Abstract:
In this paper, we explore the possibility of accreting primordial black holes as the source of heating
for the collapsing gas in the context of the direct collapse black hole scenario for the formation of super-massive
black holes (SMBHs) at high redshifts, z ∼ 6–7. One of the essential requirements for the direct collapse model
to work is to maintain the temperature of the in-falling gas at ≈104 K. We show that even under the existing
abundance limits, the primordial black holes of masses 10−2 M , can heat the collapsing gas to an extent
that the H2 formation is inhibited. The collapsing gas can maintain its temperature at 104 K till the gas reaches
a critical density nc ≈ 103 cm−3, at which the roto-vibrational states of H2 approaches local thermodynamic
equilibrium and H2 cooling becomes inefficient. In the absence of H2 cooling, the temperature of the collapsing
gas stays at ≈104 K even as it collapses further. We discuss scenarios of subsequent angular momentum removal
and the route to find collapse through either a supermassive star or a supermassive disk.
