Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
5486698 | Astroparticle Physics | 2017 | 6 Pages |
Abstract
Some discrepancies have been reported between observed and simulated muon content of extensive air showers: the number of observed muons exceeded the expectations in HiRes-MIA, Yakutsk and Pierre Auger Observatory data. Here, we analyze the data of the Moscow State University Extensive Air Shower (EAS-MSU) array on Eμ â³ 10 GeV muons in showers caused by â¼(1017â1018) eV primary particles and demonstrate that they agree with simulations (QGSJET-II-04 hadronic interaction model) once the primary composition inferred from the surface-detector data is assumed.
Related Topics
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Physics and Astronomy
Astronomy and Astrophysics
Authors
Yu.A. Fomin, N.N. Kalmykov, I.S. Karpikov, G.V. Kulikov, M.Yu. Kuznetsov, G.I. Rubtsov, V.P. Sulakov, S.V. Troitsky,