Double inflation as a single origin of primordial black holes for all dark matter and LIGO observations
Keisuke Inomata, Masahiro Kawasaki, Kyohei Mukaida, Tsutomu T., Yanagida

TL;DR
This paper proposes a single inflation model that can produce primordial black holes across a broad mass spectrum, potentially accounting for all dark matter and explaining LIGO gravitational wave observations.
Contribution
It introduces a concrete inflationary scenario that generates PBHs spanning from subsolar to stellar masses, unifying dark matter and LIGO event explanations.
Findings
PBHs can constitute all dark matter within a broad mass range.
The model produces PBHs around 10^{-13} solar masses and 10 solar masses.
Uncertainty in microlensing constraints affects PBH abundance limits.
Abstract
Primordial Black Hole (PBH) is one of the leading non-particle candidates for dark matter (DM). Although several observations severely constrain the amount of PBHs, it is recently pointed out that there is an uncertainty on the microlensing constraints below which was ignored originally but may weaken the constraints significantly. In this paper, facing this uncertainty, we investigate the possibility that PBHs can make up all DM in a broad mass spectrum. Moreover, we propose a concrete inflation model which can simultaneously produce PBHs for all DM in a broad mass spectrum around and PBHs for LIGO events in a sharp mass spectrum at .
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