Analysis of cosmic ray multi-muon phenomena in the energy region 10 to the 14th - 10 to the 16th eV

Physics

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Elementary Particle Interactions, Extraterrestrial Radiation, Muons, Primary Cosmic Rays, Energy Spectra, Heavy Nuclei, Helium, Iron

Scientific paper

Under the condition of primary cosmic rays incident with different composition, the multi-muon phenomena are simulated by the scaling model of the hadronic interactions included in the mechanism of jet production with large transverse momentum. The results show that the primary heavy nuclei contribute significantly to the large muon-multiplicity events observed deep underground. Even when the primary model with heavy-nucleus dominance is used, the simulated multi-muon even rate is still lower than the experimental data, and suggests the existence of other multi-muon sources. The lateral distribution of multi-muon events is in accordance with experiments.

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