u0431xy with the properties of edge states is established, which explains the quantization of the Hall conductivity. The quantization is shown to be exact in the high-H limit in the infinite system at zero temperature. \u0422he finite frequency effects are also discussed and the AG response is related to geometrical characteristics of equipotential lines in the external potential. ---------------------------<\/div>\n<\/p>\n

I.A. Batalin , <\/em> O.V. Ogievetsky , <\/em>
\n\u2116 198<\/strong> QUANTIZATION ON A CLASS OP SUBMANITOLDS OP PHASE SPACE
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> |\u0410\u043d\u043d\u043e\u0442\u0430\u0446\u0438\u044f|<\/a>\n

The generalization of the usual \u0416 -multiplication of Wey1 symbols is given and applied to the problem of quantization on some class of submanifolds of phase spaee. This class is defined by the requirement that one half of second class constraints must be linear commutative (in the sense of the Poisson brackets) functions. The modified \u0416 -multiplication is associative and gives correct classical limit (the Dirac brackets) for the \u0416 — commutators. The modification is obtained by replacement of the usual derivatives by their covariant projections in the Weyl \u0416 — multiplication. ---------------------------<\/div>\n<\/p>\n

S.P. Baranov , <\/em> A.A. Komar , <\/em>
\n\u2116 230<\/strong> ON THE POSSIBLE MECHANISM OF INCLUSIVE ? -MESON PRODUCTIOH IN \u041dDRO\u041d-\u041d\u0410ADRON COLLISIONS
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> <\/p>\n

\u0415.\u0413. \u0411\u0435\u0441\u0441\u043e\u043d\u043e\u0432 , <\/em>
\n\u2116 238<\/strong> \u041b\u0410\u0417\u0415\u0420\u042b \u041d\u0410 \u0421\u0412\u041e\u0411\u041e\u0414\u041d\u042b\u0425 \u042d\u041b\u0415\u041a\u0422\u0420\u041e\u041d\u0410\u0425
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> |\u0410\u043d\u043d\u043e\u0442\u0430\u0446\u0438\u044f|<\/a>\n

Fundamentals of the free-electron laser (fel) theory Is presented in this review. High efficiency, high power and extreem vacuum ultraviolet fel are discussed and some new results are presented. She consistent theory of the parametric fel is developed. The theory is valid hen the prebunched beam le considered «unfrozen» during the inter-action within the long radiator (wiggler) for the coherent emission and has a significant energy and angular spread. ---------------------------<\/div>\n<\/p>\n

M.V. Chegotov , <\/em> V.P. Silin , <\/em> V.T. Tikhonchuk , <\/em> A.A. Zosulya , <\/em>
\n\u2116 244<\/strong> THE NONLINEAR \u0422\u041dE\u041eRY \u041eF \u0422\u041d\u0412 DOUBLE MANDELSTAM-\u0412RILLOUIN S\u0421\u0410TTERING (DSBS) IN PLASMAS
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> |\u0410\u043d\u043d\u043e\u0442\u0430\u0446\u0438\u044f|<\/a>\n

Double Mandelstam-Brillouin scattering (DSBS) nonlinear theory in laser-produced plasma presented. DSBS is characterized by the nonline\u0430\u0433 coherent interaction of the pump wave components incident on plasma and reflected from the critical surface with the scattered Stokes components. The excitation thresholds and the stationary nonlinear states corresponding to the main and the higher scattering modes are examined taking into account the effects of the electromagnetic waves absorption general pump wave polarization, density and temperature inhomogneity. It is shown, that under the strong \u0435.m. waves absoription DSBS is generated from the relatively narrow rarefied plasma region. For the main DSBS mode soft excitation takes place whereas for the higher modes hard excitation regimes are revealed. ---------------------------<\/div>\n<\/p>\n

I.A. Batalin , <\/em> E.S. Pradkin , <\/em> Sh.M. Shartsman , <\/em>
\n\u2116 254<\/strong> QUAHTUM ELECTRODYNAMICSS IN EXTBRNAL CONSTANT FIELDS
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> |\u0410\u043d\u043d\u043e\u0442\u0430\u0446\u0438\u044f|<\/a>\n

Generating functional, of all quantum Green functions in an external field is found. The Green function of a scalar particle in a constant and uniform external field is calculated with the help of the modified perturbation theory. Its infra-red asymptotics Is studied. It is shown that the enhancenent of the pole takes place, the sane as in the vacuum case. ---------------------------<\/div>\n<\/p>\n

