Physics
Scientific paper
Feb 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989izssr..53..332a&link_type=abstract
(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Alma-Ata, Kazakh SSR, Sept. 13-15, 1988) Akademiia Nauk SSSR, Izvestiia, Ser
Physics
Angular Distribution, Cosmic Rays, Muons, Particle Telescopes, Scintillation Counters, Charm (Particle Physics), Energy Dissipation, Energy Spectra
Scientific paper
The contribution of charmed particles to the energy spectrum of muons observed with the Baksan scintillation telescope is evaluated; the absorption curve measured in directions close to horizon is presented, and the relationship between the absorption curve and the muon energy spectrum is discussed. It is shown that the present measurements are described well by the Volkova spectrum with R = 1.5 x 10 to the -3rd and a spectrum exponent gammamu = 2.70, but diverge somewhat from the results of Bugaev et al. (1987), where the contribution of charmed particles is derived from the recombinational quark-gluon model.
Andreev Iu. M.
Chudakov A. E.
Gurentsov V. I.
Kogai I. M.
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