arXiv:1002.0642·v2·Solar and Stellar Astrophysics
Protoneutron stars in the Brueckner-Hartree-Fock approach and finite-temperature kaon condensation
A. Li🇨🇳 · X. R. Zhou🇨🇳 · G. F. Burgio🇮🇹 · H.-J. Schulze🇮🇹
Abstract
We study the properties of hot neutrino-trapped beta-stable stellar matter using an equation of state of nuclear matter within the Brueckner-Hartree-Fock approach including three-body forces, combined with a standard chiral model for kaon condensation at finite temperature. The properties of (proto)neutron stars are then investigated within this framework.
Comments: 10 pages, 5 figures, 2 tables, PRC in press