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dc.contributor.authorAartsen, M. G.
dc.contributor.authorBesson, David Zeke
dc.contributor.authorIceCube Collaboration
dc.date.accessioned2021-01-29T20:13:48Z
dc.date.available2021-01-29T20:13:48Z
dc.date.issued2019-02-15
dc.identifier.citationM. G. Aartsen et al., "Measurement of atmospheric tau neutrino appearance with IceCube DeepCore", Phys. Rev. D 99, 032007, 15 February 2019, American Physical Society, https://doi.org/10.1103/PhysRevD.99.032007en_US
dc.identifier.urihttp://hdl.handle.net/1808/31304
dc.descriptionThis work is licensed under a Creative Commons Attribution 4.0 International License.en_US
dc.description.abstractWe present a measurement of atmospheric tau neutrino appearance from oscillations with three years of data from the DeepCore subarray of the IceCube Neutrino Observatory. This analysis uses atmospheric neutrinos from the full sky with reconstructed energies between 5.6 and 56 GeV to search for a statistical excess of cascadelike neutrino events which are the signature of ντ interactions. For CC + NC (CC-only) interactions, we measure the tau neutrino normalization to be 0.73 +0.30 −0.24 (0.57 +0.36 −0.30) and exclude the absence of tau neutrino oscillations at a significance of 3.2σ (2.0σ) These results are consistent with, and of similar precision to, a confirmatory IceCube analysis also presented, as well as measurements performed by other experiments.en_US
dc.publisherAmerican Physical Societyen_US
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/en_US
dc.titleMeasurement of atmospheric tau neutrino appearance with IceCube DeepCoreen_US
dc.typeArticleen_US
kusw.kuauthorBesson, David Zeke
kusw.kudepartmentPhysics and Astronomyen_US
dc.identifier.doi10.1103/PhysRevD.99.032007en_US
kusw.oaversionScholarly/refereed, publisher versionen_US
kusw.oapolicyThis item meets KU Open Access policy criteria.en_US
dc.rights.accessrightsopenAccessen_US


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