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arXiv · 1002.0642

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

A. Li·X. R. Zhou·G. F. Burgio·H. -J. Schulze
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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.

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A. Li, X. R. Zhou, G. F. Burgio, H. -J. Schulze. 2010-02-04. Protoneutron stars in the Brueckner-Hartree-Fock approach and finite-temperature kaon condensation. https://doi.org/10.1103/physrevc.81.025806

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