Primordial Black Holes from Inflaton Fragmentation into Oscillons
Eric Cotner, Alexander Kusenko, Volodymyr Takhistov

TL;DR
This paper proposes a mechanism where inflaton fragmentation into oscillons during inflation can produce primordial black holes across a range of masses, potentially explaining dark matter and contributing to gravitational wave sources.
Contribution
It introduces a novel process linking inflaton fragmentation into oscillons with the formation of primordial black holes of various masses, including sublunar and solar-mass scales.
Findings
Primordial black holes of sublunar mass can form from inflaton fragmentation.
The mechanism can produce solar-mass black holes relevant for gravitational wave detection.
Primordial black holes could account for all dark matter.
Abstract
We show that fragmentation of the inflaton into long-lived spatially localized oscillon configurations can lead to copious production of black holes. In a single-field inflation model primordial black holes of sublunar mass can form, and they can account for all of the dark matter. We also explore the possibility that solar-mass primordial black holes, particularly relevant for gravitational wave astronomy, are produced from the same mechanism.
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