Neutrino astronomy and the atmospheric background

Details Neutrino astronomy and the atmospheric background Neutrino astronomy and the atmospheric background

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....8..156g&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 8 p 156-159 (SEE N85-36066 24-93)

Astronomy and Astrophysics

Astrophysics

Astronomy, Cosmic Rays, Neutrinos, Protons, X Ray Irradiation, Astrophysics, Energy Spectra, Flux Density, Muons, Particle Acceleration, Photons

Scientific paper

Some aspects of neutrino astronomy are illustrated by calculating the
neutrino-induced muon flux from Cygnus X-3 binary X-ray source. The
signal depends primarily on the power in cosmic rays at the source and
on the distance to the source, and only relatively little on details of
the matter distribution in the neighborhood of the source.

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