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SUMMARY:Photon spectra from final stages of a primordial black hole evapor
 ation in different theoretical models
DTSTART;VALUE=DATE-TIME:20070709T181700Z
DTEND;VALUE=DATE-TIME:20070709T182900Z
DTSTAMP;VALUE=DATE-TIME:20260721T080418Z
UID:indico-contribution-505@cern.ch
DESCRIPTION:Speakers: Prof. BUGAEV\, Edgar (Institute for Nuclear Research
 \, Moscow\, Russia)\nPossibilities of an experimental search for gamma-ray
  bursts from primordial \nblack hole (PBH) evaporations in space are recon
 sidered. It is argued that the  \ncorresponding constraints which can be o
 btained in experiments with cosmic \nray detectors strongly depend on theo
 retical approach used for a description of \nthe PBH evaporation process. 
 Predictions of several theoretical models for \ngamma-ray spectra from fin
 al stages of PBH life (integrated over time) are given.\n\nhttps://indico.
 nucleares.unam.mx/event/4/session/98/contribution/505
LOCATION:Merida\, Mexico Uxmal + Tulum (Holiday Inn)
URL:https://indico.nucleares.unam.mx/event/4/session/98/contribution/505
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