A Three-Dimensional Calculation of Atmospheric Neutrino Fluxes

Physics – High Energy Physics – High Energy Physics - Phenomenology

Scientific paper

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30 pages, 14 figures, major revision for submission to Astroparticle Physics. Accepted 2002/04

Scientific paper

10.1016/S0927-6505(02)00159-7

We present a three-dimensional calculation of atmospheric neutrino fluxes using accurate models of the geomagnetic field, hadronic interactions, tracking and decays. Results are presented for the Super-Kamiokande (SK) and Sudbury Neutrino Observatory (SNO) sites using the GEANT-FLUKA hadronic code. We make a comparison with previous one-dimensional calculations and other three-dimensional results. The recently reported geometrical enhancement of low energy, horizontal neutrinos is confirmed. The effect on observed leptons is however, restricted to a small overall increase in flux. We report east-west asymmetries for each of the neutrino species.

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