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Black hole remnants are not too fast to be dark matter

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arxiv 2105.01627 v2 pith:4AZK6EH5 submitted 2021-05-04 gr-qc astro-ph.COhep-ph

classification gr-qcastro-ph.COhep-ph
keywords darkmatterremnantsvelocitiesblackevaporationfinalhole
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We comment on recent claims that recoil in the final stages of Hawking evaporation gives black hole remnants large velocities, rendering them inviable as a dark matter candidate. We point out that due to cosmic expansion, such large velocities at the final stages of evaporation are not in tension with the cold dark matter paradigm so long as they are attained at sufficiently early times. In particular, the predicted recoil velocities are robustly compatible with observations if the remnants form before the epoch of big bang nucleosynthesis, a requirement which is already imposed by the physics of nucleosynthesis itself.

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Cited by 1 Pith paper

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

  1. The Case For Black Hole Remnants: A Review

    gr-qc 2024-11 unverdicted novelty 2.0 of 10

    A review arguing that black hole remnants remain viable and that the species and entropy objections to them are not decisive, so remnants could resolve the information paradox.

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