# Supermassive black holes and dark halo from the Bose-condensed dark matter

## TL;DR

This paper investigates the potential formation of supermassive black holes from Bose-Einstein condensate dark matter, analyzing collapse dynamics and mass distributions to understand their origins in galaxies.

## Contribution

It introduces a model where SMBHs form from BEC dark matter waves, considering collapse conditions, angular momentum effects, and axion interactions, providing new insights into galaxy core structures.

## Key findings

- BEC waves can collapse to form SMBHs under ideal conditions
- Realistic angular momentum prevents collapse of BEC into SMBHs
- Mass distribution functions of black holes within galaxies are derived

## Abstract

Most of the galaxies harbor supermassive Black Holes (SMBH) in their center. Some of them are observed in very high redshifts. We explore the possibility that SMBH form from the coherent waves of Bose-Einstein condensate (BEC) which are supposed to form the dark matter. We first study the isotropic and anisotropic collapses of BEC. We find the BEC wave can easily collapse to form SMBH but the realistic amount of angular momentum completely prevents the collapse. We further explore the Axion case with attractive interaction and find the moderate mass ratio between the SMBH and the dark halo around it. We also obtain the mass distribution function of BH within a single galaxy.