No muon excess in extensive air showers at 100–500 PeV primary energy: EAS–MSU results

Sep 19, 2016
6 pages
Published in:
  • Astropart.Phys. 92 (2017) 1-6
  • Published: Jun, 2017
e-Print:
Report number:
  • INR-TH-2016-035

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Abstract: (Elsevier)
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 E μ ≳ 10 GeV muons in showers caused by ∼(1017−1018)  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.
Note:
  • 10 pages, 6 figures, elsart.sty. V2: extended discussion of systematic errors, numerous clarifications (results unchanged). V3: minor changes, version accepted by Astroparticle Physics
  • Extensive air showers
  • Muon data
  • Hadronic interaction models
  • showers: atmosphere
  • interaction: model
  • detector: surface
  • muon
  • air
  • Monte Carlo
  • numerical calculations