The cosmic-ray muon background in a chlorine detector of solar neutrinos

Details The cosmic-ray muon background in a chlorine detector of solar neutrinos The cosmic-ray muon background in a chlorine detector of solar neutrinos

Mar 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980izyer..44..622z&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Yerevan, Armenian SSR, June 5-7, 1979.) Akademiia Nauk SSSR, Izvestiia, Seri

Physics

Background Radiation, Cosmic Rays, High Energy Interactions, Muons, Nuclear Interactions, Solar Neutrinos, Chlorine, Energy Spectra, Particle Energy, Radiation Counters

Scientific paper

It has been shown that at large depths, where the mean energy of muons
amounts to a few GeV, the basic yield to muon background is due to the
development of nuclear cascades generated by muon-nucleus interaction.
In the present paper, a scheme for calculating nuclear cascades
generated by high-energy muons is outlined.

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