Measurement of Neutrino Oscillations with Neutrino Telescopes

IceCube and ANTARES are the world-largest neutrino telescopes. They are successfully taking data, producing a wealth of scientific results. Whereas their main goal is the detection of cosmic neutrinos with energies in the TeV-PeV range, both have demonstrated their capability to measure neutrino osc...

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Main Author: Jürgen Brunner
Format: Article
Language:English
Published: Wiley 2013-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2013/782538
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author Jürgen Brunner
author_facet Jürgen Brunner
author_sort Jürgen Brunner
collection DOAJ
description IceCube and ANTARES are the world-largest neutrino telescopes. They are successfully taking data, producing a wealth of scientific results. Whereas their main goal is the detection of cosmic neutrinos with energies in the TeV-PeV range, both have demonstrated their capability to measure neutrino oscillations by studying atmospheric neutrinos with energies of 10–50 GeV. After recalling the methods of these measurements and the first published results of these searches, the potential of existing, and planned low-energy extensions of IceCube and KM3Net are discussed. These new detectors will be able to improve the knowledge of the atmospheric neutrino oscillation parameters, and in particular they might help to understand the neutrino mass hierarchy. Such studies, which use atmospheric neutrinos, could be complemented by measurements in a long-baseline neutrino beam, which is discussed as a long-term future option.
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spelling doaj-art-1fdccd7fbdb14ce7b9a8d3613b4d1a682025-08-20T02:03:47ZengWileyAdvances in High Energy Physics1687-73571687-73652013-01-01201310.1155/2013/782538782538Measurement of Neutrino Oscillations with Neutrino TelescopesJürgen Brunner0CPPM, Aix-Marseille Université, CNRS/IN2P3, Marseille, FranceIceCube and ANTARES are the world-largest neutrino telescopes. They are successfully taking data, producing a wealth of scientific results. Whereas their main goal is the detection of cosmic neutrinos with energies in the TeV-PeV range, both have demonstrated their capability to measure neutrino oscillations by studying atmospheric neutrinos with energies of 10–50 GeV. After recalling the methods of these measurements and the first published results of these searches, the potential of existing, and planned low-energy extensions of IceCube and KM3Net are discussed. These new detectors will be able to improve the knowledge of the atmospheric neutrino oscillation parameters, and in particular they might help to understand the neutrino mass hierarchy. Such studies, which use atmospheric neutrinos, could be complemented by measurements in a long-baseline neutrino beam, which is discussed as a long-term future option.http://dx.doi.org/10.1155/2013/782538
spellingShingle Jürgen Brunner
Measurement of Neutrino Oscillations with Neutrino Telescopes
Advances in High Energy Physics
title Measurement of Neutrino Oscillations with Neutrino Telescopes
title_full Measurement of Neutrino Oscillations with Neutrino Telescopes
title_fullStr Measurement of Neutrino Oscillations with Neutrino Telescopes
title_full_unstemmed Measurement of Neutrino Oscillations with Neutrino Telescopes
title_short Measurement of Neutrino Oscillations with Neutrino Telescopes
title_sort measurement of neutrino oscillations with neutrino telescopes
url http://dx.doi.org/10.1155/2013/782538
work_keys_str_mv AT jurgenbrunner measurementofneutrinooscillationswithneutrinotelescopes