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Cosmic ray energy spectra derived from KASCADE-Grande data using post-LHC hadronic interaction models

Kang, Donghwa ORCID iD icon 1; Arteaga-Velázquez", "J. C.; Bertaina, Mario E.; Chiavassa, A.; Colmenero-Cesar", "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.; ... mehr

Abstract:

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.


Verlagsausgabe §
DOI: 10.5445/IR/1000190569
Veröffentlicht am 12.02.2026
Cover der Publikation
Zugehörige Institution(en) am KIT Institut für Astroteilchenphysik (IAP)
Publikationstyp Proceedingsbeitrag
Publikationsdatum 23.09.2025
Sprache Englisch
Identifikator ISSN: 1824-8039
KITopen-ID: 1000190569
Erschienen in Proceedings of 39th International Cosmic Ray Conference — PoS(ICRC2025); Genf, Schweiz, 15.-24.07.2025
Veranstaltung 39th International Cosmic Ray Conference (ICRC 2025), Genf, Schweiz, 15.07.2025 – 24.07.2025
Verlag Scuola Internazionale Superiore di Studi Avanzati (SISSA)
Seiten Art.Nr: 297
Serie Proceedings of Science (PoC) ; 501
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