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Primordial Black Holes and Quantum Effects

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arxiv 1402.1437 v1 pith:DLKU4JME submitted 2014-02-06 gr-qc astro-ph.CO

B. J. Carr This is my paper · ORCID
classification gr-qcastro-ph.CO
keywords pbhsquantumblackeffectsholesprimordialprobeuniverse
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abstract

Primordial black holes (PBHs) are of special interest because of the crucial role of quantum effects in their formation and evaporation. This means that they provide a unique probe of the early universe, high-energy physics and quantum gravity. We highlight some recent developments in the subject, including improved limits on the fraction of the Universe going into evaporating PBHs in the mass range $10^{9} - 10^{17}$ g and the possibility of using PBHs to probe a cosmological bounce.

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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. Four years of wide-field search for nanosecond optical transients with the TAIGA-HiSCORE Cherenkov array

    astro-ph.IM 2024-11 conditional novelty 5.0 of 10

    Four seasons of TAIGA-HiSCORE data show no nanosecond optical transients, setting an upper limit of about 1e-3 events per steradian per hour.

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