Regurgitated Dark Matter

Fuente: arXiv
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Hauptverfasser: Kim, TaeHun, Lu, Philip, Marfatia, Danny, Takhistov, Volodymyr
Format: Preprint
Veröffentlicht: 2023
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author Kim, TaeHun
Lu, Philip
Marfatia, Danny
Takhistov, Volodymyr
author_facet Kim, TaeHun
Lu, Philip
Marfatia, Danny
Takhistov, Volodymyr
contents We present a new paradigm for the production of the dark matter (DM) relic abundance based on the evaporation of early Universe primordial black holes (PBHs) themselves formed from DM particles. As a concrete realization, we consider a minimal model of the dark sector in which a first-order phase transition results in the formation of Fermiball remnants that collapse to PBHs, which then emit DM particles. We show that the regurgitated DM scenario allows for DM in the mass range $\sim1$ GeV $- \,10^{16}$ GeV, thereby unlocking parameter space considered excluded.
format Preprint
id arxiv_https___arxiv_org_abs_2309_05703
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Regurgitated Dark Matter
Kim, TaeHun
Lu, Philip
Marfatia, Danny
Takhistov, Volodymyr
High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
High Energy Astrophysical Phenomena
High Energy Physics - Experiment
We present a new paradigm for the production of the dark matter (DM) relic abundance based on the evaporation of early Universe primordial black holes (PBHs) themselves formed from DM particles. As a concrete realization, we consider a minimal model of the dark sector in which a first-order phase transition results in the formation of Fermiball remnants that collapse to PBHs, which then emit DM particles. We show that the regurgitated DM scenario allows for DM in the mass range $\sim1$ GeV $- \,10^{16}$ GeV, thereby unlocking parameter space considered excluded.
title Regurgitated Dark Matter
topic High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
High Energy Astrophysical Phenomena
High Energy Physics - Experiment
url https://arxiv.org/abs/2309.05703