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Muons in showers with energy $E_{0} \geq$ 5 EeV and QGSjetII-04 and EPOS LHC models of hadronic interactions. Is there a muon deficit in the models?

by Stanislav Knurenko, Igor Petrov

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Submission summary

Authors (as registered SciPost users): Stanislav Knurenko · Igor Petrov
Submission information
Preprint Link: https://arxiv.org/abs/2208.00606v3  (pdf)
Date accepted: 2023-06-22
Date submitted: 2022-11-29 03:30
Submitted by: Knurenko, Stanislav
Submitted to: SciPost Physics Proceedings
Proceedings issue: 21st International Symposium on Very High Energy Cosmic Ray Interactions (ISVHECRI2022)
Ontological classification
Academic field: Physics
Specialties:
  • Gravitation, Cosmology and Astroparticle Physics
Approaches: Experimental, Observational

Abstract

The paper presents data on the muon component with a threshold \(\varepsilon_{thr} \geq\) 1 GeV. Air showers were registered at the Yakutsk array during almost 50 years of continuous air shower observations. The characteristics of muons are compared with calculations of QGSjetII-04 and EPOS LHC models for a proton and an iron nucleus. There is a muon deficit in the models, at energies greater than 5 EeV. To make an agreement between experimental data and simulations on muons, further tuning of the models is required.

List of changes

p1: There is an ugly line break in "10^16-10^19 eV", i.e. the unit appears in the next line. Maybe this can be fixed.
Fixed line break

p2: "Observation stations on array plane..." I believe this needs some rewording, e.g. "Observation stations within the detector array..." or similar.
Changed the wording

p5: "Such behaviour of z-value..." I believe this sentence needs some re-wording, for example "The origin of such a behaviour of the z-value...".
Changed the wording

p6: "Large statistics of showers with a good "history" made it possible..." I do not understand what "good history" means. Also, it does not sound very scientific. Thus, I recommend a re-wording or clarification here.
Changed to "good precision"

Published as SciPost Phys. Proc. 13, 032 (2023)

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