Measurement of neutrino oscillation parameters with the first six detection units of KM3NeT/ORCA
Metadatos
Afficher la notice complèteAuteur
Aiello, S.; Díaz García, Antonio Francisco; Gutiérrez González, Miguel; Navas Concha, Sergio; KM3NeT collaboration, /Editorial
Springer Nature
Materia
Neutrino Detectors and Telescopes (experiments), Oscillation
Date
2024-10-29Referencia bibliográfica
Aiello, S. $ Díaz García, A.F. & Guitéerez Gonzáles, M. & Navas Concha, S. & KM3NeT collaboration. et. al. J. High Energ. Phys. 2024, 206 (2024). [https://doi.org/10.1007/JHEP10(2024)206]
Patrocinador
Scientific Research (FRS-FNRS), Francqui foundation, BAEF foundation; Czech Science Foundation (GAČR 24-12702S); Agence Nationale de la Recherche (contract ANR-15-CE31-0020), Centre National de la Recherche Scientifique (CNRS), Commission Européenne (FEDER fund and Marie Curie Program), LabEx UnivEarthS (ANR-10-LABX-0023 and ANR-18-IDEX-0001), Paris Île-de-France Region, Normandy Region (Alpha, Blue-waves and Neptune), France; Shota Rustaveli National Science Foundation of Georgia (SRNSFG, FR-22-13708), Georgia; MuSES project which has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 Research and Innovation Programme (grant agreement No 101142396); General Secretariat of Research and Innovation (GSRI), Greece; to Nazionale di Fisica Nucleare (INFN) and Ministero dell’Università e della Ricerca (MUR), through PRIN 2022 program (Grant PANTHEON 2022E2J4RK, Next Generation EU) and PON R&I program (Avviso n. 424 del 28 febbraio 2018, Progetto PACK-PIR01 00021), Italy; IDMAR project Po-Fesr Sicilian Region az. 1.5.1; Italian Ministero dell’Università e della Ricerca (MUR), Progetto CIR01 00021 (Avviso n. 2595 del 24 dicembre 2019); KM3NeT4RR MUR Project National Recovery and Resilience Plan (NRRP), Mission 4 Component 2 Investment 3.1, Funded by the European Union – NextGenerationEU,CUP I57G21000040001, Concession Decree MUR No. n. Prot. 123 del 21/06/2022; Ministry of Higher Education, Scientific Research and Innovation, Morocco, and the Arab Fund for Economic and Social Development, Kuwait; Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands; istry of Research, Innovation and Digitalisation, Romania; Slovak Research and Development Agency under Contract No. APVV-22-0413; Ministry of Education, Research, Development and Youth of the Slovak Republic; MCIN for PID2021-124591NB-C41, -C42, -C43 and PDC2023-145913-I00 funded by MCIN/AEI/10.13039/501100011033 and by “ERDF A way of making Europe”, for ASFAE/2022/014 and ASFAE/2022 /023 with funding from the EU NextGenerationEU (PRTR-C17.I01) and Generalitat Valenciana, for Grant AST22_6.2 with funding from Consejería de Universidad, Investigación e Innovación and Gobierno de España and European Union - NextGenerationEU, for CSIC-INFRA23013 and for CNS2023-144099, Generalitat Valenciana for CIDEGENT/2018/034, /2019/043, /2020/049, /2021/23, for CIDEIG/2023/20, for CIPROM/2023/51 and for GRISOLIAP/2021/192 and EU for MSC/101025085, Spain; Khalifa University internal grants (ESIG-2023-008 and RIG-2023-070), United Arab Emirates; The European Union’s Horizon 2020 Research and Innovation Programme (ChETEC-INFRA - Project no. 101008324)Résumé
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
sin2 θ23 = 0.51+0.04
−0.05, and Δm2
31 = 2.18+0.25
−0.35 × 10−3 eV2 ∪ {−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.