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We study the influence of hadron interaction features on the high-energyatmospheric neutrino spectrum. The 1D calculation is performed with use of theknown high-energy hadronic models, SIBYLL 2.1, QGSJET-II, Kimel and Mokhov, forthe parameterizations of primary cosmic ray spectra issued from the measurementdata. The results are compared with the Frejus data and AMANDA-II measurementsas well as with other calculations. Sizable difference of the neutrino fluxes(up to the factor of 1.8 at 1 TeV) that are obtained with the SIBYLL andQGSJET-II appears to be rather unexpected keeping in mind the hadron and muonflux calculations in the same energy region.

Impact of high-energy hadron interactions on the atmospheric neutrino flux predictions