Sensitivity to Non-Standard Interactions (NSI) with KM3NeT-ORCA
International audience ORCA (Oscillations Research with Cosmics in the Abyss) is the low-energy detector of KM3NeT, the next generation underwater Cherenkov neutrino detector in the Mediterranean Sea. Although its primary goal is to determine the Neutrino Mass Ordering (NMO) with atmospheric neutrin...
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ftccsdartic:oai:HAL:hal-02966281v1 2023-05-15T17:53:12+02:00 Sensitivity to Non-Standard Interactions (NSI) with KM3NeT-ORCA Khan Chowdhury, N.R. Thakore, T. Coelho, J.A. B. Zornoza, J.D. Navas, S. Laboratoire de l'Accélérateur Linéaire (LAL) Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS) KM3NeT Madison, United States 2019-07-24 https://hal.archives-ouvertes.fr/hal-02966281 https://doi.org/10.22323/1.358.0931 en eng HAL CCSD info:eu-repo/semantics/altIdentifier/doi/10.22323/1.358.0931 hal-02966281 https://hal.archives-ouvertes.fr/hal-02966281 doi:10.22323/1.358.0931 INSPIRE: 1819172 PoS 36th International Cosmic Ray Conference https://hal.archives-ouvertes.fr/hal-02966281 36th International Cosmic Ray Conference, Jul 2019, Madison, United States. pp.931, ⟨10.22323/1.358.0931⟩ new physics KM3NeT numerical calculations Cherenkov counter sensitivity neutrino: mass: hierarchy neutrino: detector neutrino: oscillation neutrino: atmosphere neutrino: interaction [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] info:eu-repo/semantics/conferenceObject Conference papers 2019 ftccsdartic https://doi.org/10.22323/1.358.0931 2021-09-11T22:51:39Z International audience ORCA (Oscillations Research with Cosmics in the Abyss) is the low-energy detector of KM3NeT, the next generation underwater Cherenkov neutrino detector in the Mediterranean Sea. Although its primary goal is to determine the Neutrino Mass Ordering (NMO) with atmospheric neutrinos, its access to a wide range of energies and baselines makes it optimal to discover exotic physics beyond the Standard Model (SM) such as Non-Standard Interactions (NSI).Non-Standard Interactions with neutrinos will introduce modifications in the SM potential, which will alter the event spectra at the ORCA detector. Using these NSI induced distortions inthe flavour content over three flavour standard oscillations, it is possible to constrain NSI modelparameters. This report outlines the sensitivity that ORCA can achieve in puttingupper bounds on some of these non-standard neutrino interaction parameters. Conference Object Orca Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe) Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019) 931 |
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Open Polar |
collection |
Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe) |
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ftccsdartic |
language |
English |
topic |
new physics KM3NeT numerical calculations Cherenkov counter sensitivity neutrino: mass: hierarchy neutrino: detector neutrino: oscillation neutrino: atmosphere neutrino: interaction [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] |
spellingShingle |
new physics KM3NeT numerical calculations Cherenkov counter sensitivity neutrino: mass: hierarchy neutrino: detector neutrino: oscillation neutrino: atmosphere neutrino: interaction [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] Khan Chowdhury, N.R. Thakore, T. Coelho, J.A. B. Zornoza, J.D. Navas, S. Sensitivity to Non-Standard Interactions (NSI) with KM3NeT-ORCA |
topic_facet |
new physics KM3NeT numerical calculations Cherenkov counter sensitivity neutrino: mass: hierarchy neutrino: detector neutrino: oscillation neutrino: atmosphere neutrino: interaction [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] |
description |
International audience ORCA (Oscillations Research with Cosmics in the Abyss) is the low-energy detector of KM3NeT, the next generation underwater Cherenkov neutrino detector in the Mediterranean Sea. Although its primary goal is to determine the Neutrino Mass Ordering (NMO) with atmospheric neutrinos, its access to a wide range of energies and baselines makes it optimal to discover exotic physics beyond the Standard Model (SM) such as Non-Standard Interactions (NSI).Non-Standard Interactions with neutrinos will introduce modifications in the SM potential, which will alter the event spectra at the ORCA detector. Using these NSI induced distortions inthe flavour content over three flavour standard oscillations, it is possible to constrain NSI modelparameters. This report outlines the sensitivity that ORCA can achieve in puttingupper bounds on some of these non-standard neutrino interaction parameters. |
author2 |
Laboratoire de l'Accélérateur Linéaire (LAL) Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS) KM3NeT |
format |
Conference Object |
author |
Khan Chowdhury, N.R. Thakore, T. Coelho, J.A. B. Zornoza, J.D. Navas, S. |
author_facet |
Khan Chowdhury, N.R. Thakore, T. Coelho, J.A. B. Zornoza, J.D. Navas, S. |
author_sort |
Khan Chowdhury, N.R. |
title |
Sensitivity to Non-Standard Interactions (NSI) with KM3NeT-ORCA |
title_short |
Sensitivity to Non-Standard Interactions (NSI) with KM3NeT-ORCA |
title_full |
Sensitivity to Non-Standard Interactions (NSI) with KM3NeT-ORCA |
title_fullStr |
Sensitivity to Non-Standard Interactions (NSI) with KM3NeT-ORCA |
title_full_unstemmed |
Sensitivity to Non-Standard Interactions (NSI) with KM3NeT-ORCA |
title_sort |
sensitivity to non-standard interactions (nsi) with km3net-orca |
publisher |
HAL CCSD |
publishDate |
2019 |
url |
https://hal.archives-ouvertes.fr/hal-02966281 https://doi.org/10.22323/1.358.0931 |
op_coverage |
Madison, United States |
genre |
Orca |
genre_facet |
Orca |
op_source |
PoS 36th International Cosmic Ray Conference https://hal.archives-ouvertes.fr/hal-02966281 36th International Cosmic Ray Conference, Jul 2019, Madison, United States. pp.931, ⟨10.22323/1.358.0931⟩ |
op_relation |
info:eu-repo/semantics/altIdentifier/doi/10.22323/1.358.0931 hal-02966281 https://hal.archives-ouvertes.fr/hal-02966281 doi:10.22323/1.358.0931 INSPIRE: 1819172 |
op_doi |
https://doi.org/10.22323/1.358.0931 |
container_title |
Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019) |
container_start_page |
931 |
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1766160908649758720 |