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dc.contributor.authorAartsen, M. G.
dc.contributor.authorBesson, David Zeke
dc.contributor.authorIceCube Collaboration
dc.date.accessioned2014-11-21T17:44:51Z
dc.date.available2014-11-21T17:44:51Z
dc.date.issued2013-07-08
dc.identifier.citationAartsen et al. (IceCube Collaboration) "First Observation of PeV-Energy Neutrinos with IceCube." Phys. Rev. Lett. 111, 021103 – Published 8 July 2013 http://dx.doi.org/10.1103/PhysRevLett.111.021103
dc.identifier.urihttp://hdl.handle.net/1808/15830
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 νe,μ,τ (ν¯e,μ,τ) or charged-current νe (ν¯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)+0.041−0.057(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.sponsorshipWe acknowledge the support from the following agencies: U.S. National Science Foundation-Office of Polar Programs, U.S. National Science Foundation-Physics Division, University of Wisconsin Alumni Research Foundation, the Grid Laboratory Of Wisconsin (GLOW) grid infrastructure at the University of Wisconsin—Madison, the Open Science Grid (OSG) grid infrastructure; U.S. Department of Energy, and National Energy Research Scientific Computing Center, the Louisiana Optical Network Initiative (LONI) grid computing resources; Natural Sciences and Engineering Research Council of Canada, Compute Canada, and Compute West High Performance Computing; Swedish Research Council, Swedish Polar Research Secretariat, Swedish National Infrastructure for Computing (SNIC), and Knut and Alice Wallenberg Foundation, Sweden; German Ministry for Education and Research (BMBF), Deutsche Forschungsgemeinschaft (DFG), Helmholtz Alliance for Astroparticle Physics (HAP), Research Department of Plasmas with Complex Interactions (Bochum), Germany; Fund for Scientific Research (FNRS-FWO), FWO Odysseus programme, Flanders Institute to encourage scientific and technological research in industry (IWT), Belgian Federal Science Policy Office (Belspo); University of Oxford, United Kingdom; Marsden Fund, New Zealand; Australian Research Council; Japan Society for Promotion of Science (JSPS); the Swiss National Science Foundation (SNSF), Switzerland.
dc.publisherAmerican Physical Society
dc.titleFirst Observation of PeV-Energy Neutrinos with IceCube
dc.typeArticle
kusw.kuauthorBesson, David Zeke
kusw.kudepartmentDepartment of Physics and Astronomy
kusw.oastatusfullparticipation
dc.identifier.doi10.1103/PhysRevLett.111.021103
kusw.oaversionScholarly/refereed, publisher version
kusw.oapolicyThis item meets KU Open Access policy criteria.
dc.rights.accessrightsopenAccess


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