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

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

2007-06-26

arxiv.org/abs/0706.3778v1

Proc. of the 30th International Cosmic Ray Conference; R. Caballero et al (eds.); Universidad Nacional Autonoma de Mexico, Mex

Astronomy and Astrophysics

Astrophysics

Contribution to the 30th International Cosmic Ray Conference, Merida, Mexico, July 2007; 4 pages, 5 figures

Scientific paper

Possibilities 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.

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