Protoneutron stars in the Brueckner-Hartree-Fock approach and finite-temperature kaon condensation

Details Protoneutron stars in the Brueckner-Hartree-Fock approach and finite-temperature kaon condensation Protoneutron stars in the Brueckner-Hartree-Fock approach and finite-temperature kaon condensation

2010-02-03

arxiv.org/abs/1002.0642v2

Phys.Rev.C81:025806,2010

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

10 pages, 5 figures, 2 tables, PRC in press

Scientific paper

10.1103/PhysRevC.81.025806

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.

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