Results 91 to 100 of about 22,516 (235)
Realtime Follow-up of Astrophysical Transients with the IceCube Neutrino\n Observatory [PDF]
, 2021 A. Pizzuto +2 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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Do high energy astrophysical neutrinos trace star formation?
, 2015 The IceCube Neutrino Observatory has provided the first map of the high energy (~ 0.01 -- 1 PeV) sky in neutrinos. Since neutrinos propagate undeflected, their arrival direction is an important identifier for sources of high energy particle acceleration.
Emig, Kimberly +2 more
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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
openaire +2 more sources
, 2010 A search for extremely high energy cosmic neutrinos has been carried out with the IceCube Neutrino Observatory. The main signals in the search are neutrino-induced energetic charged leptons and their rate depends on the neutrino-nucleon cross section ...
Yoshida, Shigeru
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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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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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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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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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