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Atmospheric neutrino flux at INO, South Pole and Pyh\"asalmi

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arxiv 1210.5154 v1 pith:O27XLG7P submitted 2012-10-18 hep-ph astro-ph.IM

M. Sajjad Athar , M. Honda , T. Kajita , K. Kasahara , S. Midorikawa This is my paper · ORCID
classification hep-phastro-ph.IM
keywords neutrinofluxesatmosphericasalmidifferentfluxmodelpole
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We present the calculation of the atmospheric neutrino fluxes for the neutrino experiments proposed at INO, South Pole and Pyh\"asalmi. 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.

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