| Issue |
EPJ Web Conf.
Volume 208, 2019
ISVHECRI 2018 - XX International Symposium on Very High Energy Cosmic Ray Interactions
|
|
|---|---|---|
| Article Number | 11005 | |
| Number of page(s) | 6 | |
| Section | Hadronic Interaction Models | |
| DOI | https://doi.org/10.1051/epjconf/201920811005 | |
| Published online | 10 May 2019 | |
https://doi.org/10.1051/epjconf/201920811005
EPOS
1
SUBATECH, University of Nantes – IN2P3/CNRS – IMT Atlantique, Nantes, France
2
Universidad Tecnica Federico Santa Maria y Centro Cientifico- Tecnologico de Valparaiso, Valparaiso, Chile
3
Karlsruhe Inst. of Technology, KIT, Campus North, Inst. f. Kernphysik, Germany
4
Warsaw University of Technology, Warsaw, Poland
Published online: 10 May 2019
We summarize the main features of the hadronic interaction model EPOS, which is used for cosmic ray air shower simulations but also for p-p, p-A, and A-A collisions to be compared with experimental data from LHC and RHIC.
© The Authors, published by EDP Sciences, 2019
This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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