Asymmetries from a charged memory-burdened PBH

Abstract We explore a purely gravitational origin of observed baryon asymmetry and dark matter (DM) abundance from asymmetric Hawking radiation of light primordial black holes (PBH) in presence of a non-zero chemical potential, originating from the space-time curvature. Considering the PBHs are described by a Reissner-Nordström metric, and are produced in a radiation dominated Universe, we show, it is possible to simultaneously explain the matter-antimatter asymmetry along with right DM abundance satisfying bounds from big bang nucleosynthesis, cosmic microwave background and gravitational wave energy density due to PBH density fluctuation. We also obtain the parameter space beyond the semiclassical approximation, taking into account the quantum effects on charged PBH dynamics due to memory burden.

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Publication Details

Journal
Journal of Cosmology and Astroparticle Physics
Published
2025-02-01
DOI
https://doi.org/10.1088/1475-7516/2025/02/052
Citations
7
Primary Topic
Low-power high-performance VLSI design
Type
article
Field-Weighted Citation Impact
5.11
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article

Asymmetries from a charged memory-burdened PBH

Kousik Loho, Óscar Zapata, Basabendu Barman
7 citations
Journal of Cosmology and Astroparticle Physics
Low-power high-performance VLSI design
5.11
article

Asymmetries from a charged memory-burdened PBH

Kousik Loho, Óscar Zapata, Basabendu Barman
article en
7 citations

Abstract

Abstract We explore a purely gravitational origin of observed baryon asymmetry and dark matter (DM) abundance from asymmetric Hawking radiation of light primordial black holes (PBH) in presence of a non-zero chemical potential, originating from the space-time curvature. Considering the PBHs are described by a Reissner-Nordström metric, and are produced in a radiation dominated Universe, we show, it is possible to simultaneously explain the matter-antimatter asymmetry along with right DM abundance satisfying bounds from big bang nucleosynthesis, cosmic microwave background and gravitational wave energy density due to PBH density fluctuation. We also obtain the parameter space beyond the semiclassical approximation, taking into account the quantum effects on charged PBH dynamics due to memory burden.

Journal of Cosmology and Astroparticle PhysicsVol. 2025(02)
Homi Bhabha National Institute (IN), Harish-Chandra Research Institute (IN), Universidad de Antioquia (CO), SRM University (IN)
Openalex Percentile: Top 5%
Low-power high-performance VLSI design
5.11
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