Adding an axion angle and vector repulsion to the SU(3) NJL model at finite temperature stiffens the equation of state and raises maximum proto-quark star masses to about 2.67 solar masses.
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Quark matter at finite temperature and proto-quark stars with the axion effects in SU(3) Nambu-Jona-Lasinio model
Adding an axion angle and vector repulsion to the SU(3) NJL model at finite temperature stiffens the equation of state and raises maximum proto-quark star masses to about 2.67 solar masses.