On stimulated radiation of black holes

On stimulated radiation of black holes

The Unruh's thermal state in the vicinity of the event horizon of the black hole provides conditions where impinging particles can radiate other particles. The subsequent decays eventually lead to observable radiation of photons and neutrinos. Such radiation can be induced even by massive parti...

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Veröffentlicht in:5th International Workshop on The Dark Side Of The Universe 2009-01, Vol.1178 (1), p.142-146
1. Verfasser: Ridky, Jan
Format: Artikel
Sprache:eng
Schlagworte:
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
BLACK HOLES
COSMIC PHOTONS
GAMMA RADIATION
GRAVITATIONAL INTERACTIONS
MEV RANGE
NEUTRINO OSCILLATION
NEUTRINOS
NONLUMINOUS MATTER
PARTICLE DECAY
PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
PIONS NEUTRAL
STANDARD MODEL
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Zusammenfassung:The Unruh's thermal state in the vicinity of the event horizon of the black hole provides conditions where impinging particles can radiate other particles. The subsequent decays eventually lead to observable radiation of photons and neutrinos. Such radiation can be induced even by massive particles with gravitational interaction only. The hadronic particles would induce ~ 30 MeV gamma radiation from Delta *p(0) decays.
ISSN:0094-243X
1551-7616
DOI:10.1063/1.3264549