Production of high energy neutrinos in relativistic supernova shock waves

Details Production of high energy neutrinos in relativistic supernova shock waves Production of high energy neutrinos in relativistic supernova shock waves

Jan 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979duma.work.....w&link_type=abstract

Presented at the 1978 DUMAND Summer Workshop, San Diego, Calif., 11 Aug. 1978

Physics

High Energy Interactions, Neutrinos, Particle Production, Shock Waves, Supernovae, Bursts, Gamma Rays, Hadrons, Particle Collisions

Scientific paper

The possibility of producing high-energy neutrinos (approximately 10 GeV) in relativistic supernova shock waves is considered. It is shown that, even if the dissipation in such shocks is due to hard hadron-hadron collisions, the resulting flux of neutrinos is too small to be observed by currently envisioned detectors. The associated burst of hard gamma-rays, however, may be detectable.

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