Atmospheric neutrino flux at INO, South Pole and Pyhäsalmi

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,...

Full description

Bibliographic Details
Main Authors: Athar, M. Sajjad, Honda, M., Kajita, T., Kasahara, K., Midorikawa, S.
Format: Text
Language:unknown
Published: arXiv 2012
Subjects:
High Energy Physics - Phenomenology hep-ph
Instrumentation and Methods for Astrophysics astro-ph.IM
FOS Physical sciences
South Pole
South pole
Online Access:https://dx.doi.org/10.48550/arxiv.1210.5154
https://arxiv.org/abs/1210.5154
Description
Summary: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

Similar Items