Neutrino mechanism of thermonuclear burning of carbon, formation of neutrino stars, and supernova outbursts
Gershtein S.S. , Ivanova L.N., Imshennik V.S., Khlopov M.Yu., Chechetkin V.M.
Allowance for the neutrino energy transport in explosions of carbon nuclei of stars leads, at densities 3Xl09<pc< 8.4 χ 109g/cm3, to an expansion with kinetic energy up to 1051 erg (supernova of type II), and leads at pc> 8.4xl09g/cm3 to the production of neutron stars with Μ~1.4ΜΘ and to the envelope destruction typical of supernovas of type I.