https://doi.org/10.1051/epjconf/201817207003
Tests of the SIBYLL 2.3 high-energy hadronic interaction model using the KASCADE-Grande muon data
1
Institute of Physics and Mathematics, Universidad Michoacana de San Nicolás de Hidalgo, Morelia, Mexico
2
Institut für Kernphysik, KIT - Karlsruher Institut für Technologie, Germany
3
Departimento di Fisica, Università degli Studi di Torino, Italy
4
Institut für Experimentelle Teilchenphysik, KIT - Karlsruher Institut für Technologie, Germany
5
Horia Hulubei National Institute of Physics and Nuclear Engineering, Bucharest, Romania
6
Osservatorio Astrofisico di Torino, INAF Torino, Italy
7
Universidade de São Paulo, Instituto de Física de São Carlos, Brasil
8
Fachbereich Physik, Universität Wuppertal, Germany
9
Department of Physics, Siegen University, Germany
10
Department of Astrophysics, Radboud University Nijmegen, The Netherlands
11
National Centre for Nuclear Research, Department of Astrophysics, Lodz, Poland
12
Frankfurt Institute for Advanced Studies (FIAS), Frankfurt am Main, Germany
13
Department of Physics, University of Bucharest, Bucharest, Romania
14
Now: Head of Division V at KIT - Karlsruher Institut für Technologie, Germany
15
Now at: Istituto Nazionale di Ricerca Metrologica, INRIM, Torino, Italy
16
Now at: DLR Oberpfaffenhofen, Germany
17
Now at: University of Duisburg-Essen, Duisburg, Germany
18
Spokesperson KASCADE-Grande
* e-mail: arteaga@ifm.umich.mx
** e-mail: drivera@ifm.umich.mx
*** e-mail: andreas.haungs@kit.edu
Published online: 26 January 2018
The KASCADE-Grande observatory was a ground-based air shower array dedicated to study the energy and composition of cosmic rays in the energy interval E = 1 PeV –1 EeV. The experiment consisted of different detector systems which allowed the simultaneous measurement of distinct components of air showers (EAS), such as the muon content. In this contribution, we study the total muon number and the lateral density distribution of muons in EAS detected by KASCADE-Grande as a function of the zenith angle and the total number of charged particles. The attenuation length of the muon content of EAS is also measured. The results are compared with the predictions of the SIBYLL 2.3 high-energy hadronic interaction model.
© The Authors, published by EDP Sciences, 2018
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. (http://creativecommons.org/licenses/by/4.0/).
