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arXiv · 1512.06196

A Complete Equation of State for Astrophysical Simulations

Hong Shen
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Abstract

We construct a complete equation of state (EOS) covering a wide range of temperature, proton fraction, and baryon density for the use of astrophysical simulations. We employ the relativistic mean-field (RMF) theory to describe nuclear interactions and adopt the Thomas-Fermi approximation to describe the nonuniform nuclear matter. The uniform matter and nonuniform matter are studied consistently using the same RMF theory.

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Hong Shen. 2015-12-19. A Complete Equation of State for Astrophysical Simulations. https://arxiv.org/abs/1512.06196

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