Pith. sign in

REVIEW

Micro black holes formed in the early Universe and their cosmological implications

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1811.05049 v1 pith:OU3UGQTS submitted 2018-11-12 gr-qc astro-ph.CO

classification gr-qcastro-ph.CO
keywords universeblackearlyhighholesremnantsscalesufficiently
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

High energy collisions of particles may have created tiny black holes in the early Universe, which might leave stable remnants instead of fully evaporating as a result of Hawking radiation. If the reheating temperature was sufficiently close to the fundamental gravity scale, which can be different from the usual Planck scale depending of the presence and properties of spatial extra-dimensions, the formation rate could have been sufficiently high and hence such remnants could account for the entire cold dark matter of the Universe.

Discussion (0). Sign in to comment.

Pith tools