Boosting Supermassive Black Hole Growth in the Early Universe by Fuzzy Dark Matter Solitons
H.-H. Sandy 懷萱 Chiu 邱, Hsi-Yu Schive, Hsiang-Yi Karen Yang, Hsinhao Huang, M. Gaspari
Abstract
Observations of massive supermassive black holes (SMBHs) in the early Universe challenge existing black hole formation models. We propose that soliton cores in fuzzy dark matter (FDM) offer a potential solution to this timing problem. Our FDM cosmological zoom-in simulations confirm that, for a particle mass ${m}_{\mathrm{FDM}}\ensuremath{\sim}{10}^{\ensuremath{-}22}\text{ }\text{ }\mathrm{eV}$, solitons are well developed at redshift $z\ensuremath{\sim}7$ with masses of $\ensuremath{\sim}{10}^{9}{M}_{\ensuremath{\bigodot}}$, comparable to the observed SMBHs. We then demonstrate using hydrodynamic simulations that, compared to cold dark matter, these high-$z$ massive FDM solitons with mass ${M}_{s}$ can provide additional gravitational potential to accrete gas and boost the Bondi accretion rate of a growing black hole seed with mass ${M}_{\mathrm{BH}}$ by up to 2--4 orders of magnitude, in the regime of efficient cooling and negligible radiation pressure. This accretion boosting mechanism is effective for ${10}^{\ensuremath{-}22}\ensuremath{\lesssim}{m}_{\mathrm{FDM}}\ensuremath{\lesssim}{10}^{\ensuremath{-}20}\text{ }\text{ }\mathrm{eV}$ and potentially beyond as long as ${M}_{s}>{M}_{\mathrm{BH}}$.