Neutrino Radiation-Hydrodynamics: General Relativistic versus Multidimensional Supernova Simulations
نویسندگان
چکیده
منابع مشابه
Protoneutron star evolution and the neutrino driven wind in general relativistic neutrino radiation hydrodynamics simulations
Massive progenitor stars end their life in an explosion event with kinetic energies of the order 1051 erg. Behind the explosion ejecta, the low density and high entropy region formed immediately after the explosion is subject to neutrino heating. The neutrinos emitted from the remnant at the center, a protoneutron star (PNS), continually heat the material above the PNS surface. This heat is par...
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ژورنال
عنوان ژورنال: Progress of Theoretical Physics Supplement
سال: 2010
ISSN: 0375-9687
DOI: 10.1143/ptps.186.87