High energy neutrinos from galactic sources

Details High energy neutrinos from galactic sources High energy neutrinos from galactic sources

Sep 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992zphyc..54..469t&link_type=abstract

Zeitschrift für Physik C Particles and Fields, Volume 54, Issue 3, pp.469-481

Physics

6

Scientific paper

Analytical expressions are derived which allow to calculate flux densities of energetic neutrinos from hypothetical galactic sources, consisting of a proton accelerator and a dilute gas beam dump. The same formalism is used to calculate atmospheric muon and μ-neutrino fluxes. From the results, rates of upward going muons, both from the atmosphere and galactic sources, are computed and detection limits for neutrino emitters in the sky are established. Finally, the background in a surface detector, caused by scattered muons and charm decays in the rock, is estimated for the case of a flat surrounding.

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