Atmospheric muons measured with the KM3NeT detectors in comparison with updated numeric predictions ...
The measurement of the flux of muons produced in cosmic ray air showers is essential for the study of primary cosmic rays. Such measurements are important in extensive air shower detectors to assess the energy spectrum and the chemical composition of the cosmic ray flux, complementary to the informa...
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Online Access: | https://dx.doi.org/10.48550/arxiv.2403.11946 https://arxiv.org/abs/2403.11946 |
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ftdatacite:10.48550/arxiv.2403.11946 2024-06-09T07:48:53+00:00 Atmospheric muons measured with the KM3NeT detectors in comparison with updated numeric predictions ... KM3NeT Collaboration 2024 https://dx.doi.org/10.48550/arxiv.2403.11946 https://arxiv.org/abs/2403.11946 unknown arXiv Creative Commons Attribution 4.0 International https://creativecommons.org/licenses/by/4.0/legalcode cc-by-4.0 High Energy Astrophysical Phenomena astro-ph.HE High Energy Physics - Experiment hep-ex FOS Physical sciences CreativeWork article Preprint Article 2024 ftdatacite https://doi.org/10.48550/arxiv.2403.11946 2024-05-13T10:33:59Z The measurement of the flux of muons produced in cosmic ray air showers is essential for the study of primary cosmic rays. Such measurements are important in extensive air shower detectors to assess the energy spectrum and the chemical composition of the cosmic ray flux, complementary to the information provided by fluorescence detectors. Detailed simulations of the cosmic ray air showers are carried out, using codes such as CORSIKA, to estimate the muon flux at sea level. These simulations are based on the choice of hadronic interaction models, for which improvements have been implemented in the post-LHC era. In this work, a deficit in simulations that use state-of-the-art QCD models with respect to the measurement deep underwater with the KM3NeT neutrino detectors is reported. The KM3NeT/ARCA and KM3NeT/ORCA neutrino telescopes are sensitive to TeV muons originating mostly from primary cosmic rays with energies around 10 TeV. The predictions of state-of-the-art QCD models show that the deficit with respect ... : 33 pages, 9 figures, submitted to the European Physical Journal C ... Article in Journal/Newspaper Orca DataCite Metadata Store (German National Library of Science and Technology) |
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DataCite Metadata Store (German National Library of Science and Technology) |
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topic |
High Energy Astrophysical Phenomena astro-ph.HE High Energy Physics - Experiment hep-ex FOS Physical sciences |
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High Energy Astrophysical Phenomena astro-ph.HE High Energy Physics - Experiment hep-ex FOS Physical sciences KM3NeT Collaboration Atmospheric muons measured with the KM3NeT detectors in comparison with updated numeric predictions ... |
topic_facet |
High Energy Astrophysical Phenomena astro-ph.HE High Energy Physics - Experiment hep-ex FOS Physical sciences |
description |
The measurement of the flux of muons produced in cosmic ray air showers is essential for the study of primary cosmic rays. Such measurements are important in extensive air shower detectors to assess the energy spectrum and the chemical composition of the cosmic ray flux, complementary to the information provided by fluorescence detectors. Detailed simulations of the cosmic ray air showers are carried out, using codes such as CORSIKA, to estimate the muon flux at sea level. These simulations are based on the choice of hadronic interaction models, for which improvements have been implemented in the post-LHC era. In this work, a deficit in simulations that use state-of-the-art QCD models with respect to the measurement deep underwater with the KM3NeT neutrino detectors is reported. The KM3NeT/ARCA and KM3NeT/ORCA neutrino telescopes are sensitive to TeV muons originating mostly from primary cosmic rays with energies around 10 TeV. The predictions of state-of-the-art QCD models show that the deficit with respect ... : 33 pages, 9 figures, submitted to the European Physical Journal C ... |
format |
Article in Journal/Newspaper |
author |
KM3NeT Collaboration |
author_facet |
KM3NeT Collaboration |
author_sort |
KM3NeT Collaboration |
title |
Atmospheric muons measured with the KM3NeT detectors in comparison with updated numeric predictions ... |
title_short |
Atmospheric muons measured with the KM3NeT detectors in comparison with updated numeric predictions ... |
title_full |
Atmospheric muons measured with the KM3NeT detectors in comparison with updated numeric predictions ... |
title_fullStr |
Atmospheric muons measured with the KM3NeT detectors in comparison with updated numeric predictions ... |
title_full_unstemmed |
Atmospheric muons measured with the KM3NeT detectors in comparison with updated numeric predictions ... |
title_sort |
atmospheric muons measured with the km3net detectors in comparison with updated numeric predictions ... |
publisher |
arXiv |
publishDate |
2024 |
url |
https://dx.doi.org/10.48550/arxiv.2403.11946 https://arxiv.org/abs/2403.11946 |
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Orca |
genre_facet |
Orca |
op_rights |
Creative Commons Attribution 4.0 International https://creativecommons.org/licenses/by/4.0/legalcode cc-by-4.0 |
op_doi |
https://doi.org/10.48550/arxiv.2403.11946 |
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1801380863801294848 |