Hierarchical black hole triples in young star clusters: impact of Kozai-Lidov resonance on mergers
Thomas O. Kimpson, Mario Spera, Michela Mapelli, Brunetto M. Ziosi

TL;DR
This study uses N-body simulations to analyze hierarchical black hole triples in young star clusters, revealing that Kozai-Lidov oscillations significantly increase merger rates and influence gravitational wave event interpretations.
Contribution
It introduces a new simulation approach including post-Newtonian effects to quantify the impact of Kozai-Lidov resonance on black hole merger rates in star clusters.
Findings
Kozai-Lidov oscillations occur in ~88% of simulated systems.
KL resonance causes 0.5% of systems to merge via increased eccentricity.
Accounting for KL oscillations raises the merger rate by ~50%.
Abstract
Mergers of compact object binaries are one of the most powerful sources of gravitational waves (GWs) in the frequency range of second-generation ground-based gravitational wave detectors (Advanced LIGO and Virgo). Dynamical simulations of young dense star clusters (SCs) indicate that ~27 per cent of all double compact object binaries are members of hierarchical triple systems (HTs). In this paper, we consider 570 HTs composed of three compact objects (black holes or neutron stars) that formed dynamically in N-body simulations of young dense SCs. We simulate them for a Hubble time with a new code based on the Mikkola's algorithmic regularization scheme, including the 2.5 post-Newtonian term. We find that ~88 per cent of the simulated systems develop Kozai-Lidov (KL) oscillations. KL resonance triggers the merger of the inner binary in three systems (corresponding to 0.5 per cent of the…
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