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:
- 1609.05764 [astro-ph.HE]
Report number:
- INR-TH-2016-035
View in:
Citations per year
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
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Figures(6)
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