Table 2
Binary black hole mergers above the upper-mass gap.
| IC | Isolated | Orig | DynA | DynB |
|---|---|---|---|---|
| (%) | (%) | (%) | (%) | |
| kro1 | 5.23 × 10−4 | 2.15 | 5.33 | 99.99 |
| kro5 | 0 | 60.63 | – | – |
| lar1 | 0 | 2.67 | 5.85 | 99.99 |
| lar5 | 4.32 × 10−3 | 65.27 | – | – |
| lar5che | 11.17 | 52.66 | 10.88 | 99.99 |
| log1 | 5.26 × 10−4 | 11.48 | 35.15 | 100 |
| log1che | 39.29 | 42.42 | 45.93 | 99.99 |
| log2 | 0 | 93.97 | – | – |
| log3 | 3.05 | 17.51 | – | – |
| log4 | 0 | 29.04 | – | – |
| log5 | 0.02 | 94.49 | – | – |
| top1 | 0 | 20.67 | 70.91 | 97.96 |
| top5 | 0.04 | 97.96 | – | – |
Notes. The first column reports the model name (see Table 1 and Appendix A for details), and the second column lists the percentage of isolated BBH mergers with m1 above the gap. The third, fourth, and fifth columns show the same fraction in the case of original, DynA, and DynB BBH mergers inside HM clusters.
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