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| Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , |
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| Format: | Preprint |
| Published: |
2025
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| Subjects: | |
| Online Access: | https://arxiv.org/abs/2508.21646 |
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| _version_ | 1866916925328588800 |
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| author | Kang, D. Arteaga-Velázquez, J. C. Bertaina, M. Chiavassa, A. Colmenero-César, A. L. Daumiller, K. de Souza, V. Engel, R. Gherghel-Lascu, A. Grupen, C. Haungs, A. Hörandel, J. R. Huege, T. Kampert, K. -H. Link, K. Mathes, H. J. Ostapchenko, S. Pierog, T. Rivera-Rangel, D. Roth, M. Schieler, H. Schröder, F. G. Sima, O. Weindl, A. Wochele, J. Zabierowski, J. |
| author_facet | Kang, D. Arteaga-Velázquez, J. C. Bertaina, M. Chiavassa, A. Colmenero-César, A. L. Daumiller, K. de Souza, V. Engel, R. Gherghel-Lascu, A. Grupen, C. Haungs, A. Hörandel, J. R. Huege, T. Kampert, K. -H. Link, K. Mathes, H. J. Ostapchenko, S. Pierog, T. Rivera-Rangel, D. Roth, M. Schieler, H. Schröder, F. G. Sima, O. Weindl, A. Wochele, J. Zabierowski, J. |
| contents | KASCADE-Grande was dedicated to measuring the energy spectrum and mass composition of cosmic rays in the energy range of 10 PeV to 1 EeV. We observed a knee-like structure in the heavy mass component at around 100 PeV and an ankle-like structure in the light component. In this contribution, we present updated energy spectra based on shower size measurements, using the post-LHC hadronic models QGSJet-II-04, EPOS-LHC, and SIBYLL 2.3d, including accounting for shower-to-shower fluctuations. In addition, the newly released EPOS-LHC-R model is tested for the first time with KASCADE-Grande. We will compare and discuss the results obtained using the different hadronic interaction models. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2508_21646 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Cosmic ray energy spectra derived from KASCADE-Grande data using post-LHC hadronic interaction models Kang, D. Arteaga-Velázquez, J. C. Bertaina, M. Chiavassa, A. Colmenero-César, A. L. Daumiller, K. de Souza, V. Engel, R. Gherghel-Lascu, A. Grupen, C. Haungs, A. Hörandel, J. R. Huege, T. Kampert, K. -H. Link, K. Mathes, H. J. Ostapchenko, S. Pierog, T. Rivera-Rangel, D. Roth, M. Schieler, H. Schröder, F. G. Sima, O. Weindl, A. Wochele, J. Zabierowski, J. High Energy Astrophysical Phenomena KASCADE-Grande was dedicated to measuring the energy spectrum and mass composition of cosmic rays in the energy range of 10 PeV to 1 EeV. We observed a knee-like structure in the heavy mass component at around 100 PeV and an ankle-like structure in the light component. In this contribution, we present updated energy spectra based on shower size measurements, using the post-LHC hadronic models QGSJet-II-04, EPOS-LHC, and SIBYLL 2.3d, including accounting for shower-to-shower fluctuations. In addition, the newly released EPOS-LHC-R model is tested for the first time with KASCADE-Grande. We will compare and discuss the results obtained using the different hadronic interaction models. |
| title | Cosmic ray energy spectra derived from KASCADE-Grande data using post-LHC hadronic interaction models |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2508.21646 |