Supermassive black holes formed by direct collapse of inflationary perturbations
Tomohiro Nakama, Teruaki Suyama, Jun'ichi Yokoyama

TL;DR
This paper introduces a novel inflationary perturbation mechanism that produces primordial black holes massive enough to evolve into supermassive black holes, aligning with observational constraints and predicting their existence at very high redshifts.
Contribution
The model explains the formation of supermassive black holes via inflationary perturbations without conflicting with CMB spectral distortion limits, a new approach in early universe cosmology.
Findings
Primordial black holes can grow into supermassive black holes.
The mechanism avoids CMB distortion constraints from COBE/FIRAS.
Supermassive black holes may exist at higher redshifts than currently observed.
Abstract
We propose a mechanism of producing a new type of primordial perturbations that collapse to primordial black holes whose mass can be as large as necessary for them to grow to the supermassive black holes observed at high redshifts, without contradicting COBE/FIRAS upper limits on cosmic microwave background (CMB) spectral distortions. In our model, the observable Universe consists of two kinds of many small patches which experienced different expansion histories during inflation. Primordial perturbations large enough to form primordial black holes are realized on patches that experienced more Hubble expansion than the others. By making these patches the minor component, the rarity of supermassive black holes can be explained. On the other hand, most regions of the Universe experienced the standard history and, hence, only have standard almost-scale-invariant adiabatic perturbations…
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