Hyperon stars at finite temperature in the Brueckner theory
Solar and Stellar Astrophysics
2015-03-17 v1 Nuclear Theory
Abstract
We perform Brueckner-Hartree-Fock calculations of hypernuclear matter at finite temperature and provide convenient analytical parametrizations of the results. We study then the properties of (proto)neutron stars containing hyperons. We find important effects of trapping and finite temperature on the structure of hyperonic stars.
Keywords
Cite
@article{arxiv.1101.0726,
title = {Hyperon stars at finite temperature in the Brueckner theory},
author = {G. F. Burgio and H. -J. Schulze and A. Li},
journal= {arXiv preprint arXiv:1101.0726},
year = {2015}
}
Comments
6 pages, 5 figures, accepted for publication in Phys. Rev. C