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Constraints of hadronic interaction models from the cosmic muon observations
2015
EPJ Web of Conferences
Preserved Fulltext
A simple method of the vertical muon energy spectrum simulations has been suggested. These calculations have been carried out in terms of various models of hadronic interactions. The most energetic π ± -mesons and K ± -mesons produced in hadron interactions contribute mainly to this energy spectrum of muons due to the very steep energy spectrum of the primary particles. So, some constraints on the hadronic interaction models may be set from a comparison of calculated results with cosmic data on
doi:10.1051/epjconf/20159910003
fatcat:svhecdjgrbgu7h7ej4t2avbhja