MOCCA-SURVEY data base II - Properties of intermediate mass black holes escaping from star clusters

In this work, we investigate properties of intermediate-mass black holes (IMBHs) that escape from star clusters due to dynamical interactions. The studied models were simulated as part of the preliminary second survey carried out using the MOCCA code (MOCCA-SURVEY Database II), which is based on the Monte Carlo N-body method and does not include gravitational wave recoil kick prescriptions of the binary black hole merger product. We have found that IMBHs are more likely to be formed and ejected in models where both initial central density and central escape velocities have high values. Most of our studied objects escape in a binary with another black hole (BH) as their companion and have masses between 100 and 140 M o . Escaping IMBHs tend to build-up mass most effectively through repeated mergers in a binary with BHs due to gravitational wave emission. Binaries play a key role in their ejection from the system as they allow these massive objects to gather energy needed for escape. The binaries in which IMBHs escape tend to have very high binding energy at the time of escape and the last interaction is strong but does not involve a massive intruder. These IMBHs gain energy needed to escape the cluster gradually in successive dynamical interactions. We present specific examples of the history of IMBH formation and escape from star cluster models. We also discuss the observational implications of our findings as well as the potential influence of the gravitational wave recoil kicks on the process.

Automated summary

In this study, properties of intermediate-mass black holes (IMBHs) that escape from star clusters due to dynamical interactions were investigated. The simulation models showed that high initial central density and central escape velocities increase the likelihood of IMBH formation and ejection. The majority of escaping IMBHs form binaries with other black holes and have masses between 100 and 140 M o . Escape is facilitated through repeated mergers in these binaries, with gravitational wave emission playing a key role. The study also discusses the observational implications and potential influence of gravitational wave recoil kicks on the process.