High Energy Neutrino Astronomy: Status and Perspectives
The year 2008 has witnessed remarkable steps in developing high energy neutrino telescopes. IceCube at the South Pole has been deployed with 40 of its planned 80 strings and reached half a cubic kilometer instrumented volume, in the Mediterranean Sea the "first-stage" neutrino telescope AN...
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ftdatacite:10.48550/arxiv.0811.4747 2023-05-15T18:22:22+02:00 High Energy Neutrino Astronomy: Status and Perspectives Spiering, Christian 2008 https://dx.doi.org/10.48550/arxiv.0811.4747 https://arxiv.org/abs/0811.4747 unknown arXiv https://dx.doi.org/10.1063/1.3076635 arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ Astrophysics astro-ph FOS Physical sciences article-journal Article ScholarlyArticle Text 2008 ftdatacite https://doi.org/10.48550/arxiv.0811.4747 https://doi.org/10.1063/1.3076635 2022-04-01T15:06:39Z The year 2008 has witnessed remarkable steps in developing high energy neutrino telescopes. IceCube at the South Pole has been deployed with 40 of its planned 80 strings and reached half a cubic kilometer instrumented volume, in the Mediterranean Sea the "first-stage" neutrino telescope ANTARES has been completed and takes data with 12 strings. The next years will be key years for opening the neutrino window to the high energy universe. IceCube is presently entering a region with realistic discovery potential. Early discoveries (or non-discoveries) with IceCube will strongly influence the design and the estimated discovery chances of the Northern equivalent KM3NeT. Following theoretical estimates, cubic kilometer telescopes may just scratch the regions of discovery. Therefore detectors presently planned should reach sensitivities substantially beyond those of IceCube. : Invited Talk, International Symposium on High Energy Gamma-Ray Astronomy, Heidelberg, July 2008, 12 pages, 11 figures Text South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole |
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DataCite Metadata Store (German National Library of Science and Technology) |
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Astrophysics astro-ph FOS Physical sciences |
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Astrophysics astro-ph FOS Physical sciences Spiering, Christian High Energy Neutrino Astronomy: Status and Perspectives |
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Astrophysics astro-ph FOS Physical sciences |
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The year 2008 has witnessed remarkable steps in developing high energy neutrino telescopes. IceCube at the South Pole has been deployed with 40 of its planned 80 strings and reached half a cubic kilometer instrumented volume, in the Mediterranean Sea the "first-stage" neutrino telescope ANTARES has been completed and takes data with 12 strings. The next years will be key years for opening the neutrino window to the high energy universe. IceCube is presently entering a region with realistic discovery potential. Early discoveries (or non-discoveries) with IceCube will strongly influence the design and the estimated discovery chances of the Northern equivalent KM3NeT. Following theoretical estimates, cubic kilometer telescopes may just scratch the regions of discovery. Therefore detectors presently planned should reach sensitivities substantially beyond those of IceCube. : Invited Talk, International Symposium on High Energy Gamma-Ray Astronomy, Heidelberg, July 2008, 12 pages, 11 figures |
format |
Text |
author |
Spiering, Christian |
author_facet |
Spiering, Christian |
author_sort |
Spiering, Christian |
title |
High Energy Neutrino Astronomy: Status and Perspectives |
title_short |
High Energy Neutrino Astronomy: Status and Perspectives |
title_full |
High Energy Neutrino Astronomy: Status and Perspectives |
title_fullStr |
High Energy Neutrino Astronomy: Status and Perspectives |
title_full_unstemmed |
High Energy Neutrino Astronomy: Status and Perspectives |
title_sort |
high energy neutrino astronomy: status and perspectives |
publisher |
arXiv |
publishDate |
2008 |
url |
https://dx.doi.org/10.48550/arxiv.0811.4747 https://arxiv.org/abs/0811.4747 |
geographic |
South Pole |
geographic_facet |
South Pole |
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South pole |
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South pole |
op_relation |
https://dx.doi.org/10.1063/1.3076635 |
op_rights |
arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
op_doi |
https://doi.org/10.48550/arxiv.0811.4747 https://doi.org/10.1063/1.3076635 |
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1766201774361804800 |