High energy extension of the FLUKA atmospheric neutrino flux

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dc.creatorBattistoni, G.
dc.creatorFerrari, A.
dc.creatorMontaruli, T.
dc.creatorSala, P. R.
dc.date2003-05-19
dc.date.accessioned2026-07-07T03:49:42Z
dc.date.available2026-07-07T03:49:42Z
dc.descriptionThe atmospheric neutrino flux calculated with FLUKA was originally limited to 100-200 GeV for statistical reasons. In order to make it available for the analysis of high energy events, like upward through-going muons detected by neutrino telescopes, we have extended the calculation so to provide a reliable neutrino yield per primary nucleon up to about 10**6 GeV/nucleon, as far as the interaction model is concerned. We point out that the primary flux model above 100 GeV/nucleon still contributes with an important systematic error to the neutrino flux.
dc.descriptionExtended version (10 pages) of the contribution to ICRC 2003, with the addition of flux tables
dc.identifierhttps://arxiv.org/abs/hep-ph/0305208
dc.identifierhttp://arxiv.org/abs/hep-ph/0305208
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/42507
dc.subjectHigh Energy Physics - Phenomenology
dc.titleHigh energy extension of the FLUKA atmospheric neutrino flux
dc.typetext

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