Photon spectra from final stages of a primordial black hole evaporation in different theoretical models

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dc.creatorBugaev, Edgar
dc.creatorKlimai, Peter
dc.creatorPetkov, Valery
dc.date2007-06-26
dc.date.accessioned2026-07-07T12:27:46Z
dc.date.available2026-07-07T12:27:46Z
dc.descriptionPossibilities of an experimental search for gamma-ray bursts from primordial black hole (PBH) evaporations in space are reconsidered. It is argued that the corresponding constraints which can be obtained in experiments with cosmic ray detectors strongly depend on theoretical approach used for a description of the PBH evaporation process. Predictions of several theoretical models for gamma-ray spectra from final stages of PBH life (integrated over time) are given.
dc.descriptionContribution to the 30th International Cosmic Ray Conference, Merida, Mexico, July 2007; 4 pages, 5 figures
dc.identifierhttps://arxiv.org/abs/0706.3778
dc.identifierhttp://arxiv.org/abs/0706.3778
dc.identifierProc. of the 30th International Cosmic Ray Conference; R. Caballero et al (eds.); Universidad Nacional Autonoma de Mexico, Mexico City, Mexico, 2008; Vol. 3 (OG part 2), pages 1123-1126
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/215319
dc.subjectAstrophysics
dc.titlePhoton spectra from final stages of a primordial black hole evaporation in different theoretical models
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