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