IceCube: physics, status, and future

The IceCube observatory is the first cubic kilometre scale instrument in the field of high-energy neutrino astronomy and cosmic rays. In 2009, following five successful deployment seasons, IceCube consisted of 59 strings of optical modules in the South Pole ice, together with 118 air shower detector...

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Main Author: Hultqvist, Klas
Format: Text
Language:unknown
Published: arXiv 2010
Subjects:
High Energy Astrophysical Phenomena astro-ph.HE
FOS Physical sciences
South Pole
South pole
Online Access:https://dx.doi.org/10.48550/arxiv.1003.2300
https://arxiv.org/abs/1003.2300
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spelling ftdatacite:10.48550/arxiv.1003.2300 2023-05-15T18:22:11+02:00 IceCube: physics, status, and future Hultqvist, Klas 2010 https://dx.doi.org/10.48550/arxiv.1003.2300 https://arxiv.org/abs/1003.2300 unknown arXiv https://dx.doi.org/10.1016/j.nima.2010.05.014 arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences article-journal Article ScholarlyArticle Text 2010 ftdatacite https://doi.org/10.48550/arxiv.1003.2300 https://doi.org/10.1016/j.nima.2010.05.014 2022-04-01T14:49:41Z The IceCube observatory is the first cubic kilometre scale instrument in the field of high-energy neutrino astronomy and cosmic rays. In 2009, following five successful deployment seasons, IceCube consisted of 59 strings of optical modules in the South Pole ice, together with 118 air shower detectors in the IceTop surface array. The range of physics topics includes neutrino signals from astrophysical sources, dark matter, exotic particle physics, cosmic rays, and atmospheric neutrinos. The current IceCube status and selected results are described. Anticipated future developments are also discussed, in particular the Deep Core low energy subarray which was recently deployed. : Presentation at the 4th International Workshop on Very Large Volume Neutrino Telescopes Text South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language unknown
topic High Energy Astrophysical Phenomena astro-ph.HE
FOS Physical sciences
spellingShingle High Energy Astrophysical Phenomena astro-ph.HE
FOS Physical sciences
Hultqvist, Klas
IceCube: physics, status, and future
topic_facet High Energy Astrophysical Phenomena astro-ph.HE
FOS Physical sciences
description The IceCube observatory is the first cubic kilometre scale instrument in the field of high-energy neutrino astronomy and cosmic rays. In 2009, following five successful deployment seasons, IceCube consisted of 59 strings of optical modules in the South Pole ice, together with 118 air shower detectors in the IceTop surface array. The range of physics topics includes neutrino signals from astrophysical sources, dark matter, exotic particle physics, cosmic rays, and atmospheric neutrinos. The current IceCube status and selected results are described. Anticipated future developments are also discussed, in particular the Deep Core low energy subarray which was recently deployed. : Presentation at the 4th International Workshop on Very Large Volume Neutrino Telescopes
format Text
author Hultqvist, Klas
author_facet Hultqvist, Klas
author_sort Hultqvist, Klas
title IceCube: physics, status, and future
title_short IceCube: physics, status, and future
title_full IceCube: physics, status, and future
title_fullStr IceCube: physics, status, and future
title_full_unstemmed IceCube: physics, status, and future
title_sort icecube: physics, status, and future
publisher arXiv
publishDate 2010
url https://dx.doi.org/10.48550/arxiv.1003.2300
https://arxiv.org/abs/1003.2300
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_relation https://dx.doi.org/10.1016/j.nima.2010.05.014
op_rights arXiv.org perpetual, non-exclusive license
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
op_doi https://doi.org/10.48550/arxiv.1003.2300
https://doi.org/10.1016/j.nima.2010.05.014
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