Mergers of Stellar-Mass Black Holes in Nuclear Star Clusters

TL;DR

This paper proposes nuclear star clusters as promising environments for stellar-mass black hole mergers, estimating detectable gravitational wave events and highlighting their advantages over other environments.

Contribution

It introduces nuclear star clusters as a key environment for black hole mergers and provides simulation-based estimates of detection rates for gravitational wave observatories.

Findings

Nuclear star clusters can retain black holes due to high escape speeds.

Simulations suggest at least tens of detectable events per year with Advanced LIGO.

Nuclear star clusters are more promising than globular clusters for black hole mergers.

Abstract

Mergers between stellar-mass black holes will be key sources of gravitational radiation for ground-based detectors. However, the rates of these events are highly uncertain, given that such systems are invisible. One formation scenario involves mergers in field binaries, where our lack of complete understanding of common envelopes and the distribution of supernova kicks has led to rate estimates that range over a factor of several hundred. A different, and highly promising, channel involves multiple encounters of binaries in globular clusters or young star clusters. However, we currently lack solid evidence for black holes in almost all such clusters, and their low escape speeds raise the possibility that most are ejected because of supernova recoil. Here we propose that a robust environment for mergers could be the nuclear star clusters found in the centers of small galaxies. These clusters have millions of stars, black hole relaxation times well under a Hubble time, and escape speeds that are several times those of globulars, hence they retain most of their black holes. We present simulations of the three-body dynamics of black holes in this environment and estimate that, if most nuclear star clusters do not have supermassive black holes that interfere with the mergers, at least several tens of events per year will be detectable with Advanced LIGO.