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Investigation of hadronic interaction models with the KASCADE experiment

✍ Scribed by J. Milke; T. Antoni; W.D. Apel; F. Badea; K. Bekk; A. Bercuci; H. Blümer; H. Bozdog; I.M. Brancus; C. Büttner; A. Chilingarian; K. Daumiller; P. Doll; R. Engel; J. Engler; F. Feßler; H.J. Gils; R. Glasstetter; A. Haungs; D. Heck; J.R. Hörandel; K.-H. Kampert; H.O. Klages; G. Maier; H.J. Mathes; H.J. Mayer; M. Müller; R. Obenland; J. Oehlschläger; S. Ostapchenko; M. Petcu; H. Rebel; A. Risse; M. Risse; M. Roth; G. Schatz; H. Schieler; J. Scholz; T. Thouw; H. Ulrich; J. van Buren; A. Vardanyan; A. Weindl; J. Wochele; J. Zabierowski


Publisher
Elsevier Science
Year
2006
Tongue
English
Weight
221 KB
Volume
151
Category
Article
ISSN
0920-5632

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✦ Synopsis


Using the correlations of the hadronic, electromagnetic, and muonic components of extensive air showers measured with the experiment KASCADE the influence of hadronic interaction models on the simulation of air showers is investigated. For the simulations CORSIKA with GHEISHA and FLUKA as low-energy models and DPMJET, SIBYLL, and QGSJET as high-energy models have been used.


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Various hadronic interaction models were used in extensive air showers simulations. This resulted in ambiguous estimation of primary energy, cosmic ray flux intensity, mass composition, etc. Several revisions of models have been made recently; for example, third major version of QGSjet II (QGSjet II