Self-regulating the early growth of black holes through global warming

摘要: A decade after their first discovery, the origin of giant supermassive black holes (SMBHs), with masses in excess of 109 M⊙, at redshifts as early as z > 6, remains a puzzle. One possibility is that stellar-mass “seed” BHs, left behind by the first stars, accrete gas at close to the Eddington limit during a large fraction (≳ 50%) of the time. While maintaining such a high accretion rate may itself be difficult, here we focus on another, less commonly discussed problem in this scenario: unless BH seed formation and growth are preferentially suppressed in less massive protogalaxies, the mass density in SMBHs at z ∼ 6 already exceeds the locally observed SMBH mass density by several orders of magnitude. We show that the X-rays from the earliest accreting BHs themselves can cause a self-regulation, by partially ionizing and heating the intergalactic medium (IGM). This “global warming” suppresses the formation and …