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

【摘要】：正We study the properties of hot neutrino-trappedβ-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 approach.