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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

Black hole remnants are not too fast to be dark matter

classification gr-qc astro-ph.COhep-ph
keywords darkmatterremnantsvelocitiesblackevaporationfinalhole
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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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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