Table 6.
Average rate for simulations of a given population to emit GWs within two of the prominent branches.
| NIMBH | Ncap. | ⟨Ncap.⟩ [Myr−1] | Nic | ⟨Nic⟩ [Myr−1] |
|---|---|---|---|---|
| GRX | ||||
| 10 | 24 | 0.36 | 22 | 0.96 |
| 15 | 16 | 0.62 | 48 | 1.9 |
| 20 | 5 | 0.36 | 61 | 3.5 |
| 25 | 5 | 0.62 | 57 | 4.5 |
| 30 | 4 | 0.32 | 63 | 5.6 |
| 35 | 0 | 0.00 | 78 | 7.3 |
| 40 | 0 | 0.00 | 91 | 7.6 |
| Hermite | ||||
| 10 | 0 | 0 | 28 | 0.09 |
| 20 | 0 | 0 | 71 | 1.9 |
| 30 | 0 | 0 | 101 | 3.8 |
| 40 | 0 | 0 | 86 | 6.6 |
Notes. Column 1: Cluster population. Column 2: Total number of unique binaries in the GW capture branch. Column 3: Rate at which GWs are emitted in the capture branch (hard eccentric binaries). Column 4: Total number of unique binaries in the in-cluster branch. Column 5: Rate at which GWs emit within the in-cluster merger branch (binary-single scatter).
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