Proceedings of the 34th International Cosmic Ray Conference — PoS(ICRC2015) 2016
DOI: 10.22323/1.236.0359
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KASCADE-Grande energy spectrum of cosmic rays interpreted with post-LHC hadronic interaction models

Abstract: Previous results obtained by KASCADE-Grande using QGSjetII-02, EPOS1.99 and SIBYLL hadronic interaction models have shown that the energy spectrum of cosmic rays between 10 16 eV and 10 18 eV exhibits a significant hardening at approximately 2×10 16 eV, a slight but statistically significant steepening close to 10 17 eV, i.e. the 'knee' caused by the heavy component of primary cosmic rays, and an 'ankle' like feature of the light component just above 10 17 eV. In this paper, we report on results of similar ana… Show more

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Cited by 15 publications
(18 citation statements)
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“…The selection of heavy primaries enhances the knee-like feature that is already present in the all-particle spectrum. The analysis was repeated on the basis of different hadronic interaction models [18,19]. Despite the fact that the relative abundance of the heavy particles varies significantly dependent on the model in use, the spectral feature of this 'heavy' knee is visible in all the spectra.…”
Section: Elemental Composition Of Cosmic Raysmentioning
confidence: 99%
See 1 more Smart Citation
“…The selection of heavy primaries enhances the knee-like feature that is already present in the all-particle spectrum. The analysis was repeated on the basis of different hadronic interaction models [18,19]. Despite the fact that the relative abundance of the heavy particles varies significantly dependent on the model in use, the spectral feature of this 'heavy' knee is visible in all the spectra.…”
Section: Elemental Composition Of Cosmic Raysmentioning
confidence: 99%
“…The error bars show the statistical uncertainties and the bands the systematic uncertainties; fits on the spectra and resulting slopes before and after the heavy knee are also indicated [19]. experiments worldwide.…”
Section: Hadronic Interaction Modelsmentioning
confidence: 99%
“…The selection of heavy primaries enhances the knee-like feature that is already present in the all-particle spectrum. The analysis was repeated on the basis of different hadronic interaction models [18,19]. Despite the fact that the relative abundance of the heavy particles varies significantly dependent on the model in use, the spectral feature of this 'heavy' knee is visible in all the spectra.…”
Section: Elemental Composition Of Cosmic Raysmentioning
confidence: 99%
“…Right: Reconstructed energy spectra of the heavy primary component for five hadronic interaction models. The error bars show the statistical uncertainties and the bands the systematic uncertainties; fits on the spectra and resulting slopes before and after the heavy knee are also indicated [12].…”
Section: Kascade-grandementioning
confidence: 99%
“…The analysis was repeated on basis of different hadronic interaction models [11,12]. Despite the fact, that the relative abundance of the heavy particles varies significantly dependent on the model in use, the spectral feature of this 'heavy' knee is visible in all the spectra (Fig.…”
Section: Kascade-grandementioning
confidence: 99%