Comparison of Statistical Treatments for the Equation of State for Core-Collapse Supernovae

Neutrinos emitted during the collapse, bounce, and subsequent explosion provide information about supernova dynamics. The neutrino spectra are determined by weak interactions with nuclei and nucleons in the inner regions of the star, and thus the neutrino spectra are determined by the composition of...

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Bibliographic Details
Published in:	The Astrophysical journal Vol. 707; no. 2; pp. 1495 - 1505
Main Authors:	Souza, S. R, Steiner, A. W, Lynch, W. G, Donangelo, R, Famiano, M. A
Format:	Journal Article
Language:	English
Published:	United States IOP Publishing 20-12-2009
Subjects:	APPROXIMATIONS ASTROPHYSICS, COSMOLOGY AND ASTRONOMY BASIC INTERACTIONS BINARY STARS CALCULATION METHODS COSMIC NEUTRINOS COSMIC RADIATION ELEMENTARY PARTICLES ENERGY RANGE EQUATIONS EQUATIONS OF STATE ERUPTIVE VARIABLE STARS EXPLOSIONS FERMIONS INTERACTIONS IONIZING RADIATIONS LEPTONS MASS NUMBER MASSLESS PARTICLES MATTER MEV RANGE MEV RANGE 01-10 NEUTRINOS RADIATIONS SIMULATION SPECTRA STARS SUPERNOVAE VARIABLE STARS WEAK INTERACTIONS
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