Tabulated equation of state for supernova matter including full nuclear ensemble

Abstract

This is an introduction to the tabulated data base of stellar matter properties calculated within the framework of the Statistical Model for Supernova Matter (SMSM). The tables present thermodynamical characteristics and nuclear abundances for 31 values of baryon density (10${}^{-8}<\rho /{\rho }_0<$0.32, ${\rho }_0$=0.15 fm${}^{-3}$ is the normal nuclear matter density), 35 values of temperature ($0.2<T<25$ MeV) and 28 values of electron-to-baryon ratio ($0.02<Y_e<0.56$). The properties of stellar matter in $\beta$-equilibrium are also considered. The main ingredients of the SMSM are briefly outlined, and the data structure and content of the tables are explained.

10 pages, 8 figures, submitted to Astr.Phys. Jour. (2013)

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• Nuclear Equation of state for Compact Stars and Supernovae
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• Hard-core Radius of Nucleons within the Induced Surface Tension Approach
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