Limits on light primordial black holes from high-scale leptogenesis
arXiv:2305.13369 · doi:10.1103/PhysRevD.107.123537
Abstract
We investigate the role that the evaporation of light primordial black holes may have played in the production of the baryon asymmetry of the Universe through the high-scale leptogenesis. In particular, for mass of primordial black hole in the range [-] g, we find a dilution of thermally generated lepton asymmetry via entropy injection in the primordial plasma after the sphaleron freeze-out. As a consequence, we can put strong constraints on the primordial black hole parameters, showing the mutual exclusion limits between primordial black holes and high-scale leptogenesis. Remarkably, we point out an interplay between the upper bound on the initial abundance of primordial black holes and the active neutrino mass scale.
11 pages, 6 figures
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- Superradiant Leptogenesis
- High-Energy and Ultra-High-Energy Neutrinos from Primordial Black Holes
- Impact of memory-burdened black holes on primordial gravitational waves in light of Pulsar Timing Array
- Cosmological Origin of the KM3-230213A event and associated Gravitational Waves
- Impact of memory-burdened primordial black holes on high-scale leptogenesis
- High-energy gamma-ray emission from memory-burdened primordial black holes
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- Gravothermalizing into primordial black holes, boson stars, and cannibal stars
- Gravitational Wave Signatures of Primordial Black Hole Reheating in Upcoming Interferometry Missions
- Leptogenesis assisted by scalar decays
- Neutrino Emission and Plasma Heating from Primordial Black Holes: An Improved Approach to Constraints