Table B.1.
Properties of nonrotating NSs and rotating MSPs for the TM1 family.
| L | P | Mmax | ΔM | Req(max) | ΔR | ρc(max) | Req(1.4) | e1.4 | I1.4 | Req(2.0) | e2.0 |
|---|---|---|---|---|---|---|---|---|---|---|---|
| (MeV) | (ms) | (M⊙) | (%) | (km) | (%) | (fm−3) | (km) | (1) | (1045 g cm2) | (km) | (1) |
| 40 | 1 | 2.2441 | 5.57 | 12.545 | 6.02 | 0.8294 | – | – | – | 14.096 | 0.4901 |
| 40 | 2 | 2.1542 | 1.35 | 12.001 | 1.42 | 0.8907 | 13.605 | 0.3184 | 1.6010 | 13.017 | 0.2372 |
| 40 | 3 | 2.1383 | 0.60 | 11.909 | 0.64 | 0.8990 | 13.351 | 0.2128 | 1.6544 | 12.841 | 0.1568 |
| 40 | 5 | 2.1301 | 0.21 | 11.876 | 0.36 | 0.8990 | 13.226 | 0.1278 | 1.6818 | 12.753 | 0.0937 |
| 40 | static | 2.1256 | 0 | 11.833 | 0 | 0.9094 | 13.157 | 0 | – | 12.704 | 0 |
| 60 | 1 | 2.2408 | 5.59 | 12.647 | 6.88 | 0.8199 | – | – | – | 14.269 | 0.4987 |
| 60 | 2 | 2.1492 | 1.35 | 12.081 | 1.67 | 0.8805 | 13.850 | 0.3270 | 1.6176 | 13.104 | 0.2401 |
| 60 | 3 | 2.1330 | 0.60 | 11.960 | 0.65 | 0.8990 | 13.569 | 0.2183 | 1.6738 | 12.918 | 0.1586 |
| 60 | 5 | 2.1248 | 0.21 | 11.926 | 0.36 | 0.8990 | 13.433 | 0.1310 | 1.7024 | 12.824 | 0.0947 |
| 60 | static | 2.1202 | 0 | 11.883 | 0 | 0.9094 | 13.358 | 0 | – | 12.772 | 0 |
| 80 | 1 | 2.2432 | 5.79 | 12.788 | 6.69 | 0.8105 | – | – | – | 14.269 | 0.4987 |
| 80 | 2 | 2.1500 | 1.39 | 12.166 | 1.50 | 0.8805 | 14.181 | 0.3381 | 1.6580 | 13.270 | 0.2452 |
| 80 | 3 | 2.1335 | 0.61 | 12.068 | 0.68 | 0.8907 | 13.864 | 0.2256 | 1.7169 | 13.068 | 0.1619 |
| 80 | 5 | 2.1252 | 0.22 | 12.006 | 0.17 | 0.8990 | 13.710 | 0.1354 | 1.7468 | 12.968 | 0.0966 |
| 80 | static | 2.1205 | 0 | 11.986 | 0 | 0.8990 | 13.626 | 0 | – | 12.912 | 0 |
All configurations are computed within the Kepler limit, including the maximum rotational mass Mmax, the corresponding equatorial radius Req(max) and central number density ρc(max). ΔM (ΔR) refers to the change in the maximum mass (equatorial radius) with respect to the nonrotating configuration. The equatorial radius and the eccentricity of 1.4 M⊙, 2 M⊙ MSPs are also shown.
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