Neutrino non-standard interactions with the KM3NeT/ORCA detector
KM3NeT/ORCA is a dense array that constitutes the low-energy branch of the KM3NeT project with the main goal of resolving the question of the neutrino mass ordering. At present, the KM3NeT/ORCA Phase 1 has already been deployed, which means that six out of the planned 115 detection lines are operati...
Main Authors: | , , , , , , , , , |
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Other Authors: | , |
Format: | Conference Object |
Language: | English |
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arXiv
2021
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Online Access: | http://hdl.handle.net/2117/385221 |
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author | Ageron, M. Aiello, S Alshamsi, Mohammed Ambrosone, Antonio André, Michel Androulakis, Giorgos Anghinolfi, Marco Anton, Gisela Ardid Ramírez, Miguel Aublin, J. |
author2 | Centre Tecnològic de Vilanova i la Geltrú Universitat Politècnica de Catalunya. LAB - Laboratori d'Aplicacions Bioacústiques |
author_facet | Ageron, M. Aiello, S Alshamsi, Mohammed Ambrosone, Antonio André, Michel Androulakis, Giorgos Anghinolfi, Marco Anton, Gisela Ardid Ramírez, Miguel Aublin, J. |
author_sort | Ageron, M. |
collection | Universitat Politècnica de Catalunya, BarcelonaTech: UPCommons - Global access to UPC knowledge |
description | KM3NeT/ORCA is a dense array that constitutes the low-energy branch of the KM3NeT project with the main goal of resolving the question of the neutrino mass ordering. At present, the KM3NeT/ORCA Phase 1 has already been deployed, which means that six out of the planned 115 detection lines are operational. Even with this limited configuration, neutrino oscillations can already be measured and studied. In this contribution, the sensitivity to the neutrino Non-Standard Interactions (NSI) parameter eµt using the current stage of the KM3NeT/ORCA detector together with the projections for the final configuration are presented. Postprint (published version) |
format | Conference Object |
genre | Orca |
genre_facet | Orca |
id | ftupcatalunyair:oai:upcommons.upc.edu:2117/385221 |
institution | Open Polar |
language | English |
op_collection_id | ftupcatalunyair |
op_relation | https://pos.sissa.it/395/1165/ Ageron, M. [et al.]. Neutrino non-standard interactions with the KM3NeT/ORCA detector. A: International Cosmic Ray Conference. "37th International Cosmic Ray Conference: ICRC2021: 12-23 July 2021, Berlin, Germany-online". Ithaca, NY: arXiv, 2021, ISBN 18248039. 18248039 http://hdl.handle.net/2117/385221 |
op_rights | Attribution-NonCommercial-NoDerivatives 4.0 International http://creativecommons.org/licenses/by-nc-nd/4.0/ Open Access |
publishDate | 2021 |
publisher | arXiv |
record_format | openpolar |
spelling | ftupcatalunyair:oai:upcommons.upc.edu:2117/385221 2025-01-17T00:08:59+00:00 Neutrino non-standard interactions with the KM3NeT/ORCA detector Ageron, M. Aiello, S Alshamsi, Mohammed Ambrosone, Antonio André, Michel Androulakis, Giorgos Anghinolfi, Marco Anton, Gisela Ardid Ramírez, Miguel Aublin, J. Centre Tecnològic de Vilanova i la Geltrú Universitat Politècnica de Catalunya. LAB - Laboratori d'Aplicacions Bioacústiques 2021 application/pdf http://hdl.handle.net/2117/385221 eng eng arXiv https://pos.sissa.it/395/1165/ Ageron, M. [et al.]. Neutrino non-standard interactions with the KM3NeT/ORCA detector. A: International Cosmic Ray Conference. "37th International Cosmic Ray Conference: ICRC2021: 12-23 July 2021, Berlin, Germany-online". Ithaca, NY: arXiv, 2021, ISBN 18248039. 18248039 http://hdl.handle.net/2117/385221 Attribution-NonCommercial-NoDerivatives 4.0 International http://creativecommons.org/licenses/by-nc-nd/4.0/ Open Access Àrees temàtiques de la UPC::Física::Astronomia i astrofísica Neutrinos Neutrino astrophysics Astronomy--Observations Particle detectors Dense arrays Interaction parameters Lower energies Neutrino mass Neutrino oscillations Neutrons Neutrins Astrofísica Conference report 2021 ftupcatalunyair 2024-07-25T11:14:09Z KM3NeT/ORCA is a dense array that constitutes the low-energy branch of the KM3NeT project with the main goal of resolving the question of the neutrino mass ordering. At present, the KM3NeT/ORCA Phase 1 has already been deployed, which means that six out of the planned 115 detection lines are operational. Even with this limited configuration, neutrino oscillations can already be measured and studied. In this contribution, the sensitivity to the neutrino Non-Standard Interactions (NSI) parameter eµt using the current stage of the KM3NeT/ORCA detector together with the projections for the final configuration are presented. Postprint (published version) Conference Object Orca Universitat Politècnica de Catalunya, BarcelonaTech: UPCommons - Global access to UPC knowledge |
spellingShingle | Àrees temàtiques de la UPC::Física::Astronomia i astrofísica Neutrinos Neutrino astrophysics Astronomy--Observations Particle detectors Dense arrays Interaction parameters Lower energies Neutrino mass Neutrino oscillations Neutrons Neutrins Astrofísica Ageron, M. Aiello, S Alshamsi, Mohammed Ambrosone, Antonio André, Michel Androulakis, Giorgos Anghinolfi, Marco Anton, Gisela Ardid Ramírez, Miguel Aublin, J. Neutrino non-standard interactions with the KM3NeT/ORCA detector |
title | Neutrino non-standard interactions with the KM3NeT/ORCA detector |
title_full | Neutrino non-standard interactions with the KM3NeT/ORCA detector |
title_fullStr | Neutrino non-standard interactions with the KM3NeT/ORCA detector |
title_full_unstemmed | Neutrino non-standard interactions with the KM3NeT/ORCA detector |
title_short | Neutrino non-standard interactions with the KM3NeT/ORCA detector |
title_sort | neutrino non-standard interactions with the km3net/orca detector |
topic | Àrees temàtiques de la UPC::Física::Astronomia i astrofísica Neutrinos Neutrino astrophysics Astronomy--Observations Particle detectors Dense arrays Interaction parameters Lower energies Neutrino mass Neutrino oscillations Neutrons Neutrins Astrofísica |
topic_facet | Àrees temàtiques de la UPC::Física::Astronomia i astrofísica Neutrinos Neutrino astrophysics Astronomy--Observations Particle detectors Dense arrays Interaction parameters Lower energies Neutrino mass Neutrino oscillations Neutrons Neutrins Astrofísica |
url | http://hdl.handle.net/2117/385221 |