Table 1.
Runs simulated and discussed in this paper.
| Run | EoS | q | Mchirp(M⊙) | M1(M⊙) | Mwind(M⊙) | Mdyn(M⊙) | ⟨vej⟩/c | ⟨Ye⟩ |
|---|---|---|---|---|---|---|---|---|
| 1 | DD2 | 1 | 1.22 | 1.4 | 3.708 × 10−2 | 4 × 10−4 | 0.22 | 0.17 |
| 2 | SFHo | 1 | 1.22 | 1.4 | 3 × 10−5 | 4 × 10−4 | 0.35 | 0.19 |
| 3 | DD2 | 1 | 1.39 | 1.6 | 5.88 × 10−3 | 1.2 × 10−3 | 0.24 | 0.14 |
| 4 | DD2 | 1 | 1.31 | 1.5 | 5.31 × 10−2 | 7.0 × 10−4 | 0.17 | 0.2 |
| 5 | DD2 | 1.036 | 1.23 | 1.44 | 4.32 × 10−2 | 5.0 × 10−4 | 0.2 | 0.17 |
| 6 | SFHo | 1.036 | 1.23 | 1.44 | 2.7 × 10−4 | 4.0 × 10−4 | 0.33 | 0.18 |
| 7 | LS220 | 1 | 1.22 | 1.4 | 1.37 × 10−2 | 1.4 × 10−3 | 0.17 | 0.14 |
| 8 | LS220 | 1.036 | 1.23 | 1.44 | 1.17 × 10−2 | 1.9 × 10−3 | 0.16 | 0.14 |
| 9 | LS220 | 1 | 1.31 | 1.5 | 4.80 × 10−4 | 3.0 × 10−4 | 0.19 | 0.08 |
| 10 | LS220 | 1 | 1.39 | 1.6 | 2.10 × 10−4 | 3.0 × 10−4 | 0.21 | 0.07 |
| 11 | LS220 | 1 | 1.49 | 1.71 | 1.80 × 10−4 | 3.0 × 10−4 | 0.22 | 0.08 |
| 12 | SFHo | 1.092 | 1.137 | 1.365 | 2.64 × 10−2 | 1.5 × 10−3 | 0.23 | 0.14 |
| 13 | SFHo | 1.17 | 1.128 | 1.4 | 3.52 × 10−2 | 1.2 × 10−3 | 0.2 | 0.14 |
| 14 | SFHo | 1 | 1.175 | 1.35 | 1.87 × 10−2 | 3.50 × 10−3 | 0.24 | 0.17 |
| A | LS220 | 1 | 1.188 | 1.365 | 2.16 × 10−2 | 1.6 × 10−3 | 0.16 | 0.22 |
| B | DD2 | 1 | 1.188 | 1.365 | 4.62 × 10−2 | 1.1 × 10−3 | 0.18 | 0.25 |
| C | SFHo | 1 | 1.188 | 1.365 | 5.67 × 10−3 | 2.8 × 10−3 | 0.21 | 0.23 |
| D | DD2 | 1.43 | 1.188 | 1.637 | 9.12 × 10−2 | 7.0 × 10−3 | 0.14 | 0.14 |
| E | LS220 | 1.43 | 1.188 | 1.637 | 5.34 × 10−2 | 7.3 × 10−3 | 0.17 | 0.16 |
| F | LS220 | 1.66 | 1.188 | 1.769 | 2.04 × 10−2 | 1.11 × 10−2 | 0.14 | 0.07 |
| G | DD2 | 1.22 | 1.188 | 1.509 | 6.27 × 10−2 | 2.50 × 10−3 | 0.17 | 0.19 |
| H | SFHo | 1.43 | 1.188 | 1.637 | 6.03 × 10−2 | 3.80 × 10−3 | 0.2 | 0.14 |
| I | SFHo | 1.66 | 1.188 | 1.769 | 5.31 × 10−2 | 1.50 × 10−3 | 0.12 | 0.07 |
Notes. Column Run is the label of the run, EoS is the Equation of State assumed in the Numerical Relativity (NR) simulation, q, Mchirp and M1 are the mass ratio, chirp mass and mass of the heavier NS, respectively; Mwind, Mdyn are the wind and dynamically ejected mass respectively (we take Mwind = 0.3 Mdisk as a prescription). ⟨vej⟩≡⟨vdyn⟩ and ⟨Ye⟩≡⟨Ye, dyn⟩ are the average ejecta velocity and electron fraction composition in the dynamically ejected material. Models 1-14 correspond to Radice et al. (2018) while A-I to Nedora et al. (2021).
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