High energy cosmic ray interactions and UHECR composition problem
- The differences between contemporary Monte Carlo generators of high energy hadronic interactions are discussed and their impact on the interpretation of experimental data on ultra-high energy cosmic rays (UHECRs) is studied. Key directions for further model improvements are outlined. The prospect for a coherent interpretation of the data in terms of the UHECR composition is investigated.
Author: | Sergey Ostapchenko |
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URN: | urn:nbn:de:hebis:30:3-500961 |
DOI: | https://doi.org/10.1051/epjconf/201921002001 |
ISSN: | 2100-014X |
Parent Title (English): | EPJ Web of Conferences |
Document Type: | Conference Proceeding |
Language: | English |
Year of Completion: | 2019 |
Date of first Publication: | 2019/05/17 |
Publishing Institution: | Universitätsbibliothek Johann Christian Senckenberg |
Contributing Corporation: | Ultra High Energy Cosmic Rays 2018 (UHECR 2018) |
Release Date: | 2019/06/05 |
Volume: | 210 |
Issue: | Article Number: 02001 |
Page Number: | 10 |
First Page: | 1 |
Last Page: | 10 |
HeBIS-PPN: | 450418979 |
Institutes: | Physik / Physik |
Wissenschaftliche Zentren und koordinierte Programme / Frankfurt Institute for Advanced Studies (FIAS) | |
Dewey Decimal Classification: | 5 Naturwissenschaften und Mathematik / 53 Physik / 530 Physik |
Sammlungen: | Universitätspublikationen |
Licence (German): | Creative Commons - Namensnennung 4.0 |