Sensitivity to light sterile neutrino mixing parameters with KM3NeT/ORCA
International audience KM3NeT/ORCA is a next-generation neutrino telescope optimised for atmospheric neutrino oscillations studies. In this paper, the sensitivity of ORCA to the presence of a light sterile neutrino in a 3+1 model is presented. After three years of data taking, ORCA will be able to p...
Published in: | Journal of High Energy Physics |
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Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Other Authors: | , , , , , , , , , , , , , , |
Format: | Article in Journal/Newspaper |
Language: | English |
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HAL CCSD
2021
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Online Access: | https://hal.archives-ouvertes.fr/hal-03325201 https://doi.org/10.1007/JHEP10(2021)180 |
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ftccsdartic:oai:HAL:hal-03325201v1 |
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openpolar |
institution |
Open Polar |
collection |
Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe) |
op_collection_id |
ftccsdartic |
language |
English |
topic |
proposed experiment numerical calculations: Monte Carlo anomaly cosmological model neutrino: mass difference neutrino: mixing angle KM3NeT sensitivity neutrino: oscillation neutrino: mixing neutrino: atmosphere neutrino: detector neutrino: sterile Neutrino Detectors and Telescopes (experiments) Oscillation [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex] |
spellingShingle |
proposed experiment numerical calculations: Monte Carlo anomaly cosmological model neutrino: mass difference neutrino: mixing angle KM3NeT sensitivity neutrino: oscillation neutrino: mixing neutrino: atmosphere neutrino: detector neutrino: sterile Neutrino Detectors and Telescopes (experiments) Oscillation [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex] Aiello, S. Albert, A. Alshamsi, M. Alves Garre, S. Aly, Z. Ambrosone, A. Ameli, F. Andre, M. Androulakis, G. Anghinolfi, M. Anguita, M. Anton, G. Ardid, M. Ardid, S. Aublin, J. Bagatelas, C. Baret, B. Basegmez du Pree, S. Bendahman, M. Benfenati, F. Berbee, E. Berg, A.M. van den Bertin, V. Biagi, S. Bissinger, M. Boettcher, M. Bou Cabo, M. Boumaaza, J. Bouta, M. Bouwhuis, M. Bozza, C. Brânzaş, H. Bretaudeau, F. Bruijn, R. Brunner, J. Bruno, R. Buis, E. Buompane, R. Busto, J. Caiffi, B. Calvo, D. Campion, S. Capone, A. Carretero, V. Castaldi, P. Celli, S. Chabab, M. Chau, N. Chen, A. Cherubini, S. Sensitivity to light sterile neutrino mixing parameters with KM3NeT/ORCA |
topic_facet |
proposed experiment numerical calculations: Monte Carlo anomaly cosmological model neutrino: mass difference neutrino: mixing angle KM3NeT sensitivity neutrino: oscillation neutrino: mixing neutrino: atmosphere neutrino: detector neutrino: sterile Neutrino Detectors and Telescopes (experiments) Oscillation [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex] |
description |
International audience KM3NeT/ORCA is a next-generation neutrino telescope optimised for atmospheric neutrino oscillations studies. In this paper, the sensitivity of ORCA to the presence of a light sterile neutrino in a 3+1 model is presented. After three years of data taking, ORCA will be able to probe the active-sterile mixing angles θ$_{14}$, θ$_{24}$, θ$_{34}$ and the effective angle θ$_{μe}$, over a broad range of mass squared difference $ \Delta {m}_{41}^2 $ ∼ [10$^{−5}$, 10] eV$^{2}$, allowing to test the eV-mass sterile neutrino hypothesis as the origin of short baseline anomalies, as well as probing the hypothesis of a very light sterile neutrino, not yet constrained by cosmology. ORCA will be able to explore a relevant fraction of the parameter space not yet reached by present measurements.[graphic not available: see fulltext] |
