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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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 |
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DataCite Metadata Store (German National Library of Science and Technology) |
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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 |
_version_ |
1766201178599718912 |