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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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