Energy spectra and intensities of cosmic-ray muons at large depths

Details Energy spectra and intensities of cosmic-ray muons at large depths Energy spectra and intensities of cosmic-ray muons at large depths

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985izyak..49.1389b&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Yakutsk, USSR, July 1984) Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheskai

Physics

Angular Distribution, Cosmic Rays, Energy Spectra, Muons, Charm (Particle Physics), Kinetic Equations, Nuclear Interactions, Soils, Water

Scientific paper

A kinetic-equation method is used to calculate the spectra and angular distributions of muons at large depths in water and soil. Various questions pertaining to the investigation of cosmic-ray muons are examined: (1) spectral slope at sea level at an energy of approximately 10 to the 13th eV; (2) the possibility of studying photonuclear interaction at large depths; and (3) the fraction of direct muons generated from the decay of short-lived D and Lambda-c particles.

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