Redshift Effects in Particle Production from Kerr Primordial Black Holes
Andrew Cheek, Lucien Heurtier, Yuber F. Perez-Gonzalez, Jessica Turner

TL;DR
This paper studies how the rotation of primordial black holes affects the production and redshift of dark radiation and dark matter, revealing a suppression in dark radiation signals and refining constraints on light dark matter candidates.
Contribution
It introduces a detailed analysis of redshift effects in particle emission from rotating black holes and provides a new computational tool, FRISBHEE, for modeling black hole evaporation in the early universe.
Findings
Rotation enhances higher-spin particle production.
Redshift effects suppress dark radiation by a factor of about 10.
Higher spin particles are more affected by late dilution and constraints.
Abstract
When rotating primordial black holes evaporate via Hawking radiation, their rotational energy and mass are dissipated with different dynamics. We investigate the effect of these dynamics on the production of dark radiation -- in the form of hot gravitons or vector bosons -- and non-cold dark matter. Although the production of higher-spin particles is enhanced while primordial black holes are rotating, we show that the energy density of dark radiation experiences an extra redshift because their emission effectively halts before PBH evaporation completes. We find that taking this effect into account leads to suppression by a factor of of for maximally rotating black holes as compared to previous results. Using the solution of the Friedmann and Boltzmann equations to accurately calculate the evolution of linear perturbations, we revisit the warm dark…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Pulsars and Gravitational Waves Research · Particle Accelerators and Free-Electron Lasers
