Protoneutron stars in the Brueckner-Hartree-Fock approach and finite-temperature kaon condensation
arXiv:1002.0642 · doi:10.1103/PhysRevC.81.025806
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.
10 pages, 5 figures, 2 tables, PRC in press