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The first search for extremely-high energy cosmogenic neutrinos with the IceCube Neutrino Observatory
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arxiv 1009.1442 v1 pith:OVGXU4CF submitted 2010-09-08 astro-ph.CO astro-ph.HE
The first search for extremely-high energy cosmogenic neutrinos with the IceCube Neutrino Observatory
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We report on the results of the search for extremely-high energy (EHE) neutrinos with energies above $10^7$ GeV obtained with the partially ($\sim$30%) constructed IceCube in 2007. From the absence of signal events in the sample of 242.1 days of effective livetime, we derive a 90% C.L. model independent differential upper limit based on the number of signal events per energy decade at $E^2 \phi_{\nu_e+\nu_\mu+\nu_\tau}\simeq 1.4 \times 10^{-6}$ GeV cm$^{-2}$ sec$^{-1}$ sr$^{-1}$ for neutrinos in the energy range from $3\times10^7$ to $3\times10^9$ GeV.
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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.
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TeV-PeV Gamma-ray and Neutrino Emission in the Galactic Plane
astro-ph.HE 2026-06 unverdicted novelty 3.0
Alternative ISRF models produce only modest changes to the LHAASO diffuse gamma-ray fit; the associated pp neutrinos remain consistent with IceCube all-sky data and compatible with ANTARES/KM3NeT limits.
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