Gravitational Wave observatories may be able to detect hyperbolic encounters of Black Holes

TL;DR

This paper investigates the potential for ground-based gravitational wave detectors to observe hyperbolic encounters of black holes in dense star clusters, estimating detection rates and emphasizing their significance for understanding black hole populations.

Contribution

It provides the first detailed estimation of detection rates for hyperbolic black hole encounters using realistic cluster models and discusses their implications for astrophysics.

Findings

Detection of such encounters could occur within the next few years.

Estimated detection rates are one to few events per year with current and future observatories.

Actual detection rates may be higher due to outliers in large populations.

Abstract

Gravitational Wave (GW) astronomy promises to observe different kinds of astrophysical sources. Here we explore the possibility of detection of GWs from hyperbolic interactions of compact stars with ground-based interferometric detectors. It is believed that a bound compact cluster, such as a globular cluster, can be a primary environment for these interactions. We estimate the detection rates for such events by considering local geometry within the cluster, accounting for scattering probability of compact stars at finite distances, and assuming realistic cluster properties guided by available numerical models, their formation times, and evolution of stars inside them. We find that, even in the conservative limit, it may be possible to detect such black hole encounters in the next few years by the present network of observatories with the ongoing sensitivity upgrades and one to few events per year with the next generation observatories. In practice, actual detection rates can significantly surpass the estimated average rates, since the chances of finding outliers in a very large population can be high. Such observations (or, no observation) may provide crucial constraints to estimate the number of isolated compact stars in the universe. These detections will be exciting discoveries on their own and will be complimentary to observations of binary mergers bringing us one step closer to address a fundamental question, how many black holes are there in the observable universe.