Primary cosmic rays studied on the basis of spectrum analysis of muons at sea level

Details Primary cosmic rays studied on the basis of spectrum analysis of muons at sea level Primary cosmic rays studied on the basis of spectrum analysis of muons at sea level

May 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976izssr..40.1054t&link_type=abstract

(Vsesoiuznaia Konferentsiia po Fizike Kosmicheskikh Luchei, Samarkand, Uzbek SSR, Oct. 29-31, 1975.) Akademiia Nauk SSSR, Izvest

Computer Science

Cosmic Ray Showers, Muons, Nuclear Radiation Spectroscopy, Nucleon-Nucleon Interactions, Primary Cosmic Rays, Chemical Composition, Energy Spectra, High Energy Interactions, Particle Flux Density, Spectrum Analysis

Scientific paper

A nucleon-nucleon interaction model is used to calculate fluxes of muons produced from various groups of nuclei. It is assumed that the primary nucleus at the first collision breaks up into nucleons and that in this case for equal energies A times more mesons are released per nucleon than for the case of proton-nucleus interactions. Differential muon fluxes and the charge relations of muon fluxes at sea level are calculated, as are the differential spectra of primary cosmic ray nuclei.

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