arXiv:2207.12146·v1·Nuclear Theory
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
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.
Comments: 9 pages, 7 figures