Primordial Black Holes Arise When The Inflaton Falls
Keisuke Inomata, Evan McDonough, Wayne Hu

TL;DR
This paper shows that small, rapid changes in the inflaton potential during inflation can significantly amplify fluctuations, leading to primordial black hole formation that could account for dark matter or observed black holes.
Contribution
It introduces a novel mechanism where a small downward step in the inflaton potential during inflation enhances fluctuations, resulting in primordial black holes.
Findings
Small potential steps can produce significant PBH abundance.
PBHs from this mechanism could explain dark matter.
Black holes detected by gravitational waves may originate from this process.
Abstract
Primordial Black Holes (PBHs) have entered the forefront of theoretical cosmology, due their potential role in phenomena ranging from gravitational waves, to dark matter, to galaxy formation. While producing PBHs from inflationary fluctuations naively would seem to require a large deceleration of the inflaton from its velocity at the horizon exit of CMB scales, in this work we demonstrate that an acceleration from a relatively small downward step in the potential that is transited in much less than an e-fold amplifies fluctuations as well. Depending on the location of the step, such PBHs could explain dark matter or the black holes detected by the gravitational wave interferometers. The perturbation enhancement has a natural interpretation as particle production due to the non-adiabatic transition associated with the step.
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