Skip to main navigation Skip to search Skip to main content

Measurement of neutrino oscillation parameters 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
  • Mohammed V University in Rabat
  • 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
  • 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

19 Citations (Scopus)

Abstract

KM3NeT/ORCA is a water Cherenkov neutrino detector under construction and anchored at the bottom of the Mediterranean Sea. The detector is designed to study oscillations of atmospheric neutrinos and determine the neutrino mass ordering. This paper focuses on an initial configuration of ORCA, referred to as ORCA6, which comprises six out of the foreseen 115 detection units of photo-sensors. A high-purity neutrino sample was extracted, corresponding to an exposure of 433 kton-years. The sample of 5828 neutrino candidates is analysed following a binned log-likelihood method in the reconstructed energy and cosine of the zenith angle. The atmospheric oscillation parameters are measured to be sin2θ23=0.51−0.05+0.04, and Δm312=2.18−0.35+0.25×10−3eV2∪−2.25−1.76×10−3 eV2 at 68% CL. The inverted neutrino mass ordering hypothesis is disfavoured with a p-value of 0.25.

Original languageEnglish
Article number206
JournalJournal of High Energy Physics
Volume2024
Issue number10
DOIs
Publication statusPublished - Oct 2024

Keywords

  • Neutrino Detectors and Telescopes (experiments)
  • Oscillation

ASJC Scopus subject areas

  • Nuclear and High Energy Physics

Fingerprint

Dive into the research topics of 'Measurement of neutrino oscillation parameters with the first six detection units of KM3NeT/ORCA'. Together they form a unique fingerprint.

Cite this