Recent Results from the AMANDA Experiment
AMANDA (Antarctic Muon And Neutrino Detector Array) is a neutrino telescope built under the southern polar icecap and its scope is to explore the possibility to detect high energy cosmic neutrinos. This should generate insight into the powerful celestial objects where acceleration mechanisms can bri...
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ftdatacite:10.48550/arxiv.astro-ph/0306209 2023-05-15T13:34:03+02:00 Recent Results from the AMANDA Experiment Niessen, Peter 2003 https://dx.doi.org/10.48550/arxiv.astro-ph/0306209 https://arxiv.org/abs/astro-ph/0306209 unknown arXiv Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004 http://arxiv.org/licenses/assumed-1991-2003/ Astrophysics astro-ph FOS Physical sciences Preprint Article article CreativeWork 2003 ftdatacite https://doi.org/10.48550/arxiv.astro-ph/0306209 2022-04-01T16:33:39Z AMANDA (Antarctic Muon And Neutrino Detector Array) is a neutrino telescope built under the southern polar icecap and its scope is to explore the possibility to detect high energy cosmic neutrinos. This should generate insight into the powerful celestial objects where acceleration mechanisms can bring up to $10^{20}$ eV. We describe the achievements and results from the AMANDA-B10 prototype and the preliminary results from the current AMANDA-II detector which show dramatic increase in sensitivity. : to appear in the proceedings of the 38th Rencontres of Moriond (Electroweak Interactions and Unified Theories) - 2003 Report Antarc* Antarctic DataCite Metadata Store (German National Library of Science and Technology) Antarctic |
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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 Niessen, Peter Recent Results from the AMANDA Experiment |
topic_facet |
Astrophysics astro-ph FOS Physical sciences |
description |
AMANDA (Antarctic Muon And Neutrino Detector Array) is a neutrino telescope built under the southern polar icecap and its scope is to explore the possibility to detect high energy cosmic neutrinos. This should generate insight into the powerful celestial objects where acceleration mechanisms can bring up to $10^{20}$ eV. We describe the achievements and results from the AMANDA-B10 prototype and the preliminary results from the current AMANDA-II detector which show dramatic increase in sensitivity. : to appear in the proceedings of the 38th Rencontres of Moriond (Electroweak Interactions and Unified Theories) - 2003 |
format |
Report |
author |
Niessen, Peter |
author_facet |
Niessen, Peter |
author_sort |
Niessen, Peter |
title |
Recent Results from the AMANDA Experiment |
title_short |
Recent Results from the AMANDA Experiment |
title_full |
Recent Results from the AMANDA Experiment |
title_fullStr |
Recent Results from the AMANDA Experiment |
title_full_unstemmed |
Recent Results from the AMANDA Experiment |
title_sort |
recent results from the amanda experiment |
publisher |
arXiv |
publishDate |
2003 |
url |
https://dx.doi.org/10.48550/arxiv.astro-ph/0306209 https://arxiv.org/abs/astro-ph/0306209 |
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Antarctic |
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Antarctic |
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Antarc* Antarctic |
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Antarc* Antarctic |
op_rights |
Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004 http://arxiv.org/licenses/assumed-1991-2003/ |
op_doi |
https://doi.org/10.48550/arxiv.astro-ph/0306209 |
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1766048516015128576 |