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Table 2.

Maximum mass configuration properties for various thermodynamical stellar conditions considered in this work.

EOS model MG (M) R (km) nc (fm−3) MB (M)
BL T = 0 2.080 10.26 1.156 2.456
BLh T = 0.1 2.070 10.18 1.175 2.457
BLh T = 5 2.072 10.00 1.162 2.457
BLh T = 10 2.073 10.05 1.158 2.457
BLh T = 30 2.090 10.31 1.141 2.449
BLh T = 50 2.112 10.91 1.084 2.406
BLh S/A = 1 2.076 10.37 1.141 2.446
BLh S/A = 2 2.082 10.81 1.098 2.390
BLh S/A = 3 2.088 11.97 0.992 2.296
BLh S/A = 1 ν 2.021 10.39 1.190 2.323
BLh S/A = 2 ν 2.034 10.92 1.129 2.289
BLh S/A = 3 ν 2.051 12.07 1.018 2.223

Notes. Stellar gravitational maximum mass MG, corresponding radius R, central baryon number density nc, and baryonic maximum mass MB. Stellar masses are given in units of solar mass M = 1.989 × 1033 g.

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