Please use this identifier to cite or link to this item: http://hdl.handle.net/2440/117495
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dc.contributor.authorAartsen, M.G.en
dc.contributor.authorAckermann, M.en
dc.contributor.authorAdams, J.en
dc.contributor.authorAguilar, J.A.en
dc.contributor.authorAhlers, M.en
dc.contributor.authorAhrens, M.en
dc.contributor.authorSamarai, I.A.en
dc.contributor.authorAltmann, D.en
dc.contributor.authorAndeen, K.en
dc.contributor.authorAnderson, T.en
dc.contributor.authorAnsseau, I.en
dc.contributor.authorAnton, G.en
dc.contributor.authorArgüelles, C.en
dc.contributor.authorAuffenberg, J.en
dc.contributor.authorAxani, S.en
dc.contributor.authorBackes, P.en
dc.contributor.authorBagherpour, H.en
dc.contributor.authorBai, X.en
dc.contributor.authorBarron, J.P.en
dc.contributor.authorBarwick, S.W.en
dc.contributor.authoret al.en
dc.date.issued2018en
dc.identifier.citationEuropean Physical Journal C, 2018; 78(10):831-1-831-9en
dc.identifier.issn1434-6044en
dc.identifier.issn1434-6052en
dc.identifier.urihttp://hdl.handle.net/2440/117495-
dc.description.abstractWith the observation of high-energy astrophysical neutrinos by the IceCube Neutrino Observatory, interest has risen in models of PeV-mass decaying dark matter particles to explain the observed flux. We present two dedicated experimental analyses to test this hypothesis. One analysis uses 6 years of IceCube data focusing on muon neutrino ‘track’ events from the Northern Hemisphere, while the second analysis uses 2 years of ‘cascade’ events from the full sky. Known background components and the hypothetical flux from unstable dark matter are fitted to the experimental data. Since no significant excess is observed in either analysis, lower limits on the lifetime of dark matter particles are derived: we obtain the strongest constraint to date, excluding lifetimes shorter than 1028 s at 90% CL for dark matter masses above 10 TeV.en
dc.description.statementofresponsibilityM. G. Aartsen, M. Ackermann, J. Adams, J. A. Aguilar, M. Ahlers ... G. C. Hill ... et al.en
dc.language.isoenen
dc.publisherSpringeren
dc.rights© The Author(s) 2018. This article is distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made.en
dc.titleSearch for neutrinos from decaying dark matter with IceCube: IceCube Collaborationen
dc.typeJournal articleen
dc.identifier.rmid0030102488en
dc.identifier.doi10.1140/epjc/s10052-018-6273-3en
dc.identifier.pubid404968-
pubs.library.collectionPhysics publicationsen
pubs.library.teamDS10en
pubs.verification-statusVerifieden
pubs.publication-statusPublisheden
Appears in Collections:Physics publications

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