Influence of hadronic interaction models on characteristics of the high-energy atmospheric neutrino flux

The high-energy conventional atmospheric neutrino fluxes are calculated with the hadronic interaction models: Kimel & Mokhov, QGSJET II-03(04), SIBYL 2.1(2.3), EPOS LHC. The influence of hadron-nuclear interactions on the neutrino flux ratios, v/v¯,(vμ+v¯μ)/(ve+v¯e) , is studied. A comparison of...

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Veröffentlicht in:	Journal of physics. Conference series 2017-12, Vol.934 (1), p.12008
Hauptverfasser:	Morozova, A D, Kochanov, A A, Sinegovskaya, T S, Sinegovsky, S I
Format:	Artikel
Sprache:	eng
Schlagworte:	Atmospheric correction Atmospheric models Cosmic rays Interaction models Muons Neutrinos Nuclear interactions Parameterization Physics
Online-Zugang:	Volltext
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