A standard source for high energy neutrino astronomy

Details A standard source for high energy neutrino astronomy A standard source for high energy neutrino astronomy

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....8..148b&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 8 p 148-151 (SEE N85-36066 24-93)

Computer Science

Decay, High Energy Interactions, Neutrinos, Proton-Proton Reactions, Cosmic Rays, Detection, Flux Density, Kaons, Muons, Particle Acceleration, Radiation Detectors, Resolution

Scientific paper

The authors discuss a standard source of high energy neutrinos composed of a source of accelerated particles imbedded in a cloud of low density gas. The main mechanism of neutrino production in the source is pp-collision, and the main process of detection is through muons produced underground by the neutrinos. The flux of neutrino-produced muons is computed for sources with different spectral index.

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