# MOCCA Survey Database I. BHs in star clusters

## TL;DR

The paper introduces the MOCCA Survey Database I, which compiles over 2000 star cluster models to study black hole formation, cluster dissolution, black hole mergers, and tidal disruption events.

## Contribution

It provides a comprehensive database of Monte Carlo star cluster models and initial analysis of black hole-related phenomena within these clusters.

## Key findings

- Insights into formation of intermediate mass black holes
- Understanding of cluster dissolution with black hole subsystems
- Data on black hole merger retention fractions

## Abstract

We briefly describe and discuss the set-up of the project MOCCA Survey Database I. The database contains more than 2000 Monte Carlo models of evolution of real star cluster performed with the MOCCA code. Then, we very briefly discuss results of analysis of the database regarding the following projects: formation of intermediate mass black holes, abrupt cluster dissolution harboring black hole subsystems, retention fraction of black hole - black hole mergers, and tidal disruption events with intermediate mass black holes.