Atmospheric neutrino flux at INO, South Pole and Pyhäsalmi

Abstract

We present the calculation of the atmospheric neutrino fluxes for the neutrino experiments proposed at INO, South Pole and Pyhäsalmi. Neutrino fluxes have been obtained using ATMNC, a simulation code for cosmic ray in the atmosphere. Even using the same primary flux model and the interaction model, the calculated atmospheric neutrino fluxes are different for the different sites due to the geomagnetic field. The prediction of these fluxes in the present paper would be quite useful in the experimental analysis.

12Pages,9Figs

References in corpus (2)

• Calculation of atmospheric neutrino flux using the interaction model calibrated with atmospheric muon data
• Improvement of low energy atmospheric neutrino flux calculation using the JAM nuclear interaction model

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