4.6 Article

Remnant Black Hole Kicks and Implications for Hierarchical Mergers

Journal

ASTROPHYSICAL JOURNAL LETTERS
Volume 918, Issue 2, Pages -

Publisher

IOP Publishing Ltd
DOI: 10.3847/2041-8213/ac20db

Keywords

-

Funding

  1. Department of Science and Technology, India [DST/SJF/PSA-01/2017-18]
  2. Science and Engineering Research Board of India [EMR/2016/005594]
  3. Infosys foundation
  4. NSF's LIGO Laboratory
  5. NSF support via NSF CAREER award [PHY-1653374]
  6. NSF [AST-2006384, PHY-2012083, PHY1836779]
  7. Italian Istituto Nazionale della Fisica Nucleare (INFN)
  8. Dutch Nikhef

Ask authors/readers for more resources

This study investigates the retention probability of remnants formed by hierarchical mergers in star clusters, based on the kick velocities imparted to the black hole remnants. Utilizing the gravitational-wave event database, it is found that star clusters with escape speeds of 200 km s(-1) can retain about 50% of the events in the second gravitational-wave transient catalog. The study highlights the significance of considering kick velocity inferences in future studies of hierarchical mergers.
When binary black holes merge in dense star clusters, their remnants can pair up with other black holes in the cluster, forming heavier and heavier black holes in a process called hierarchical merger. The most important condition for hierarchical merger to occur is that remnants formed by mergers are retained by the host star cluster. Using the publicly available gravitational-wave event database, we infer the magnitudes of kick velocities imparted to the remnant black holes due to anisotropic emission of gravitational waves and use that to quantify the retention probability of each event as a function of the escape speed of the star cluster. Among the second gravitational-wave transient catalog (GWTC-2) events, GW190814 provides the tightest constraint on the kick magnitude with V-kick=74(-7)(+10) km s(-1) at the 90% credible level. We find that star clusters with escape speeds of 200 km s(-1) can retain about 50% of the events in the GWTC-2. Using the escape speed distributions of nuclear star clusters and globular clusters, we find that similar to 17 (2) remnants of GWTC-2 may be retained by the host star cluster if all GWTC-2 events occurred in nuclear (globular) clusters. Our study demonstrates the importance of folding in kick velocity inferences in future studies of hierarchical mergers.

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

4.6
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

No Data Available
No Data Available