author2 |
Institut Pluridisciplinaire Hubert Curien (IPHC) Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS) IUT de Colmar AstroParticule et Cosmologie (APC (UMR_7164)) Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP) Centre de Physique des Particules de Marseille (CPPM) Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS) Laboratoire de physique subatomique et des technologies associées (SUBATECH) Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST) Université de Nantes (UN)-Université de Nantes (UN)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique) Institut Mines-Télécom Paris (IMT)-Institut Mines-Télécom Paris (IMT) Laboratoire Univers et Particules de Montpellier (LUPM) Centre National de la Recherche Scientifique (CNRS)-Université de Montpellier (UM)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Montpellier 2 - Sciences et Techniques (UM2) KM3NeT |
format |
Article in Journal/Newspaper |
author |
Aiello, S. Albert, A. Alshamsi, M. Alves Garre, S. Aly, Z. Ambrosone, A. Ameli, F. Andre, M. Androulakis, G. Anghinolfi, M. Anguita, M. Anton, G. Ardid, M. Ardid, S. Aublin, J. Bagatelas, C. Baret, B. Basegmez du Pree, S. Bendahman, M. Benfenati, F. Berbee, E. Berg, A.M. van den Bertin, V. Biagi, S. Bissinger, M. Boettcher, M. Bou Cabo, M. Boumaaza, J. Bouta, M. Bouwhuis, M. Bozza, C. Brânzaş, H. Bretaudeau, F. Bruijn, R. Brunner, J. Bruno, R. Buis, E. Buompane, R. Busto, J. Caiffi, B. Calvo, D. Campion, S. Capone, A. Carretero, V. Castaldi, P. Celli, S. Chabab, M. Chau, N. Chen, A. Cherubini, S. |
author_facet |
Aiello, S. Albert, A. Alshamsi, M. Alves Garre, S. Aly, Z. Ambrosone, A. Ameli, F. Andre, M. Androulakis, G. Anghinolfi, M. Anguita, M. Anton, G. Ardid, M. Ardid, S. Aublin, J. Bagatelas, C. Baret, B. Basegmez du Pree, S. Bendahman, M. Benfenati, F. Berbee, E. Berg, A.M. van den Bertin, V. Biagi, S. Bissinger, M. Boettcher, M. Bou Cabo, M. Boumaaza, J. Bouta, M. Bouwhuis, M. Bozza, C. Brânzaş, H. Bretaudeau, F. Bruijn, R. Brunner, J. Bruno, R. Buis, E. Buompane, R. Busto, J. Caiffi, B. Calvo, D. Campion, S. Capone, A. Carretero, V. Castaldi, P. Celli, S. Chabab, M. Chau, N. Chen, A. Cherubini, S. |
author_sort |
Aiello, S. |
title |
Sensitivity to light sterile neutrino mixing parameters with KM3NeT/ORCA |
title_short |
Sensitivity to light sterile neutrino mixing parameters with KM3NeT/ORCA |
title_full |
Sensitivity to light sterile neutrino mixing parameters with KM3NeT/ORCA |
title_fullStr |
Sensitivity to light sterile neutrino mixing parameters with KM3NeT/ORCA |
title_full_unstemmed |
Sensitivity to light sterile neutrino mixing parameters with KM3NeT/ORCA |
title_sort |
sensitivity to light sterile neutrino mixing parameters with km3net/orca |
publisher |
HAL CCSD |
publishDate |
2021 |
url |
https://hal.archives-ouvertes.fr/hal-03325201 https://doi.org/10.1007/JHEP10(2021)180 |
genre |
Orca |
genre_facet |
Orca |
op_source |
JHEP https://hal.archives-ouvertes.fr/hal-03325201 JHEP, 2021, 10, pp.180. ⟨10.1007/JHEP10(2021)180⟩ |
op_relation |
info:eu-repo/semantics/altIdentifier/arxiv/2107.00344 info:eu-repo/semantics/altIdentifier/doi/10.1007/JHEP10(2021)180 hal-03325201 https://hal.archives-ouvertes.fr/hal-03325201 ARXIV: 2107.00344 doi:10.1007/JHEP10(2021)180 INSPIRE: 1873786 |
op_doi |
https://doi.org/10.1007/JHEP10(2021)180 |
container_title |
Journal of High Energy Physics |
