2018
DOI: 10.1051/epjconf/201817207003
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Tests of the SIBYLL 2.3 high-energy hadronic interaction model using the KASCADE-Grande muon data

Abstract: Abstract. The KASCADE-Grande observatory was a ground-based air shower array dedicated to study the energy and composition of cosmic rays in the energy interval E = 1 PeV −1 EeV. The experiment consisted of different detector systems which allowed the simultaneous measurement of distinct components of air showers (EAS), such as the muon content. In this contribution, we study the total muon number and the lateral density distribution of muons in EAS detected by KASCADE-Grande as a function of the zenith angle … Show more

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Cited by 2 publications
(1 citation statement)
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“…Muon studies with KASCADE-Grande J.C. Arteaga-Velazquez a ratio of 2.9 and another one with 0.99 at 100 PeV. These values are close to other ones observed from previous analyses of composition in KASCADE-Grande using different post-LHC hadronic interaction models (QGSJET-II-04, EPOS-LHC and SIBYLL 2.3) [18]. The maximum/minimum variations in the results with respect to the reference value were computed as the systematic uncertainties due to composition.…”
Section: Pos(icrc2021)376supporting
confidence: 85%
“…Muon studies with KASCADE-Grande J.C. Arteaga-Velazquez a ratio of 2.9 and another one with 0.99 at 100 PeV. These values are close to other ones observed from previous analyses of composition in KASCADE-Grande using different post-LHC hadronic interaction models (QGSJET-II-04, EPOS-LHC and SIBYLL 2.3) [18]. The maximum/minimum variations in the results with respect to the reference value were computed as the systematic uncertainties due to composition.…”
Section: Pos(icrc2021)376supporting
confidence: 85%