Is there a maximum mass for black holes in galactic nuclei?
Kohei Inayoshi, Zoltan Haiman

TL;DR
This paper proposes a physical limit on the maximum mass of supermassive black holes in galactic nuclei, around 10^{10} to 10^{11} solar masses, due to accretion physics and star formation processes.
Contribution
It introduces a model linking small-scale accretion physics and star formation to the maximum SMBH mass, independent of galaxy properties or cosmology.
Findings
Maximum SMBH mass is between 1-6 x 10^{10} solar masses.
High accretion rates lead to star formation that limits black hole growth.
Transition to advection-dominated flow suppresses further accretion.
Abstract
The largest observed supermassive black holes (SMBHs) have a mass of M_BH ~ 10^{10} M_sun, nearly independent of redshift, from the local (z~0) to the early (z>6) Universe. We suggest that the growth of SMBHs above a few 10^{10} M_sun is prevented by small-scale accretion physics, independent of the properties of their host galaxies or of cosmology. Growing more massive BHs requires a gas supply rate from galactic scales onto a nuclear region as high as >10^3 M_sun/yr. At such a high accretion rate, most of the gas converts to stars at large radii (~10-100 pc), well before reaching the BH. We adopt a simple model (Thompson et al. 2005) for a star-forming accretion disk, and find that the accretion rate in the sub-pc nuclear region is reduced to the smaller value of at most a few M_sun/yr. This prevents SMBHs from growing above ~10^{11} M_sun in the age of the Universe. Furthermore, once…
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