arXiv · hep-ph/0305208
High energy extension of the FLUKA atmospheric neutrino flux
Abstract
The 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.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
G. Battistoni, A. Ferrari, T. Montaruli, P. R. Sala. 2003-05-19. High energy extension of the FLUKA atmospheric neutrino flux. https://arxiv.org/abs/hep-ph/0305208
Cite the original work for its findings. Save a collection to share your selection of sources.