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AbstractAbstract
[en] We have deduced the muon energy spectrum from primary cosmic ray nucleon spectrum in the energy range 4 to 105 GeV using latest PAMELLA, CREAM AND ATIC-2 BALLOON-BORNE experimental data. The derived muon spectra have been compared with experimental data of CosmoAleph and as well as theoretical calculation of Bugaev and Hebbeker and Timmermans considering the validity if hypothesis of Feynman regarding scale invariance in particle production. (author)
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Department of Physics, University of Kalyani, Kalyani (India); 61 p; 2014; p. 58; CTPPR-2014: national conference on current trends in particle physics research; Kalyani (India); 13-15 Mar 2014
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Conference
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