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Abstract: We present results of simulations of a muon content in the air showersinduced by very high energy cosmic rays. Muon energy distributions and muondensities at ground level are given. We discuss a prompt muon componentgenerated by decays of charm mesons. The method combines standard Monte Carlogenerators incorporated in the CORSIKA code and phenomenological estimates ofthe charm hadroproduction.



Author: J.Ridky, D.Nosek, P.Travnicek, P.Necesal

Source: https://arxiv.org/







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