The cosmic coincidences of primordial-black-hole dark matter
arXiv:2109.09875 · doi:10.1103/PhysRevLett.128.031102
Abstract
If primordial black holes (PBHs) contribute more than 10 percent of the dark matter (DM) density, their energy density today is of the same order as that of the baryons. Such a cosmic coincidence might hint at a mutual origin for the formation scenario of PBHs and the baryon asymmetry of the Universe. Baryogenesis can be triggered by a sharp transition of the rolling rate of inflaton from slow-roll to (nearly) ultraslow-roll phases that produces large curvature perturbations for PBH formation in single-field inflationary models. We show that the baryogenesis requirement drives the PBH contribution to DM, along with the inferred PBH mass range, the resulting stochastic gravitational wave background frequency window, and the associated cosmic microwave background tensor-to-scalar ratio amplitude, into potentially observable regimes.
7 pages, 3 figures, version matched with publication (Editors' Suggestion)
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Cited by in corpus (5)
- Baryogenesis, Primordial Black Holes and MHz-GHz Gravitational Waves
- Induced gravitational waves from the cosmic coincidence
- Constraints on ultra-slow-roll inflation from the third LIGO-Virgo observing run
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