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Measurement of Atmospheric Neutrino Oscillation Parameters Using Convolutional Neural Networks with 9.3 Years of Data in IceCube DeepCore
Stockholm University, Faculty of Science, Department of Physics. Stockholm University, Faculty of Science, The Oskar Klein Centre for Cosmo Particle Physics (OKC).ORCID iD: 0000-0003-3350-390x
Stockholm University, Faculty of Science, Department of Physics. Stockholm University, Faculty of Science, The Oskar Klein Centre for Cosmo Particle Physics (OKC).
Stockholm University, Faculty of Science, Department of Physics. Stockholm University, Faculty of Science, The Oskar Klein Centre for Cosmo Particle Physics (OKC).ORCID iD: 0000-0003-0602-9472
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Number of Authors: 4262025 (English)In: Physical Review Letters, ISSN 0031-9007, E-ISSN 1079-7114, Vol. 134, no 9, article id 091801Article in journal (Refereed) Published
Abstract [en]

The DeepCore subdetector of the IceCube Neutrino Observatory provides access to neutrinos with energies above approximately 5 GeV. Data taken between 2012 and 2021 (3387 days) are utilized for an atmospheric nu(mu) disappearance analysis that studied 150 257 neutrino-candidate events with reconstructed energies between 5 and 100 GeV. An advanced reconstruction based on a convolutional neural network is applied, providing increased signal efficiency and background suppression, resulting in a measurement with both significantly increased statistics compared to previous DeepCore oscillation results and high neutrino purity. For the normal neutrino mass ordering, the atmospheric neutrino oscillation parameters and their 1 sigma errors are measured to be Delta m(32)(2) = 2.40(-0.04)(+0.05) x 10(-3) eV(2) and sin(2)theta(23) = 0.54(-0.03)(+0.04). The results are the most precise to date using atmospheric neutrinos, and are compatible with measurements from other neutrino detectors including long-baseline accelerator experiments.

Place, publisher, year, edition, pages
2025. Vol. 134, no 9, article id 091801
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Subatomic Physics
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URN: urn:nbn:se:su:diva-247805DOI: 10.1103/PhysRevLett.134.091801ISI: 001498354800001PubMedID: 40131048Scopus ID: 2-s2.0-105001999636OAI: oai:DiVA.org:su-247805DiVA, id: diva2:2008213
Available from: 2025-10-22 Created: 2025-10-22 Last updated: 2025-10-22Bibliographically approved

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Finley, ChadHidvegi, AttilaHultqvist, KlasNeste, LudwigWalck, Christian

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