Black hole binary mergers in dense star clusters: the importance of primordial binaries
Jordan Barber, Debatri Chattopadhyay, Fabio Antonini

TL;DR
This paper investigates how primordial binaries in dense star clusters influence black hole binary mergers, highlighting the roles of cluster dynamics, escape velocity, and metallicity in shaping merger populations.
Contribution
It introduces a comprehensive analysis of primordial binary black hole formation and evolution within clusters, emphasizing the impact of cluster properties on merger outcomes.
Findings
Populations (i) and (ii) dominate BBH mergers in low escape velocity clusters.
Higher escape velocities increase the role of dynamical interactions in BBH evolution.
Primordial BBHs in low-metallicity clusters mainly interact with other BBHs, affecting merger rates.
Abstract
Dense stellar clusters are expected to house the ideal conditions for binary black hole (BBH) formation, both through binary stellar evolution and through dynamical encounters. We use theoretical arguments as well as -body simulations to make predictions for the evolution of BBHs formed through stellar evolution inside clusters from the cluster birth (which we term ), and for the sub-population of merging BBHs. We identify three key populations: (i) BBHs that form in the cluster, and merge before experiencing any dynamical interaction; (ii) binaries that are ejected from the cluster after only one dynamical interaction; and, (iii) BBHs that experience more than one strong interaction inside the cluster. We find that populations (i) and (ii) are the dominant source of all BBH mergers formed in clusters with escape velocity…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsAstrophysical Phenomena and Observations · Adaptive optics and wavefront sensing · Astronomy and Astrophysical Research
