Table 3.
Parameters of various NS EoS models (Lasky et al. 2014; Ravi & Lasky 2014; Li et al. 2016a; Ai et al. 2018).
| EoS | MTOV (M⊙) | RM (km) | I (1045 g cm2) |
 (10−10 s ) |
 |
|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) | (6) |
| SLy | 2.05 | 9.99 | 1.91 | 1.60 | −2.75 |
| BSk20 | 2.17 | 10.17 | 3.50 | 3.39 | −2.68 |
| APR | 2.2 | 10 | 2.13 | 0.303 | −2.95 |
| GM1 | 2.37 | 12.05 | 3.33 | 1.58 | −2.84 |
| DDME2 | 2.48 | 12.09 | 5.85 | 1.966 | −2.84 |
| AB-N | 2.67 | 12.90 | 4.3 | 0.112 | −3.22 |
| AB-L | 2.71 | 13.70 | 4.7 | 2.92 | −2.82 |
| NL3ωρ | 2.75 | 12.99 | 7.89 | 1.706 | −2.88 |
Notes. Column 1: EoS name. Column 2: maximum mass for a non-rotating NS or Tolman-Oppenheimer-Volkoff (TOV) mass. Columns 3 and 4: radius and inertia of the NSs, respectively. Columns 5 and 6: parameters of the NS for each EoS, which are related to the maximum gravitational mass of a rotating NS as 
, where P is the rotational period.
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