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

TL;DR

This paper uses the Field Correlator Method to calculate properties of strange stars, showing that certain parameter values produce models consistent with observational data.

Contribution

It introduces a novel application of the Field Correlator Method to determine strange star properties aligning with astrophysical observations.

Findings

Strange star sequences match semi-empirical mass-radius data.

Specific gluon condensate values yield realistic critical temperatures.

Model consistency with observational constraints is demonstrated.

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 $G_2=0.006\;{\rm GeV}^4$ and $G_2=0.0068\;{\rm GeV}^4$, which give a critical temperature $T_c\sim170\;{\rm MeV}$ 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.