PROTO-NEUTRON AND NEUTRON STARS

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type 01 Apr 2010Embargo end date: 01 Jan 2008Publisher:World Scientific Pub Co Pte LtdJournal:Astronomy and Relativistic Astrophysics

Authors: Dexheimer, V.; Schramm, S.; Stoecker, H.;

doi: 10.1142/9789814304887_0004 , 10.48550/arxiv.0801.2523

arXiv: 0801.2523

PROTO-NEUTRON AND NEUTRON STARS

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Abstract

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.

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

Related Organizations

Goethe University Frankfurt
Germany
Johann Wolfgang Goethe-Universitaet
Germany

Keywords

Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

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