Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/79920
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dc.contributor.authorAartsen, M.-
dc.contributor.authorHill, G.-
dc.date.issued2013-
dc.identifier.citationPhysical Review Letters, 2013; 111(2):1-7-
dc.identifier.issn0031-9007-
dc.identifier.issn1079-7114-
dc.identifier.urihttp://hdl.handle.net/2440/79920-
dc.description.abstractWe report on the observation of two neutrino-induced events which have an estimated deposited energy in the IceCube detector of 1.04±0.16 and 1.14±0.17 PeV, respectively, the highest neutrino energies observed so far. These events are consistent with fully contained particle showers induced by neutral-current ν(e,μ,τ) (ν̅ (e,μ,τ)) or charged-current ν(e) (ν̅ e) interactions within the IceCube detector. The events were discovered in a search for ultrahigh energy neutrinos using data corresponding to 615.9 days effective live time. The expected number of atmospheric background is 0.082±0.004(stat)₋₀.₀₅₇⁺⁰.⁰⁴¹ (syst). The probability of observing two or more candidate events under the atmospheric background-only hypothesis is 2.9×10⁻³ (2.8σ) taking into account the uncertainty on the expected number of background events. These two events could be a first indication of an astrophysical neutrino flux; the moderate significance, however, does not permit a definitive conclusion at this time.-
dc.description.statementofresponsibilityM. G. Aartsen ... G. C. Hill ... et al. (IceCube Collaboration)-
dc.language.isoen-
dc.publisherAmerican Physical Soc-
dc.rights© 2013 American Physical Society-
dc.source.urihttp://dx.doi.org/10.1103/physrevlett.111.021103-
dc.subjectIceCube Collaboration-
dc.titleFirst observation of PeV-energy neutrinos with IceCube-
dc.typeJournal article-
dc.identifier.doi10.1103/PhysRevLett.111.021103-
dc.relation.grantARC-
pubs.publication-statusPublished-
Appears in Collections:Aurora harvest
Chemistry and Physics publications

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