Results 131 to 140 of about 28,160 (279)
Nuclear Physics B - Proceedings Supplements, 2009 The IceCube detector allows for the first time a measurement of atmospheric muon and neutrino energy spectra from tens of GeV up to the PeV range. The lepton flux in the highest energy region depends on both the primary cosmic ray composition around the "knee" and the contribution from prompt decays of mostly charmed hadrons produced in air showers. It
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Prospects for Observing Astrophysical Transients with Gigaelectronvolt Neutrinos
The Astrophysical JournalAlthough Cherenkov detectors of high-energy neutrinos in ice and water are often optimized to detect teraelectronvolt–petaelectronvolt neutrinos, they may also be sensitive to transient neutrino sources in the 1–100 GeV energy range.
Angelina Sherman +4 more
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Probing particle physics with IceCube
European Physical Journal C: Particles and Fields, 2018 The IceCube observatory located at the South Pole is a cubic-kilometre optical Cherenkov telescope primarily designed for the detection of high-energy astrophysical neutrinos.
Markus Ahlers +2 more
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Are both BL Lacs and pulsar wind nebulae the astrophysical counterparts of IceCube neutrino events?
, 2014 IceCube has recently reported the discovery of high-energy neutrinos of astrophysical origin, opening up the PeV (10^15 eV) sky. Because of their large positional uncertainties, these events have not yet been associated to any astrophysical source.
Padovani, P., Resconi, E.
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No Black Holes at IceCube [PDF]
, 2006 10 pages, 5 figures, submitted to Journal of Cosmology and Astroparticle ...
Harbach, Ulrich, Bleicher, Marcus
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A test of spatial coincidence between CHIME FRBs and IceCube TeV energy neutrinos [PDF]
, 2021 S. Desai
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Journal of Physics: Conference Series, 2013 4 pages, 2 figures, from a talk given at NUFACT 11, the XIIIth Intl. Workshop on Neutrino Factories, Super beams and Beta beams, 1-6 August 2011 at CERN and the University of Geneva ...
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Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019), 2019 The IceCube Neutrino Observatory is the world's largest neutrino detector, instrumenting a cubic kilometer of ice at the geographic South Pole. The detector probes neutrino energies from GeV to PeV, and collects high statistics neutrino samples by virtue of its extremely large volume.
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EPJ Web of Conferences, 2016 The last IceCube catalog of High Energy Starting Events (HESE) obtained with a livetime of 1347 days comprises 54 neutrino events equally-distributed between the three families with energies between 25 TeV and few PeVs.
Marinelli Antonio +4 more
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The IceCube Realtime Alert System [PDF]
, 2017 Although high-energy astrophysical neutrinos were discovered in 2013, their origin is still unknown. Aiming for the identification of an electromagnetic counterpart of a rapidly fading source, we have implemented a realtime analysis framework for the ...
Andeen, Karen, IceCube Collaboration
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