... at the latest stages of the evolution (thousands of years) are magnetic dipole radiation, for radio pulsars, and gravitational waves radiation (D. R. Lorimer and M. Kramer, Handbook of Pulsar Astronomy, 2004) Neutrinos may significantly contribute to the ...
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Ссылки http://nuclphys.sinp.msu.ru/conf/lpp14/200809/Dvornikov.pdf -- 287.0 Кб -- 16.09.2009 Похожие документы
... NECKLACES V.B., A.Vilenkin, PRL 79, 5202, 1997 G H в U (1) H в Z2 m s 2 mass of monopole: m = 4 m /e, tension: µ = 2 s Due to gravitationalradiation, strings shrink, and monopoles inevitably annihilate. ...
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Ссылки http://nuclphys.sinp.msu.ru/neutrino/Berezinsky-14-04-2010.pdf -- 1320.6 Кб -- 25.04.2011 Похожие документы
... The energies and intensities of the thermal radiation being due to the accretion of baryons onto mini-holes exceed the corresponding values for the dipole radiation of the graviatoms providing the baryons' sizes to be neglected. ...
... 17.50 G.Hammond (SUPA, Univ. of Glasgow) Gravitational Wave Astronomy (25 min) . ... related to the search for neutrino radiation from SN1987A: commentary (20 min ... Radiative and hadronic decays of vector mesons in the gauge model of quark-meson ...
... 215I 15y12-Prosper p. 47 Check: Tc M 2/3 1/3 c 15y12-Prosper p. 48 Check: Tc M 2/3 1/3 c 15y12-Prosper p. 49 If radiation dominates in P When plasma is radiation-dominated (for massive 4 stars), then, P T , and Tc M 1/6 1/3 c . ...
... Moore, Stadel, 2005) Remnants (cores) of clumps gravitational shocks (E )j E - rough ... in the units of density at matter-radiation equality eq in dependence on the loop ...
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Ссылки http://nuclphys.sinp.msu.ru/conf/lpp14/210809/Berezinsky_Dokuch_Erosh.pdf -- 233.2 Кб -- 16.09.2009 Похожие документы