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Possibilities of an experimental search for gamma-ray bursts from primordialblack hole (PBH) evaporations in space are reconsidered. It is argued that thecorresponding constraints which can be obtained in experiments with cosmic raydetectors strongly depend on theoretical approach used for a description of thePBH evaporation process. Predictions of several theoretical models forgamma-ray spectra from final stages of PBH life (integrated over time) aregiven.

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