Strange stars properties calculated in the framework of the Field Correlator Method

Abstract

We calculate the strange star properties in the framework of the Field Correlator Method. We find that for the values of the gluon condensate $G_2=0.006{\mathrm{GeV}}^4$ and $G_2=0.0068{\mathrm{GeV}}^4$, which give a critical temperature $T_c\sim 170\mathrm{MeV}$ at ${\mu }_c=0$, the sequences of strange stars are compatible with some of the semi-empirical mass-radius relations and data obtained from astrophysical observations.

26 pages, 10 figures

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• Low mass strange stars and the compact star 1E1207.4-5209 in the Field Correlator Method