Multimessenger search for evaporating primordial black holes V.B. Petkov, E.V. Bugaev, P.A. Klimai

Abstract

      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.

Reference:
V.B. Petkov, E.V. Bugaev, P.A. Klimai, "Multimessenger search for evaporating primordial black holes" in Proceedings of The International Conference "SN 1987A, Quark Phase Transition in Compact Objects and Multimessenger Astronomy", Russia, Terskol (BNO INR RAS), Nizhnij Arkhyz (SAO RAS), 2-8 July 2017, INR RAS, Moscow, 2018, ISBN 978-5-94274-327-7, pp. 158-164.
DOI: 10.26119/SAO.2020.1.52331
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