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,...

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Main Authors: Athar, M. Sajjad, Honda, M., Kajita, T., Kasahara, K., Midorikawa, S.
Format: Text
Language:unknown
Published: arXiv 2012
Subjects:
Online Access:https://dx.doi.org/10.48550/arxiv.1210.5154
https://arxiv.org/abs/1210.5154
id ftdatacite:10.48550/arxiv.1210.5154
record_format openpolar
spelling ftdatacite:10.48550/arxiv.1210.5154 2023-05-15T18:21:51+02:00 Atmospheric neutrino flux at INO, South Pole and Pyhäsalmi Athar, M. Sajjad Honda, M. Kajita, T. Kasahara, K. Midorikawa, S. 2012 https://dx.doi.org/10.48550/arxiv.1210.5154 https://arxiv.org/abs/1210.5154 unknown arXiv https://dx.doi.org/10.1016/j.physletb.2012.12.016 arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ High Energy Physics - Phenomenology hep-ph Instrumentation and Methods for Astrophysics astro-ph.IM FOS Physical sciences article-journal Article ScholarlyArticle Text 2012 ftdatacite https://doi.org/10.48550/arxiv.1210.5154 https://doi.org/10.1016/j.physletb.2012.12.016 2022-04-01T13:36:44Z 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 Text South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language unknown
topic High Energy Physics - Phenomenology hep-ph
Instrumentation and Methods for Astrophysics astro-ph.IM
FOS Physical sciences
spellingShingle High Energy Physics - Phenomenology hep-ph
Instrumentation and Methods for Astrophysics astro-ph.IM
FOS Physical sciences
Athar, M. Sajjad
Honda, M.
Kajita, T.
Kasahara, K.
Midorikawa, S.
Atmospheric neutrino flux at INO, South Pole and Pyhäsalmi
topic_facet High Energy Physics - Phenomenology hep-ph
Instrumentation and Methods for Astrophysics astro-ph.IM
FOS Physical sciences
description 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
format Text
author Athar, M. Sajjad
Honda, M.
Kajita, T.
Kasahara, K.
Midorikawa, S.
author_facet Athar, M. Sajjad
Honda, M.
Kajita, T.
Kasahara, K.
Midorikawa, S.
author_sort Athar, M. Sajjad
title Atmospheric neutrino flux at INO, South Pole and Pyhäsalmi
title_short Atmospheric neutrino flux at INO, South Pole and Pyhäsalmi
title_full Atmospheric neutrino flux at INO, South Pole and Pyhäsalmi
title_fullStr Atmospheric neutrino flux at INO, South Pole and Pyhäsalmi
title_full_unstemmed Atmospheric neutrino flux at INO, South Pole and Pyhäsalmi
title_sort atmospheric neutrino flux at ino, south pole and pyhäsalmi
publisher arXiv
publishDate 2012
url https://dx.doi.org/10.48550/arxiv.1210.5154
https://arxiv.org/abs/1210.5154
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_relation https://dx.doi.org/10.1016/j.physletb.2012.12.016
op_rights arXiv.org perpetual, non-exclusive license
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
op_doi https://doi.org/10.48550/arxiv.1210.5154
https://doi.org/10.1016/j.physletb.2012.12.016
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