Proto-Neutron and Neutron Stars

Details Proto-Neutron and Neutron Stars Proto-Neutron and Neutron Stars

2008-01-16

arxiv.org/abs/0801.2523v1

Astronomy and Astrophysics

Astrophysics

Prepared for International Workshop on Astronomy and Relativistic Astrophysics (IWARA 2007), Joao Pessoa, Brazil, 3-6 Oct 2007

Scientific paper

The parity doublet model, containing the SU(2) multiplets including the
baryons identified as the chiral partners of the nucleons is applied to neutron
stars. The maximum mass for the star is calculated for different stages of the
cooling taking into account finite temperature/entropy effect, trapped
neutrinos and fixed baryon number. Rotation effects are also included.

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