Using a superposition model in the analysis of muon groups generated by high-energy nuclei of primary cosmic rays

Details Using a superposition model in the analysis of muon groups generated by high-energy nuclei of primary cosmic rays Using a superposition model in the analysis of muon groups generated by high-energy nuclei of primary cosmic rays

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pzetf..50....6b&link_type=abstract

Pis'ma v Zhurnal Eksperimental'noi i Teoreticheskoi Fiziki (ISSN 0370-274X), vol. 50, July 10, 1989, p. 6-9. In Russian.

Physics

Nuclear Physics

1

High Energy Interactions, Muons, Nuclei (Nuclear Physics), Primary Cosmic Rays, Superposition (Mathematics), Cosmic Ray Showers, Energy Distribution, Monte Carlo Method, Protons, Scintillation Counters

Scientific paper

Muon groups generated by the nuclei of primary cosmic rays are analyzed using the Monte Carlo method. By comparing the characteristics of the extensive atmospheric showers generated by nuclei and protons, the validity of the superposition model is demonstrated. Calculations are carried out for a muon energy of 0.2 TeV, which corresponds to the minimum threshold energy of muon registration by the Baksanskii underground scintillation telescope.

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