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Strange stars at finite temperature

Subharthi Ray·Manjari Bagchi·Jishnu Dey·Mira Dey
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Abstract

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 Λand Λ^\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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Subharthi Ray, Manjari Bagchi, Jishnu Dey, Mira Dey. 2006-02-04. Strange stars at finite temperature. https://doi.org/10.1088/1742-6596%2F31%2F1%2F018

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