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arXiv · 2304.07184

Effects of Heat Conduction on Blocking off the Super-Eddington Growth of Black Holes at High Redshift

Norita Kawanaka·Kazunori Kohri
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Abstract

We investigate the effect of conductive heating of the gas surrounding a geometrically thick accretion disk on the growth of a black hole at high redshift. If a black hole is accreting the surrounding gas at a super-Eddington rate, the X-ray radiation from the vicinity of the black hole would be highly anisotropic due to the self-shielding of a geometrically thick accretion disk, and then the radiative feedback on the surrounding medium would be suppressed in the equatorial region, within which super-Eddington accretion can continue. However, if this region is sufficiently heated via thermal conduction from the adjacent region that is not shielded and heated by the X-ray irradiation, the surrounding gas becomes isotropically hot and the Bondi accretion rate would be suppressed and become sub-Eddington. We evaluate the condition under which such isotropic heating is realized, and derive new criteria required for super-Eddington accretion.

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Norita Kawanaka, Kazunori Kohri. 2023-04-14. Effects of Heat Conduction on Blocking off the Super-Eddington Growth of Black Holes at High Redshift. https://arxiv.org/abs/2304.07184

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