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Exploration of mass splitting and muon/tau mixing parameters for an eV-scale sterile neutrino with IceCube
Loyola Univ Chicago, Dept Phys, Chicago, IL 60660 USA.
Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, High Energy Physics.ORCID iD: 0000-0002-7448-4189
Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, High Energy Physics.ORCID iD: 0000-0001-8588-7306
Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, High Energy Physics.ORCID iD: 0000-0003-1510-1712
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Number of Authors: 4232024 (English)In: Physics Letters B, ISSN 0370-2693, E-ISSN 1873-2445, Vol. 858, article id 139077Article in journal (Refereed) Published
Abstract [en]

We present the first three-parameter fit to a 3+1 sterile neutrino model using 7.634 years of data from the IceCube Neutrino Observatory on nu(mu) + (nu) over bar (mu) charged-current interactions in the energy range 500-9976 GeV. Our analysis is sensitive to the mass-squared splitting between the heaviest and lightest mass state (Delta m(41)(2)), the mixing matrix element connecting muon flavor to the fourth mass state (vertical bar U-mu 4 vertical bar(2)), and the element connecting tau flavor to the fourth mass state (vertical bar U-tau 4 vertical bar(2)). Predicted propagation effects in matter enhance the signature through a resonance as atmospheric neutrinos from the Northern Hemisphere traverse the Earth to the IceCube detector at the South Pole. The remaining sterile neutrino matrix elements are left fixed, with vertical bar U-e4 vertical bar(2) = 0 and delta(14) = 0, as they have a negligible effect, and delta(24) = pi is set to give the most conservative limits. The result is consistent with the no-sterile neutrino hypothesis with a probability of 4.3%. Profiling the likelihood of each parameter yields the 90% confidence levels: 2.4 eV(2) < Delta m(41)(2) < 9.6 eV(2), 0.0081 < vertical bar U-mu 4 vertical bar(2) < 0.10, and vertical bar U-tau 4 vertical bar(2) < 0.035, which narrows the allowed parameter-space for vertical bar U-tau 4 vertical bar(2). However, the primary result of this analysis is the first map of the 3+1 parameter space exploring the interdependence of Delta m(41)(2), vertical bar U-mu 4 vertical bar(2), and |U-tau 4 vertical bar(2).

Place, publisher, year, edition, pages
Elsevier, 2024. Vol. 858, article id 139077
Keywords [en]
Atmospheric neutrino IceCube TeV oscillation sterile
National Category
Subatomic Physics
Identifiers
URN: urn:nbn:se:uu:diva-547661DOI: 10.1016/j.physletb.2024.139077ISI: 001381336400001Scopus ID: 2-s2.0-85206874882OAI: oai:DiVA.org:uu-547661DiVA, id: diva2:1928841
Funder
German Research Foundation (DFG)Swedish Research CouncilSwedish National Infrastructure for Computing (SNIC)Knut and Alice Wallenberg FoundationAustralian Research Council
Note

For complete list of authors see http://dx.doi.org/10.1016/j.physletb.2024.139077

Available from: 2025-01-17 Created: 2025-01-17 Last updated: 2025-01-17Bibliographically approved

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Beise, JakobBotner, OlgaColeman, AlanGlaser, ChristianGlüsenkamp, ThorstenHallgren, AllanHeyer, NilsO'Sullivan, ErinPérez de los Heros, CarlosPontén, AxelRavn, MartinValtonen-Mattila, Nora

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Beise, JakobBotner, OlgaColeman, AlanGlaser, ChristianGlüsenkamp, ThorstenHallgren, AllanHeyer, NilsO'Sullivan, ErinPérez de los Heros, CarlosPontén, AxelRavn, MartinValtonen-Mattila, Nora
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High Energy Physics
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Physics Letters B
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