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Search for non-standard neutrino interactions with the first six detection units of KM3NeT/ORCA

  • the KM3NeT Collaboration
  • National Institute for Nuclear Physics
  • Université de Strasbourg
  • Université de Haute-Alsace
  • Khalifa University of Science and Technology
  • Aix-Marseille Université
  • University of Valencia
  • University of Naples Federico II
  • Polytechnic University of Catalonia
  • Nantes Université
  • Polytechnic University of Valencia
  • Université de Paris
  • University of Genoa
  • Université de Caen
  • Czech Technical University in Prague
  • Comenius University
  • University of Bologna
  • University of Campania Luigi Vanvitelli
  • LPC
  • University of Hull
  • National Institute for Subatomic Physics
  • North West University
  • Badji Mokhtar University
  • Mohammed V University in Rabat
  • University of Salerno
  • Institute for Space Sciences
  • University of Amsterdam
  • Netherlands Organisation for Applied Scientific Research
  • University of Rome La Sapienza
  • Cadi Ayyad University
  • University of the Witwatersrand
  • University of Catania
  • Université catholique de Louvain
  • University of Granada
  • Friedrich-Alexander University Erlangen-Nürnberg
  • Demokritos National Centre for Scientific Research
  • Mohamed I University
  • Western Sydney University
  • Royal Netherlands Institute for Sea Research - NIOZ
  • Leiden University
  • Ivane Javakhishvili Tbilisi State University
  • The University of Georgia, Tbilisi
  • Institut universitaire de France
  • Max Planck Institute for Radio Astronomy
  • Harvard University
  • Mohammed VI Polytechnic University
  • National Centre for Nuclear Research
  • Université Montpellier 2

Research output: Contribution to journalArticlepeer-review

6 Citations (Scopus)

Abstract

KM3NeT/ORCA is an underwater neutrino telescope under construction in the Mediterranean Sea. Its primary scientific goal is to measure the atmospheric neutrino oscillation parameters and to determine the neutrino mass ordering. ORCA can constrain the oscillation parameters Δm 231 and θ 23 by reconstructing the arrival direction and energy of multi-GeV neutrinos crossing the Earth. Searches for deviations from the Standard Model of particle physics in the forward scattering of neutrinos inside Earth matter, produced by Non-Standard Interactions, can be conducted by investigating distortions of the standard oscillation pattern of neutrinos of all flavours. This work reports on the results of the search for non-standard neutrino interactions using the first six detection units of ORCA and 433 kton-years of exposure. No significant deviation from standard interactions was found in a sample of 5828 events reconstructed in the 1 GeV-1 TeV energy range. The flavour structure of the non-standard coupling was constrained at 90% confidence level to be |ϵμτ | ≤ 5.4 × 10-3, |ϵ | ≤ 7.4 × 10-2, |ϵ | ≤ 5.6 × 10-2 and -0.015 ≤ ϵττ - ϵμμ ≤ 0.017. The results are comparable to the current most stringent limits placed on the parameters by other experiments.

Original languageEnglish
Article number073
JournalJournal of Cosmology and Astroparticle Physics
Volume2025
Issue number2
DOIs
Publication statusPublished - 1 Feb 2025

Keywords

  • neutrino experiments
  • neutrino properties
  • solar and atmospheric neutrinos

ASJC Scopus subject areas

  • Astronomy and Astrophysics

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