{"id":5646,"date":"2013-03-21T17:17:32","date_gmt":"2013-03-21T13:17:32","guid":{"rendered":"http:\/\/ellphi.lebedev.ru\/?p=5646"},"modified":"2013-04-05T15:15:34","modified_gmt":"2013-04-05T11:15:34","slug":"1973-en","status":"publish","type":"post","link":"http:\/\/preprints.lebedev.ru\/?p=5646","title":{"rendered":"1973 En"},"content":{"rendered":"

V.A. Tsarev<\/em> ,
\n \u2116 1 <\/strong> ASYMPTOTIC BEHAVIOR AS A CONSEQUENCE OF SUMMATION OF RESONANCE CONTRIBUTIONS IN CROSS CHANNEL
\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

High energy amplitude is constructed by summation of t-channel resonance contributions. Fixed cut and pairs of poles in complex J — plant are arised when width of resonances are taken into account. Properties of the model are discussed ---------------------------<\/div>\n<\/p>\n

A.S. Belousov<\/em> , N.P. Budanov<\/em> , B.B. Govorkov<\/em> , A.I. Lebedev<\/em> , K.I. Malinovsky<\/em> , E.V. Minarik<\/em> , I.V. Michailova<\/em> , V.P. Plaksin<\/em> , S.V. Rusakov<\/em> , V.I. Sergienko<\/em> , E.I. Tamm<\/em> , P.A. Cherenkov<\/em> , P.N. Sareyko<\/em> , A.I. Alikhanian<\/em> , G.L. Baiatian<\/em> , G.S. Vartanian<\/em> , A.T. Markanian<\/em> , A.M. Frolov<\/em> ,
\n \u2116 19 <\/strong> TOTAL HADRONIC PHOTOABSORPTION CROSS SECTIONS ON PROTON IN ENERGY REGION 12 — 30 GEV
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> <\/p>\n

V.A. Tsarev<\/em> ,
\n \u2116 35 <\/strong> PP DIffrACTIOn SLOPE AND «QuASIPOLE» MODE
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> <\/p>\n

M.S. Rabinovich<\/em> , V.N. Tsytovich<\/em> ,
\n \u2116 55 <\/strong> THE FUTURE OF NEW COLLECTIVE METHODS OF ACCELERARION
\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 general analysis of the future of different collective acceleration of charged particles, proposed by V.I.Veksler [l] is given ---------------------------<\/div>\n<\/p>\n

L.M. Ozernoy<\/em> , V.V. Usov<\/em> ,
\n \u2116 65 <\/strong> SOP\u0415RMASSIVE OBLIQUE R\u041e\u0422\u0410\u0422\u041eR: ELECTRODYNAMICS, EVOLUTION, OBSERVAT’IONAL TESTS
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> <\/p>\n

V.A. Tsarev<\/em> ,
\n \u2116 69 <\/strong> QUASIPOLE MODEL FOR HIGH ENERGY SCATtERING AMPLlTUDE
\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

»Quasipole» model for scattering amplitude is constructed by summation of cross channel resonance contributions. In this model Regge poles at t > 0 are on the first sheet of complex angular momentum plane, but at t\u2264t\u2264\u041e pass to the second sheet through the fixed cut which arrise due to resonance width. In some S — and t — region these poles are close to the real axis and determine properties of the amplitude imitating the presence of moving poles on the first sheet. The model explains recent data on elastic high energy pp scattering ---------------------------<\/div>\n<\/p>\n

\u042e.\u0412. \u0410\u0444\u0430\u043d\u0430\u0441\u044c\u0435\u0432<\/em> , \u0412.\u0410. \u0413\u0440\u0438\u0431\u043a\u043e\u0432<\/em> , \u041e.\u041d. \u041a\u0440\u043e\u0445\u0438\u043d<\/em> , \u0412.\u042f. \u041d\u0438\u043a\u0443\u043b\u0438\u043d<\/em> , \u0413.\u0412. \u0421\u043a\u043b\u0438\u0437\u043a\u043e\u0432<\/em> , \u041c.\u0410. \u0421\u0443\u043b\u0442\u0430\u043d\u043e\u0432<\/em> ,
\n \u2116 87 <\/strong> \u041a\u0423\u041c\u0423\u041b\u042f\u0422\u0418\u0412\u041d\u042b\u0415 \u042d\u0424\u0424\u0415\u041a\u0422\u042b \u0412 \u041b\u0410\u0417\u0415\u0420\u041d\u041e\u0419 \u041f\u041b\u0410\u0417\u041c\u0415 (\u0447\u0430\u0441\u0442\u044cI)
\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

High speed interferometry and soft X-ray filter diagnostic shows, that the collision of laser flares under the plane and cylindrical configurations leads to the plasma hunches with anomalous properties I TTl, high ionic polarisability, turbulent state. ---------------------------<\/div>\n<\/p>\n

L.M. Ozernoy<\/em> ,
\n \u2116 102 <\/strong> Dinamics of superclusters as the most powerful test for theories of galaxy formation.
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> <\/p>\n

N.I. Starkov<\/em> , V.A. Tsarev<\/em> , N.P. Zotov<\/em> ,
\n \u2116 103 <\/strong>ON A CONSISTENT DESCRIPTION OF AND DIFFErEnce
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> <\/p>\n

