8 research outputs found

    Test of Hadronic Interaction Models in the Forward Region with KASCADE Event Rates

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    An analysis of muon and hadron rates observed in the central detector of the KASCADE experiment has been carried out. The data are compared to CORSIKA simulations employing the high-energy hadronic interaction models QGSJET, DPMJET, HDPM, SIBYLL, and VENUS. In addition, first results with the new hadronic interaction model neXus 2 are discussed. Differences of the model predictions, both among each other and when confronted with measurements, are observed. The hadron rates mainly depend on the inelastic cross-section and on the contribution of diffraction dissociation. The discrepancy between simulations and measurements at low primary energies around 5 TeV can be reduced by increasing the non-diffractive part of the inelastic cross-section of nucleon-air interactions. Examination of hadron multiplicities points towards harder spectra of secondary pions and kaons needed in the calculations.Comment: 14 pages, 7 figures, corresponding author: M. Risse, accepted for publication in J. Phys. G: Nucl. Part. Phy

    Kneelike structure in the spectrum of the heavy component of cosmic rays observed with KASCADE-Grande

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    We report the observation of a steepening in the cosmic ray energy spectrum of heavy primary particles at about 8×10168 \times 10^{16} eV. This structure is also seen in the all-particle energy spectrum, but is less significant. Whereas the `knee' of the cosmic ray spectrum at 3−5×10153-5 \times 10^{15} eV was assigned to light primary masses by the KASCADE experiment, the new structure found by the KASCADE-Grande experiment is caused by heavy primaries. The result is obtained by independent measurements of the charged particle and muon components of the secondary particles of extensive air showers in the primary energy range of 101610^{16} to 101810^{18} eV. The data are analyzed on a single-event basis taking into account also the correlation of the two observables.Comment: 5 pages, 5 figures, accepted by PRL, published October, 7th, 201
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