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arxiv: hep-th/0703070 · v2 · submitted 2007-03-08 · ✦ hep-th · astro-ph

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Reheating, Dark Matter and Baryon Asymmetry: a Triple Coincidence in Inflationary Models

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classification ✦ hep-th astro-ph
keywords observedasymmetrybaryondarkepochforminflationarymatter
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A scenario in which primeval black holes (PBHs) form at the end of an extended inflationary period is capable of producing, via Hawking radiation, the observed entropy, as well as the observed dark matter density in the form of Planck mass relics. The observed net baryon asymmetry is produced by sphaleron processes in the domain wall surrounding the PBHs as they evaporate around the electroweak transition epoch. The conditions required to satisfy these three observables determines the PBH formation epoch, which can be associated with the end of inflation, at $t\sim 10^{-32}\s$.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Constraints on Primordial Black Holes

    astro-ph.CO 2020-02 accept novelty 4.0

    Updated compilation shows PBHs are tightly constrained across 55 orders of magnitude in mass, ruling out dominant dark matter contributions except in narrow windows, with many limits carrying observational uncertainties.