Search for ultra-high-energy neutrinos with AMANDA-11

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dc.contributor.authorAckermann, M.
dc.contributor.authorHill, G.
dc.date.issued2008
dc.description.abstractA search for diffuse neutrinos with energies in excess of 10⁵ GeV is conducted with AMANDA-II data recorded between 2000 and 2002. Above 10⁷ GeV, the Earth is essentially opaque to neutrinos. This fact, combined with the limited overburden of the AMANDA-II detector (roughly 1.5 km), concentrates these ultra-high-energy neutrinos at the horizon. The primary background for this analysis is bundles of downgoing, high-energy muons from the interaction of cosmic rays in the atmosphere. No statistically significant excess above the expected background is seen in the data, and an upper limit is set on the diffuse all-flavor neutrino flux of E²Φ₉₀% (sub)CL < 2.7 × 10⁻⁷ GeV cm⁻² s⁻¹ sr⁻¹ valid over the energy range of 2 × 10⁵ to 10⁹ GeV. A number of models that predict neutrino fluxes from active galactic nuclei are excluded at the 90% confidence level.
dc.description.statementofresponsibilityM. Ackermann ... G. C. Hill ... et al. (IceCube Collaboration)
dc.identifier.citationLetters of the Astrophysical Journal, 2008; 675(2):1014-1024
dc.identifier.doi10.1086/527046
dc.identifier.issn2041-8205
dc.identifier.issn1538-4357
dc.identifier.urihttp://hdl.handle.net/2440/76781
dc.language.isoen
dc.publisherInstitute of Physics Publishing Ltd.
dc.rights© 2008. The American Astronomical Society. All rights reserved.
dc.source.urihttps://doi.org/10.1086/527046
dc.titleSearch for ultra-high-energy neutrinos with AMANDA-11
dc.typeJournal article
pubs.publication-statusPublished

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