container_volume |
2021 |
container_issue |
10 |
_version_ |
1766160821218443264 |
spelling |
ftccsdartic:oai:HAL:hal-03325201v1 2023-05-15T17:53:06+02:00 Sensitivity to light sterile neutrino mixing parameters with KM3NeT/ORCA Aiello, S. Albert, A. Alshamsi, M. Alves Garre, S. Aly, Z. Ambrosone, A. Ameli, F. Andre, M. Androulakis, G. Anghinolfi, M. Anguita, M. Anton, G. Ardid, M. Ardid, S. Aublin, J. Bagatelas, C. Baret, B. Basegmez du Pree, S. Bendahman, M. Benfenati, F. Berbee, E. Berg, A.M. van den Bertin, V. Biagi, S. Bissinger, M. Boettcher, M. Bou Cabo, M. Boumaaza, J. Bouta, M. Bouwhuis, M. Bozza, C. Brânzaş, H. Bretaudeau, F. Bruijn, R. Brunner, J. Bruno, R. Buis, E. Buompane, R. Busto, J. Caiffi, B. Calvo, D. Campion, S. Capone, A. Carretero, V. Castaldi, P. Celli, S. Chabab, M. Chau, N. Chen, A. Cherubini, S. Institut Pluridisciplinaire Hubert Curien (IPHC) Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS) IUT de Colmar AstroParticule et Cosmologie (APC (UMR_7164)) Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP) Centre de Physique des Particules de Marseille (CPPM) Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS) Laboratoire de physique subatomique et des technologies associées (SUBATECH) Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST) Université de Nantes (UN)-Université de Nantes (UN)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique) Institut Mines-Télécom Paris (IMT)-Institut Mines-Télécom Paris (IMT) Laboratoire Univers et Particules de Montpellier (LUPM) Centre National de la Recherche Scientifique (CNRS)-Université de Montpellier (UM)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Montpellier 2 - Sciences et Techniques (UM2) KM3NeT 2021 https://hal.archives-ouvertes.fr/hal-03325201 https://doi.org/10.1007/JHEP10(2021)180 en eng HAL CCSD info:eu-repo/semantics/altIdentifier/arxiv/2107.00344 info:eu-repo/semantics/altIdentifier/doi/10.1007/JHEP10(2021)180 hal-03325201 https://hal.archives-ouvertes.fr/hal-03325201 ARXIV: 2107.00344 doi:10.1007/JHEP10(2021)180 INSPIRE: 1873786 JHEP https://hal.archives-ouvertes.fr/hal-03325201 JHEP, 2021, 10, pp.180. ⟨10.1007/JHEP10(2021)180⟩ proposed experiment numerical calculations: Monte Carlo anomaly cosmological model neutrino: mass difference neutrino: mixing angle KM3NeT sensitivity neutrino: oscillation neutrino: mixing neutrino: atmosphere neutrino: detector neutrino: sterile Neutrino Detectors and Telescopes (experiments) Oscillation [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex] info:eu-repo/semantics/article Journal articles 2021 ftccsdartic https://doi.org/10.1007/JHEP10(2021)180 2021-11-27T23:42:22Z International audience KM3NeT/ORCA is a next-generation neutrino telescope optimised for atmospheric neutrino oscillations studies. In this paper, the sensitivity of ORCA to the presence of a light sterile neutrino in a 3+1 model is presented. After three years of data taking, ORCA will be able to probe the active-sterile mixing angles θ$_{14}$, θ$_{24}$, θ$_{34}$ and the effective angle θ$_{μe}$, over a broad range of mass squared difference $ \Delta {m}_{41}^2 $ ∼ [10$^{−5}$, 10] eV$^{2}$, allowing to test the eV-mass sterile neutrino hypothesis as the origin of short baseline anomalies, as well as probing the hypothesis of a very light sterile neutrino, not yet constrained by cosmology. ORCA will be able to explore a relevant fraction of the parameter space not yet reached by present measurements.[graphic not available: see fulltext] Article in Journal/Newspaper Orca Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe) Journal of High Energy Physics 2021 10 |