High energy neutrinos in the atmosphere

Details High energy neutrinos in the atmosphere High energy neutrinos in the atmosphere

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990nuphs..13..398k&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 13, p. 398-400.

Physics

Nuclear Physics

Scientific paper

The fluxes of neutrinos from the γ-ray point sources are predicted assuming the widely accepted picture that those sources are binary systems where one of the companions is a compact object producing cosmic rays. Interactions of the cosmic rays with atmosphere of the other companion is a source of γ rays (via production of π°) and also of neutrinos. It is shown that the ratio of electron to muon neutrino for the neutrinos produced in the sources is, at energies around 1 TeV, much higher than the same ratio for the atmospheric neutrinos.

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