... with M > 10M is quite different from low massstars, and what happens at M 100M 51 ... 52 The carbon-oxygen cores of low massstars turn out to be degenerate at the moment ...
... stars might be either evolved low luminocity ones or dead by now, and together with BH they could make (all?) cosmological DM ... 62 EXOTIC EVENTS Similar massstar-antistar collision, -bursters (???): E 1048 er g Annihilation apart. ...
... stars: an overview If a degenerate core (or white dwarf) exceeds the Chandrasekhar ... star is that for which the surface layers are "in orbit" The actual angular ... star surface: ua(in)(R,)=ua(out)(R,) ( 2 E a ) =-Va + 4Va + ma Energy has a ...
[
Текст
]
Ссылки http://nuclphys.sinp.msu.ru/conf/lpp14/200809/Dvornikov.pdf -- 287.0 Кб -- 16.09.2009 Похожие документы
... The standard model for a type II supernova is a massivestar that has reached a point in its evolution when the pressure from fusion reactions can not support the gravitational pressure of the outer regions. ...
... mass states (originally SLv was considered for the case of equal masses of neutrino in initial and final states) The rate of the process provided by the transition magnetic moment is of the same order as provided by the diagonal one The energy spectrum of ...
[
Текст
]
Ссылки http://nuclphys.sinp.msu.ru/neutrino/Lokhov-02-11-2010.pdf -- 1907.6 Кб -- 25.04.2011 Похожие документы
... mass function and numb er density of clumps dM dM 0.02(n + 3) M M (r ) DM ncl (M , R ... mass function 1014 dlog M , Mpc 3 1012 3 kpc 1010 dn M 8.5 kpc 108 10 8 10 6 10 4 MM ...
[
Текст
]
Ссылки http://nuclphys.sinp.msu.ru/conf/lpp14/210809/Berezinsky_Dokuch_Erosh.pdf -- 233.2 Кб -- 16.09.2009 Похожие документы
... Mass of the nearest supermassive black in the Galactic center M = (4.2 ± 0.2) 106 M Previously known value: M = (4.1 ± 0.4) 106 M The nearest supermassive black hole rotates not very fast a = 0.65 ± 0.05 Identification of quasi-perio dic oscillations from ...
... to nuclear matter EOS; neutron stars Krivoruchenko, Simkovic, Faessler, 2009 the fact that the bounds are similar to ours is not surprising: V g 2 /µ2 , so precision data on np - scattering compete with information from observations of neutron stars ...
... while the fundamental mass parameter M (higher-dimensional Planck mass) is taken of ... Massive modes Fourier components with n = 0 can be suitably rearranged to form an ...