Stellar core collapse - Numerical model and infall epoch

The core infall stage of the final evolution of a ten solar mass star is studied using an accurate and detailed numerical model. The features of the model include a realistic initial model and equation of state, general relativistic hydrodynamics, independent treatment of neutrino pairs, multigroup...

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Veröffentlicht in:	Astrophys. J., Suppl. Ser.; (United States) Suppl. Ser.; (United States), 1985-08, Vol.58, p.771-841
1. Verfasser:	Bruenn, S W
Format:	Artikel
Sprache:	eng
Schlagworte:	640102 - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources BARYONS BASIC INTERACTIONS CAPTURE CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS COSMIC NEUTRINOS COSMIC RADIATION DATA DENSITY DIAGRAMS ELECTRON CAPTURE ELEMENTARY PARTICLES ENERGY TRANSFER ENTROPY FERMIONS FLUID MECHANICS GRAVITATIONAL COLLAPSE HADRONS HEAT TRANSFER HYDRODYNAMICS INFORMATION INTERACTIONS IONIZING RADIATIONS LEPTONS LUMINOSITY MASSLESS PARTICLES MATHEMATICS MECHANICS NEUTRINOS NUMERICAL ANALYSIS NUMERICAL DATA OPTICAL PROPERTIES PHYSICAL PROPERTIES RADIANT HEAT TRANSFER RADIATIONS STAR EVOLUTION STARS THEORETICAL DATA THERMODYNAMIC PROPERTIES WEAK INTERACTIONS
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