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Table 1.
List of the BNS merger simulations considered in this work.
| EOS | MA [M⊙] | MB [M⊙] | q | Viscosity | Remnant | Refs. |
|---|---|---|---|---|---|---|
| BLh | 1.364 | 1.364 | 1.00 | NO | Long-lived | Nedora et al. (2021) |
| DD2 | 1.364 | 1.364 | 1.00 | NO | Long-lived | Nedora et al. (2019) |
| SFHo | 1.364 | 1.364 | 1.00 | YES | Very short-lived | Bernuzzi et al. (2020) |
| BLh | 1.146 | 1.635 | 1.43 | YES | Long-lived | Nedora et al. (2021) |
Notes. The nuclear equation of state is listed under EOS, MA and MB are the gravitational masses of the binary, and q = MB/MA is the binary mass ratio.
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