Processes of the generation of high-energy muons in cosmic rays

Details Processes of the generation of high-energy muons in cosmic rays Processes of the generation of high-energy muons in cosmic rays

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982izssr..46.2410v&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Samarkand, Uzbek SSR, Oct. 27-29, 1981.) Akademiia Nauk SSSR, Izvestiia, Ser

Physics

Cosmic Rays, Energetic Particles, Incident Radiation, Muons, Spectral Energy Distribution, Flux Quantization, Test Chambers, Vertical Motion, X Ray Apparatus

Scientific paper

The energy spectra of cosmic-ray muons in the 3-30 TeV energy region were determined using X-ray emulsion chambers at an underground depth of 1000 g/cu cm. It is shown that the intensity of the vertical flux is higher than expected in the region of gamma-ray energies exceeding 10 TeV, which may be due to the contribution of rapidly generated muons. It may be that the steepening of the spectrum of muons from pi- and K-decay is masked by the fragmentation of rapidly generated muons.

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