Multimessenger search for evaporating primordial black holes

E.V. Bugaev; P. A. Klimai; V.B. Petkov

Multimessenger search for evaporating primordial black holes

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arxiv 1912.01317 v1 pith:POW25IR6 submitted 2019-12-03 astro-ph.HE

V.B. Petkov , E.V. Bugaev , P. A. Klimai This is my paper · ORCID

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keywords pbhsblackevaporatingholesprimordialmultimessengersearchinguniverse

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Primordial black holes (PBHs) are black holes which may form in the early Universe through the gravitational collapse of primordial cosmological density fluctuations. Due to Hawking radiation these PBHs are supposed to evaporate by emitting particles. Recent developments in the experimental searching for evaporating PBHs in the local Universe are reviewed. The multimessenger techniques of searching for signals from evaporating PBHs are discussed.

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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

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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