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Sensitivity of KASCADE-Grande data to hadronic interaction models

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arxiv 1009.4902 v1 pith:DIK3C3VI submitted 2010-09-24 astro-ph.HE

Sensitivity of KASCADE-Grande data to hadronic interaction models

D. Kang , W.D. Apel , J.C. Arteaga-Vel\'azquez , K. Bekk , M. Bertaina , J. Bl\"umer , H. Bozdog , I.M. Brancus
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P. Buchholz E. Cantoni A. Chiavassa F. Cossavella K. Daumiller V. de Souza F. di Pierro P. Doll R. Engel J. Engler M. Finger D. Fuhrmann P.L. Ghia H.J. Gils R. Glasstetter C. Grupen A. Haungs D. Heck J.R. H\"orandel T. Huege P.G. Isar K.-H. Kampert D. Kickelbick H.O. Klages K. Link P. Luczak M. Ludwig H.J. Mathes H.J. Mayer M. Melissas J. Milke B. Mitrica C. Morello G. Navarra S. Nehls J. Oehlschl\"ager S. Ostapchenko S. Over N. Palmieria M. Petcu T. Pierog H. Rebel M. Roth H. Schieler F.G. Schr\"oder O. Sima G. Toma G.C. Trinchero H. Ulrich A. Weindl J. Wochele M. Wommer J. Zabierowski
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classification astro-ph.HE
keywords hadronicinteractionmodelsdataenergyeposexperimentalhigh-energy
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KASCADE-Grande is a large detector array dedicated for studies of high-energy cosmic rays in the primary energy range from 100 TeV to 1 EeV. The multi-detector concept of the experimental set-up offers the possibility to measure simultaneously various observables related to the electromagnetic, muonic, and hadronic air shower components. The experimental data are compared to predictions of CORSIKA simulations using high-energy hadronic interaction models (e.g. QGSJET or EPOS), as well as low-energy interaction models (e.g. FLUKA or GHEISHA). This contribution will summarize the results of such investigations. In particular, the validity of the new EPOS version 1.99 for EAS with energy around 100 PeV will be discussed.

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