A new calculation of atmospheric neutrino flux: the FLUKA approach.

Physics – Nuclear Physics

Scientific paper

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Neutrinos: Earth Atmosphere, Neutrinos: Cosmic Rays

Scientific paper

Preliminary results from a full 3-D calculation of atmospheric neutrino fluxes using the FLUKA interaction model are presented and compared to previous existing calculations. This effort is motivated mainly by the 3-D capability and the satisfactory degree of accuracy of the hadron-nucleus models embedded in the FLUKA code. The authors show examples of benchmarking tests of the model with cosmic ray experiment results. A comparison of this calculation of the atmospheric neutrino flux with that of the Bartol group, for Eν > 1 GeV, is presented.

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