G.A. Askarjan<\/em> , W.A. Namiot<\/em> , M.S. Rabinovich<\/em> ,
\n \u2116 109 <\/strong> Application of super-high compression of matter by reactive ablation pressure for production of microcritical mass of fisser, production of superstrong magnetic field and acceleration of charged particles.
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> <\/p>\n

V.P. Frolov<\/em> ,
\n \u2116 114 <\/strong>Kerr-nut like space-nime with term.
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> <\/p>\n

V.O. Papanyan<\/em> , V.I. Ritus<\/em> ,
\n \u2116 115 <\/strong>\u0422\u041dREE-\u0420\u041d\u041e\u0422\u041eN INTERACTION AND PHOTOH SPLITTING IN \u0410N IN\u0422ENCE FIELD AND SCALE INVARIANCE
\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

<\/p>\n

The three-photon vertex function (the third-rank polari\u2116 zation tensor), which describes the Interaction of three real or virtual photons in an intense constant electromagnetic field of the fore E\u2534H,E=H is obtained
\n ---------------------------<\/div>\n<\/p>\n

E.L. Feinberg<\/em> ,
\n \u2116 125 <\/strong>Statistical and hydrodynamical modele of multiple hadron production.
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> <\/p>\n

L.M. Ozernoy<\/em> , L.E. Ulanovsky<\/em> ,
\n \u2116 141 <\/strong>On the theory of radio variability of galactic and quasar nuclei.
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> <\/p>\n

E.V. Aglitsky<\/em> , V.A. Boyko<\/em> , A.V. Vinogradov<\/em> , E.A. Yukov<\/em> ,
\n \u2116 145 <\/strong>The diagnostic of dense laser produced plasma from spectra of hydrogen-like and helium-like highly stripped ions.
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> <\/p>\n

Yu.M. Aleksandrov<\/em> , V.F. Grushin<\/em> , E.M. Leikin<\/em> , A.Ya. Rotvain<\/em> ,
\n \u2116 151 <\/strong>On the multipole amplitudes of pion photoproduction on protons obtained in the phenomenological analyses.
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> <\/p>\n

D.S. Chernavskii<\/em> , I.M. Dremin<\/em> , A.M. Dunaevskii<\/em> , I.I. Royzen<\/em> , E.I. Volkov<\/em> ,
\n \u2116 154 <\/strong>Multiperipherality at 70 Gev.
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> <\/p>\n

V.V. Musakhanyan<\/em> , A.I. Nikishov<\/em> ,
\n \u2116 156 <\/strong>On the Cherenkov raditiation change by external field.
\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 164 <\/strong>The remormalization in on non-abelian gauge theories.
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> <\/p>\n

A.V. Vinigradov<\/em> , I.I. Sobelman<\/em> , E.A. Yukov<\/em> ,
\n \u2116 173 <\/strong>On the spectroscopic methods for diagnostics of superdense hot plasmas.
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> <\/p>\n

V.M. Fyodorov<\/em> , Yu.A. Trubkin<\/em> ,
\n \u2116 175 <\/strong>On energy spectrum and absorption of cosmic muons.
\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

<\/p>\n

Avavlable experimental data on the differential energy spectrum of cosmic muons at sww level have been analysed in a single way by means of the least squares method. Then underground absortion curves calculated with the use of the obtained results and different rates of muon energy losses in matter are compared with the Kolar Gold Fields experimental data.
\n ---------------------------<\/div>\n<\/p>\n

D.I. Khomskii<\/em> , K.I. Kugel<\/em> ,
\n \u2116 177 <\/strong>Exchange-induced orbital ordering and magnetic structure of insulators with jahn-teller ions.
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> <\/p>\n

A.M. Frolov<\/em> ,
\n \u2116 185 <\/strong>Total hadronic photoabsorption cross section on neutron in energy region 12-30gev.
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> <\/p>\n

D.T. Alimov<\/em> , N.B. Delone<\/em> , B.A. Zon<\/em> , B.G. Katznelson<\/em>
\n \u2116 191 <\/strong>Investigations of high-excited state spectrum of a xenon atom in a strong light field.
\n\u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442<\/a> <\/p>\n","protected":false},"excerpt":{"rendered":"

V.A. Tsarev , \u2116 1 ASYMPTOTIC BEHAVIOR AS A CONSEQUENCE OF SUMMATION OF RESONANCE CONTRIBUTIONS IN CROSS CHANNEL \u0421\u043a\u0430\u0447\u0430\u0442\u044c \u043f\u0440\u0435\u043f\u0440\u0438\u043d\u0442 |\u0410\u043d\u043d\u043e\u0442\u0430\u0446\u0438\u044f| High energy amplitude is constructed by summation of t-channel resonance contributions. Fixed cut and pairs of poles in complex J — plant are arised when width of resonances are taken into account. Properties of […]<\/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\/5646"}],"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=5646"}],"version-history":[{"count":0,"href":"http:\/\/preprints.lebedev.ru\/index.php?rest_route=\/wp\/v2\/posts\/5646\/revisions"}],"wp:attachment":[{"href":"http:\/\/preprints.lebedev.ru\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=5646"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"http:\/\/preprints.lebedev.ru\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=5646"},{"taxonomy":"post_tag","embeddable":true,"href":"http:\/\/preprints.lebedev.ru\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=5646"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}