N.G. Basov , <\/em> S.Yu. Gus’kov , <\/em> G.V. Danilova , <\/em> N.N. Demchenko , <\/em> N.V. Zmitrenko , <\/em> V.Ya. Karpov , <\/em> T.V. Mishchenko , <\/em> V.B. Rozanov , <\/em> A.A. Samarsky , <\/em>
\n\u2116 256<\/strong> THERMONUCLEAR YIELD OF SHORT-WAVE (?<1 ?m) HIGH-POWER LASER TARGETS\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> |\u0410\u043d\u043d\u043e\u0442\u0430\u0446\u0438\u044f|<\/a>\n

Within the frames of a single optimization scheme we have numerically obtained the dependences of the gain coefficient K = Kfus\/Eab(Efus is the energy released in fusion reactions) on the absorbed energy 0.3 \u2264 Eab \u226410 MJ for the lasers having t’e wavelength ? \u2264 1 \u2264m, and for simple two-layer targets (CH2 — ablator and DT-ice) with the given aspect ratio. ---------------------------<\/div>\n<\/p>\n

K.S. Fradkin , <\/em> A.A. Tseytlin , <\/em>
\n\u2116 261<\/strong> EFFECTIVE FIELD THEORY FROM QUANTIZED STRINGS
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> |\u0410\u043d\u043d\u043e\u0442\u0430\u0446\u0438\u044f|<\/a>\n

We present a covenant definition of effective action \u0413 ‘for fields corresponding to different string excitations (scalar, external metric, antisymmetric tensor, …) in termsof string path Integral with external sources. The problem of deriving the gravitational part of \u0413 is reduced to establishing the effective action for a generalized ? -model on a curved 2-dinensional background and subsequent integration over 2-dlmeneional metrics. It is shown that \u0413 contains the Einstein term in a zero slope limit. A consistent formalism is developed for a study of a ground state problem (including the problem of space-time compactifiwtion) in the quantum string theory. It is shown that the stable vacuum exists in which the scalar, cetric and antisymmetric tensor have non-zero background values. This provides a solution to the old «tachyon problem». Generalizations to Fermi string theory and theories of other extended objects (membranes, etc) are also discussed. ---------------------------<\/div>\n<\/p>\n

O.K. Kalashnikov , <\/em>
\n\u2116 265<\/strong> QUARK-GLUON PLASMA THKOUOH PERTURBATIVE AND NOKPERTURBATIVE CALCULATIONS
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> |\u0410\u043d\u043d\u043e\u0442\u0430\u0446\u0438\u044f|<\/a>\n

QCD at \u0422,??0 is studied using the temperature Green function method, the standard polarization operator of gluons is calculated both in relativistic and axial gauge, and its asymptotic behaviour is investigated. Both Fermi- and Bose-excitation spectrum of quark-gluon plasma are found. Their gauge invariance is proved and the renormalization group improvement of the dispersion curves is given. The QCD thermodynamical potential is exactly expressed in terms of the temperature Green functions end calculated with the nonanalytical ---------------------------<\/div>\n<\/p>\n","protected":false},"excerpt":{"rendered":"

A.D. Linde , \u2116 8 QUANTUM CREATION OF INPLATIONARY UNIVERSE \u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442 |\u0410\u043d\u043d\u043e\u0442\u0430\u0446\u0438\u044f| It is shown that the process of quantum creation of the universe in a wide class of elementary particle theories with a large probability leads to the creation of the exponentially expanding (Inflationary) universe, which after expansion 28 acquires the else l […]<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[8],"tags":[],"_links":{"self":[{"href":"http:\/\/preprints.lebedev.ru\/index.php?rest_route=\/wp\/v2\/posts\/4329"}],"collection":[{"href":"http:\/\/preprints.lebedev.ru\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"http:\/\/preprints.lebedev.ru\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"http:\/\/preprints.lebedev.ru\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"http:\/\/preprints.lebedev.ru\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=4329"}],"version-history":[{"count":0,"href":"http:\/\/preprints.lebedev.ru\/index.php?rest_route=\/wp\/v2\/posts\/4329\/revisions"}],"wp:attachment":[{"href":"http:\/\/preprints.lebedev.ru\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=4329"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"http:\/\/preprints.lebedev.ru\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=4329"},{"taxonomy":"post_tag","embeddable":true,"href":"http:\/\/preprints.lebedev.ru\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=4329"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}