ÚTEFČVUT Ústav technické a experimentální fyziky ČVUT v PrazeInstitute of Experimental and Applied Physics, CTU in Prague

Updated results on neutrino Non-Standard Interactions with KM3NeT/ORCA6

NázevTitle
Updated results on neutrino Non-Standard Interactions with KM3NeT/ORCA6Updated results on neutrino Non-Standard Interactions with KM3NeT/ORCA6
Druh výsledkuResult type
Příspěvek ve sborníkuProceedings paper
AutořiAuthors
A.L. Pedrajas, S. Aiello, A. Albert, S. Alves Garre, Z. Bardačová, E. Eckerová, F. Mamedov, Y. Shitov, I. Štekl
Klíčová slovaKeywords
KM3NeT, neutrino telescope, neutrino Non-Standard Interactions
KonferenceConference
38th International Cosmic Ray Conference (Nagoya, Japan, 2023-07-26)
ExperimentCollaboration
KM3NeT
DOIDOI
10.22323/1.444.0998
Časopis / citaceJournal / citation
In: Proceedings of 38th International Cosmic Ray Conference — PoS(ICRC2023), Sissa Medialab, 2024, pp. 998 · ISSN 1824-8039
RokYear
2024
JazykLanguage
eng
ZáznamyRecords
ProjektProject
Laboratoire Souterrain de Modane - účast ČRLaboratoire Souterrain de Modane – participation of the Czech Republic; Institucionální podpora na rozvoj výzkumné org.Institucionální podpora na rozvoj výzkumné org.
CitovánoCited by
7 (INSPIRE-HEP)
2023: 12024: 6
Plný text (open access)Full text (open access)
https://pos.sissa.it/444/998/pdf
Citace ke staženíDownload citation
TXT · BibTeX

AbstraktAbstract

KM3NeT/ORCA is an underwater neutrino telescope currently under construction in the Mediterranean Sea, with the goal of measuring atmospheric neutrino oscillation parameters and determining the neutrino mass ordering. KM3NeT/ORCA can additionally provide constraints on physics beyond the Standard Model which could appear through strong matter effects, such as the neutrino Non-Standard Interactions (NSIs). This work reports on the results of the NSIs search with the final dataset of ORCA6, the first configuration of ORCA with six detection units, which uses 433 kton-years of exposure and improved calibration, reconstruction and selection methods compared to previous works. The obtained bounds at 90% CL, |εμτ| ≤ 5.5 · 10−3, |εeτ| ≤ 7.8 · 10−2, |εeμ| ≤ 5.8 · 10−2 and −0.015 ≤ εττ − εμμ ≤ 0.016, are comparable to the current most stringent limits on any NSIs parameter.

KM3NeT/ORCA is an underwater neutrino telescope currently under construction in the Mediterranean Sea, with the goal of measuring atmospheric neutrino oscillation parameters and determining the neutrino mass ordering. KM3NeT/ORCA can additionally provide constraints on physics beyond the Standard Model which could appear through strong matter effects, such as the neutrino Non-Standard Interactions (NSIs). This work reports on the results of the NSIs search with the final dataset of ORCA6, the first configuration of ORCA with six detection units, which uses 433 kton-years of exposure and improved calibration, reconstruction and selection methods compared to previous works. The obtained bounds at 90% CL, |εμτ| ≤ 5.5 · 10−3, |εeτ| ≤ 7.8 · 10−2, |εeμ| ≤ 5.8 · 10−2 and −0.015 ≤ εττ − εμμ ≤ 0.016, are comparable to the current most stringent limits on any NSIs parameter.

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