Microscopic nuclear equation of state at finite temperature and stellar stability
Nuclear Theory
2022-08-17 v1
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.
Keywords
Cite
@article{arxiv.2207.12146,
title = {Microscopic nuclear equation of state at finite temperature and stellar stability},
author = {Hong-Ming Liu and Jing Zhang and Zeng-Hua Li and Jin-Biao Wei and G. F. Burgio and H. -J. Schulze},
journal= {arXiv preprint arXiv:2207.12146},
year = {2022}
}
Comments
9 pages, 7 figures