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arXiv · 2207.12146

Microscopic nuclear equation of state at finite temperature and stellar stability

Hong-Ming Liu·Jing Zhang·Zeng-Hua Li·Jin-Biao Wei·G. F. Burgio·H. -J. Schulze
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Abstract

A microscopic nuclear equation of state compatible with all current astrophysical constraints constructed within the Brueckner-Hartree-Fock formalism is presented and extended in a consistent way to finite temperature. The effects of finite temperature on the properties of neutron stars are studied in detail and a universal relation regarding stellar stability is proposed.

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Hong-Ming Liu, Jing Zhang, Zeng-Hua Li, Jin-Biao Wei, G. F. Burgio, H. -J. Schulze. 2022-07-25. Microscopic nuclear equation of state at finite temperature and stellar stability. https://doi.org/10.1103/physrevc.106.025801

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