Constraints of hadronic interaction models from the cosmic muon observations
A simple method of the vertical muon energy spectrum simulations has been suggested. These calculations have been carried out in terms of various models of hadronic interactions. The most energetic π±-mesons and K±-mesons produced in hadron interactions contribute mainly to this energy spectrum of m...
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Online Access: | http://dx.doi.org/10.1051/epjconf/20159910003 |
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doaj-f2fe1691def54eb8bdbc4d40be5dc71b2021-08-02T01:18:12ZengEDP SciencesEPJ Web of Conferences2100-014X2015-01-01991000310.1051/epjconf/20159910003epjconf-isvhecri2014_10003Constraints of hadronic interaction models from the cosmic muon observationsDedenko L.G.Lukyashin A.V.0Fedorova G.F.1Roganova T.M.2Faculty of Physics M.V. Lomonosov Moscow State University, Leninskie GorySkobeltsin Institute of Nuclear Physics, Lomonosov Moscow State UniversitySkobeltsin Institute of Nuclear Physics, Lomonosov Moscow State UniversityA simple method of the vertical muon energy spectrum simulations has been suggested. These calculations have been carried out in terms of various models of hadronic interactions. The most energetic π±-mesons and K±-mesons produced in hadron interactions contribute mainly to this energy spectrum of muons due to the very steep energy spectrum of the primary particles. So, some constraints on the hadronic interaction models may be set from a comparison of calculated results with cosmic data on the vertical muon energy spectrum. This comparison showed that the most energetic secondary particles production is too high in the case of the QGSJET II-04 model and rather low in the case of the QGSJET II-03 model. These conclusion have been supported by the LHC data.http://dx.doi.org/10.1051/epjconf/20159910003 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Dedenko L.G. Lukyashin A.V. Fedorova G.F. Roganova T.M. |
spellingShingle |
Dedenko L.G. Lukyashin A.V. Fedorova G.F. Roganova T.M. Constraints of hadronic interaction models from the cosmic muon observations EPJ Web of Conferences |
author_facet |
Dedenko L.G. Lukyashin A.V. Fedorova G.F. Roganova T.M. |
author_sort |
Dedenko L.G. |
title |
Constraints of hadronic interaction models from the cosmic muon observations |
title_short |
Constraints of hadronic interaction models from the cosmic muon observations |
title_full |
Constraints of hadronic interaction models from the cosmic muon observations |
title_fullStr |
Constraints of hadronic interaction models from the cosmic muon observations |
title_full_unstemmed |
Constraints of hadronic interaction models from the cosmic muon observations |
title_sort |
constraints of hadronic interaction models from the cosmic muon observations |
publisher |
EDP Sciences |
series |
EPJ Web of Conferences |
issn |
2100-014X |
publishDate |
2015-01-01 |
description |
A simple method of the vertical muon energy spectrum simulations has been suggested. These calculations have been carried out in terms of various models of hadronic interactions. The most energetic π±-mesons and K±-mesons produced in hadron interactions contribute mainly to this energy spectrum of muons due to the very steep energy spectrum of the primary particles. So, some constraints on the hadronic interaction models may be set from a comparison of calculated results with cosmic data on the vertical muon energy spectrum. This comparison showed that the most energetic secondary particles production is too high in the case of the QGSJET II-04 model and rather low in the case of the QGSJET II-03 model. These conclusion have been supported by the LHC data. |
url |
http://dx.doi.org/10.1051/epjconf/20159910003 |
work_keys_str_mv |
AT dedenkolg constraintsofhadronicinteractionmodelsfromthecosmicmuonobservations AT lukyashinav constraintsofhadronicinteractionmodelsfromthecosmicmuonobservations AT fedorovagf constraintsofhadronicinteractionmodelsfromthecosmicmuonobservations AT roganovatm constraintsofhadronicinteractionmodelsfromthecosmicmuonobservations |
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1721244987390164992 |