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Search for Neutrino Doublets and Triplets Using 11.4 yr of IceCube Data
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: 4272025 (English)In: Astrophysical Journal, ISSN 0004-637X, E-ISSN 1538-4357, Vol. 981, no 2, article id 159Article in journal (Refereed) Published
Abstract [en]

We report a search for high-energy astrophysical neutrino multiplets, detections of multiple neutrino clusters in the same direction within 30 days, based on an analysis of 11.4 yr of IceCube data. A new search method optimized for transient neutrino emission with a monthly timescale is employed, providing a higher sensitivity to neutrino fluxes. This result is sensitive to neutrino transient emission, reaching per-flavor flux of approximately 1 0 − 10 erg cm − 2 s − 1 from the Northern Sky in the energy range E ≳ 50 TeV. The number of doublets and triplets identified in this search is compatible with the atmospheric background hypothesis, which leads us to set limits on the nature of neutrino transient sources with emission timescales of one month.

Place, publisher, year, edition, pages
2025. Vol. 981, no 2, article id 159
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Astronomy, Astrophysics and Cosmology
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URN: urn:nbn:se:su:diva-241909DOI: 10.3847/1538-4357/adb312ISI: 001449300400001Scopus ID: 2-s2.0-105000437193OAI: oai:DiVA.org:su-241909DiVA, id: diva2:1951553
Available from: 2025-04-11 Created: 2025-04-11 Last updated: 2025-04-11Bibliographically approved

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Finley, ChadHidvegi, AttilaHultqvist, KlasNeste, LudwigWalck, Christian

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