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Table 1
Comparison between RNS and XNS for rigidly rotating compact stars.
| Model | Ω | M | r e | rp/re | |||
| (×10-2) | RNS | XNS | RNS | XNS | RNS | XNS | |
|
|
|||||||
| BU0 | 0.000 | 1.400 | 1.400 | 8.13 | 8.13 | 1.00 | 1.00 |
| BU1 | 1.075 | 1.432 | 1.433 | 8.33 | 8.34 | 0.95 | 0.95 |
| BU2 | 1.509 | 1.466 | 1.468 | 8.58 | 8.56 | 0.90 | 0.90 |
| BU3 | 1.829 | 1.503 | 1.505 | 8.82 | 8.85 | 0.85 | 0.85 |
| BU4 | 2.084 | 1.543 | 1.455 | 9.13 | 9.15 | 0.80 | 0.80 |
| BU5 | 2.290 | 1.585 | 1.586 | 9.50 | 9.52 | 0.75 | 0.75 |
| BU6 | 2.452 | 1.627 | 1.629 | 9.95 | 9.98 | 0.70 | 0.70 |
| BU7 | 2.569 | 1.666 | 1.667 | 10.51 | 10.53 | 0.65 | 0.65 |
| BU8 | 2.633 | 1.692 | 1.693 | 11.26 | 11.30 | 0.60 | 0.60 |
| BU9 | 2.642 | 1.695 | 1.698 | 11.63 | 11.60 | 0.58 | 0.58 |
Notes. Gravitational masses are in units of M⊙, re, and rp are the equatorial and polar radii.
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