Neutrino non-standard interactions with the KM3NeT/ORCA detector

the KM3NeT Collaboration

Neutrino non-standard interactions with the KM3NeT/ORCA detector

the KM3NeT Collaboration

Physics

University of Valencia
Aix-Marseille Université
University of Padua
University of Granada
National Institute for Nuclear Physics
Université de Strasbourg
Université de Haute-Alsace
Université de Paris
IFIC (CSIC-Universitat de València)
University of Naples Federico II
Polytechnic University of Catalonia
Demokritos National Centre for Scientific Research
Friedrich-Alexander University Erlangen-Nürnberg
Polytechnic University of Valencia
National Institute for Subatomic Physics
Mohammed V University in Rabat
University of Bologna
University of Groningen
North West University
Unidad Mixta IEO-UPV
Mohamed I University
Nantes Université
University of Salerno
Institute for Space Sciences
University of Amsterdam
Netherlands Organisation for Applied Scientific Research
University of Campania Luigi Vanvitelli
University of Rome La Sapienza
Cadi Ayyad University
University of the Witwatersrand
University of Catania
International Centre for Radio Astronomy Research
University of Bari
University of Würzburg
Western Sydney University
University of Münster
University of Genoa
Université de Caen
Royal Netherlands Institute for Sea Research - NIOZ
Ivane Javakhishvili Tbilisi State University
Leiden University
National Centre for Nuclear Research
Utrecht University
Institut universitaire de France
University of Johannesburg
University of Tübingen
University of Pisa
Université Montpellier 2

Research output: Contribution to journal › Conference article › peer-review

Abstract

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 ε_μτ using the current stage of the KM3NeT/ORCA detector together with the projections for the final configuration are presented.

Original language	English
Article number	1165
Journal	Proceedings of Science
Volume	395
Publication status	Published - 18 Mar 2022
Event	37th International Cosmic Ray Conference, ICRC 2021 - Virtual, Berlin, Germany Duration: 12 Jul 2021 → 23 Jul 2021

ASJC Scopus subject areas

Multidisciplinary

Cite this

@article{bb1b902e85534700b864f0b27b4b0316,

title = "Neutrino non-standard interactions with the KM3NeT/ORCA detector",

abstract = "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 εμτ using the current stage of the KM3NeT/ORCA detector together with the projections for the final configuration are presented.",

author = "\{the KM3NeT Collaboration\} and Jerzy Ma{\'n}czak and Chowdhury, \{Nafis Rezwan Khan\} and Hern{\'a}ndez-Rey, \{Juan Jos{\'e}\} and Concha, \{Sergio Navas\} and M. Ageron and S. Aiello and A. Albert and M. Alshamsi and \{Alves Garre\}, S. and Z. Aly and A. Ambrosone and F. Ameli and M. Andre and G. Androulakis and M. Anghinolfi and M. Anguita and G. Anton and M. Ardid and S. Ardid and W. Assal and J. Aublin and C. Bagatelas and B. Baret and \{Basegmez du Pree\}, S. and M. Bendahman and F. Benfenati and E. Berbee and \{van den Berg\}, \{A. M.\} and V. Bertin and S. Beurthey and \{van Beveren\}, V. and S. Biagi and M. Billault and M. Bissinger and M. Boettcher and \{Bou Cabo\}, M. and J. Boumaaza and M. Bouta and C. Boutonnet and G. Bouvet and M. Bouwhuis and C. Bozza and H. Br{\^a}nza{\c s} and R. Bruijn and J. Brunner and R. Bruno and E. Buis and R. Buompane and J. Busto and S. Razzaque",

note = "Publisher Copyright: {\textcopyright} Copyright owned by the author(s).; 37th International Cosmic Ray Conference, ICRC 2021 ; Conference date: 12-07-2021 Through 23-07-2021",

year = "2022",

month = mar,

day = "18",

language = "English",

volume = "395",

journal = "Proceedings of Science",

issn = "1824-8039",

publisher = "Sissa Medialab Srl",

}

TY - JOUR

T1 - Neutrino non-standard interactions with the KM3NeT/ORCA detector

AU - the KM3NeT Collaboration

AU - Mańczak, Jerzy

AU - Chowdhury, Nafis Rezwan Khan

AU - Hernández-Rey, Juan José

AU - Concha, Sergio Navas

AU - Ageron, M.

AU - Aiello, S.

AU - Albert, A.

AU - Alshamsi, M.

AU - Alves Garre, S.

AU - Aly, Z.

AU - Ambrosone, A.

AU - Ameli, F.

AU - Andre, M.

AU - Androulakis, G.

AU - Anghinolfi, M.

AU - Anguita, M.

AU - Anton, G.

AU - Ardid, M.

AU - Ardid, S.

AU - Assal, W.

AU - Aublin, J.

AU - Bagatelas, C.

AU - Baret, B.

AU - Basegmez du Pree, S.

AU - Bendahman, M.

AU - Benfenati, F.

AU - Berbee, E.

AU - van den Berg, A. M.

AU - Bertin, V.

AU - Beurthey, S.

AU - van Beveren, V.

AU - Biagi, S.

AU - Billault, M.

AU - Bissinger, M.

AU - Boettcher, M.

AU - Bou Cabo, M.

AU - Boumaaza, J.

AU - Bouta, M.

AU - Boutonnet, C.

AU - Bouvet, G.

AU - Bouwhuis, M.

AU - Bozza, C.

AU - Brânzaş, H.

AU - Bruijn, R.

AU - Brunner, J.

AU - Bruno, R.

AU - Buis, E.

AU - Buompane, R.

AU - Busto, J.

AU - Razzaque, S.

PY - 2022/3/18

Y1 - 2022/3/18

N2 - 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 εμτ using the current stage of the KM3NeT/ORCA detector together with the projections for the final configuration are presented.

AB - 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 εμτ using the current stage of the KM3NeT/ORCA detector together with the projections for the final configuration are presented.

UR - https://www.scopus.com/pages/publications/85144590838

M3 - Conference article

AN - SCOPUS:85144590838

SN - 1824-8039

VL - 395

JO - Proceedings of Science

JF - Proceedings of Science

M1 - 1165

T2 - 37th International Cosmic Ray Conference, ICRC 2021

Y2 - 12 July 2021 through 23 July 2021

ER -

Neutrino non-standard interactions with the KM3NeT/ORCA detector

Abstract

ASJC Scopus subject areas

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