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, 2021 The observation of electromagnetic radiation from radio to $\gamma$-ray wavelengths has provided a wealth of information about the universe. However, at PeV (10$^{15}$ eV) energies and above, most of the universe is impenetrable to photons. New messengers, namely cosmic neutrinos, are needed to explore the most extreme environments of the universe ...
, IceCube-Gen2 Collaboration +9 more
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EPJ Web of Conferences, 2013 IceCube and ANTARES are neutrino detectors sensitive to energies from 20 GeV up to PeV. Both detectors have been completed and take data. Several years of data have been already analysed including periods with the partly assembled detectors. The primary goal of these two neutrino telescopes is the observation of astrophysical sources of neutrinos ...
openaire +2 more sources
IceCube sensitivity for low-energy neutrinos from nearby supernovae (Corrigendum) [PDF]
, 2014 A correction to "IceCube sensitivity for low-energy neutrinos from nearby supernovae" Volume 535, Article 109 (2011) [10.1051/0004-6361/201117810]
IceCube Collaboration
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This is the home page for IceCube, a one-cubic-kilometer international high-energy neutrino observatory being built and installed in the clear deep ice below the South Pole Station.
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Search for a Diffuse Flux of Astrophysical Muon Neutrinos with the IceCube 40-String Detector [PDF]
, 2011 The IceCube Neutrino Observatory is a 1 km(3) detector currently taking data at the South Pole. One of the main strategies used to look for astrophysical neutrinos with IceCube is the search for a diffuse flux of high-energy neutrinos from unresolved ...
Bohm, Christian, +8 more
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All-flavour search for neutrinos from dark matter annihilations in the Milky Way with IceCube/DeepCore [PDF]
, 2016 We present the first IceCube search for a signal of dark matter annihilations in the Milky Way using all-flavour neutrino-induced particle cascades. The analysis focuses on the DeepCore sub-detector of IceCube, and uses the surrounding IceCube strings as
IceCube Collaboration
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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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Early decay of Peccei–Quinn fermion and the IceCube neutrino events
Physics Letters B, 2016 IceCube observed high-energy neutrino flux in the energy region from TeV to PeV. The decay of a massive long-lived particle in the early universe can be the origin of the IceCube neutrino events, which we call an “early decay scenario.” In this paper, we
Yohei Ema, Takeo Moroi
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IceCube searches for neutrino emission from galactic and extragalactic sources
EPJ Web of Conferences, 2015 The IceCube Neutrino Observatory, located near the geographic South Pole, is currently the world’s largest neutrino telescope. IceCube is principally designed to detect high-energy neutrinos from galactic and extragalactic sources. The detector comprises
Palczewski Tomasz Jan
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