Strange stars at finite temperature

Details Strange stars at finite temperature Strange stars at finite temperature

2006-02-04

arxiv.org/abs/astro-ph/0602095v1

J.Phys.Conf.Ser. 31 (2006) 107-110

Astronomy and Astrophysics

Astrophysics

To be published in the proceedings of The Third 21COE Symposium, held at Department of Physics, Waseda University, Tokyo, Japa

Scientific paper

10.1088/1742-6596/31/1/018

We calculate strange star properties, using large N_c approximation with built-in chiral symmetry restoration (CSM). We used a relativistic Hartree Fock mean field approximation method, using a modified Richardson potential with two scale parameters \Lambda and \Lambda^\prime, to find a new set of equation of states for strange quark matter. We take the effect of temperature (T) on gluon mass, in addition to the usual density dependence, and find that the transition T from hadronic matter to strange matter is 80 MeV. Therefore formation of strange stars may be the only signal for formation of QGP with asymptotic freedom and CSM.

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