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Primordial Black Holes

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arxiv 1503.01166 v1 pith:3TNHDCNE submitted 2015-03-03 astro-ph.HE

Jane H MacGibbon , Tilan N. Ukwatta , J.T. Linnemann , S.S. Marinelli , D. Stump , K. Tollefson This is my paper · ORCID
classification astro-ph.HE
keywords blackholespbhsburstgamma-rayprimordialradiationbackground
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Primordial Black Holes (PBHs) are of interest in many cosmological contexts. PBHs lighter than about 1012 kg are predicted to be directly detectable by their Hawking radiation. This radiation should produce both a diffuse extragalactic gamma-ray background from the cosmologically-averaged distribution of PBHs and gamma-ray burst signals from individual light black holes. The Fermi, Milagro, Veritas, HESS and HAWC observatories, in combination with new burst recognition methodologies, offer the greatest sensitivity for the detection of such black holes or placing limits on their existence.

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Cited by 1 Pith paper

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  1. Connecting the Higgs Potential and Primordial Black Holes

    hep-ph 2019-09 conditional novelty 6.0 of 10

    A percolation calculation connects the Higgs potential parameters to the allowed masses and formation temperatures of primordial black holes, excluding regions where vacuum decay bubbles would have destroyed the universe.

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