Uncertainty of the atmospheric neutrino fluxes

Details Uncertainty of the atmospheric neutrino fluxes Uncertainty of the atmospheric neutrino fluxes

1998-11-30

arxiv.org/abs/hep-ph/9811504v2

Nucl.Phys.Proc.Suppl. 77 (1999) 140-145

Physics

High Energy Physics

High Energy Physics - Phenomenology

7 pages, LaTeX, 9 figures, talk given at Neutrino98, Takayama, Japan, 4-9 June, 1998

Scientific paper

10.1016/S0920-5632(99)00409-0

The uncertainty in the calculation of atmospheric neutrino fluxes is studied. The absolute value of atmospheric neutrino fluxes is sensitive to variation of the primary cosmic ray flux model and/or the interaction model. However, the ratios between different kind of neutrinos stay almost unchanged with these variations. It is unlikely that the anomalous ratio $(\nu_{\mu}/\nu_e)_{obs}/(\nu_{\mu}/\nu_e)_{MC}$ reported by Kamiokande and Super Kamiokande is caused by the uncertainty of predicted atmospheric neutrino fluxes.

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