21-cm constraints on spinning primordial black holes
arXiv:2108.13256 · doi:10.1088/1475-7516/2022/03/012
Abstract
Hawking radiation from primordial black holes (PBH) can ionize and heat up neutral gas during the cosmic dark ages, leaving imprints on the global 21-cm signal of neutral hydrogen. We use the global 21-cm signal to constrain the abundance of spinning PBHs in mass range of grams. We consider several extended PBH distribution models. Our results show that 21-cm can set the most stringent PBH bounds in our mass window. Compared with constraints set by {\it Planck} cosmic microwave background (CMB) data, 21-cm limits are more stringent by about two orders of magnitudes. PBHs with higher spin are typically more strongly constrained. Our 21-cm constraints for the monochromatic mass distribution rule out spinless PBHs with initial mass below , whereas extreme Kerr PBHs with reduced initial spin of are excluded as the dominant dark matter component for masses below . We also derived limits for the log-normal, power-law and critical collapse PBH mass distributions.
JCAP accepted version, references added, some minor typos corrected. 22 pages, 6 figures
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