γ-ray flash from relativistic shock accelerated particles in the Hypernova environment

Details γ-ray flash from relativistic shock accelerated particles in the Hypernova environment γ-ray flash from relativistic shock accelerated particles in the Hypernova environment

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..801..129m&link_type=abstract

ASTROPHYSICAL SOURCES OF HIGH ENERGY PARTICLES AND RADIATION. AIP Conference Proceedings, Volume 801, pp. 129-130 (2005).

Astronomy and Astrophysics

Astrophysics

Supernovae, Gamma-Ray Sources (Astronomical), Shock Waves, Acceleration, Supernovae, Gamma-Ray Sources, Gamma-Ray Bursts, Elementary Particle Processes, Hydrodynamics

Scientific paper

The observational signatures of relativistic shock break out at the surface of Hypernova star are investigated. The interaction of accelerated particles with the particles of circumstellar medium is considered. Particularly we analyze a gamma-ray flash as a result of neutral pion decay from inelastic p-p collisions and determine its detectability.

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