Submitted to Astroparticle Physics
Necessary technical experience is being gained from successful construction and deployment of current prototype detectors to search for UHE neutrinos in Antarctica, Lake Baikal in Russia, and the Mediterranean. The prototype detectors have also the important central purpose of determining whether or...
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ftciteseerx:oai:CiteSeerX.psu:10.1.1.258.1888 2023-05-15T13:57:47+02:00 Submitted to Astroparticle Physics Joshua R. Klein The Pennsylvania State University CiteSeerX Archives 1998 application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.258.1888 http://arxiv.org/pdf/astro-ph/9806152v1.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.258.1888 http://arxiv.org/pdf/astro-ph/9806152v1.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://arxiv.org/pdf/astro-ph/9806152v1.pdf text 1998 ftciteseerx 2016-01-07T20:02:22Z Necessary technical experience is being gained from successful construction and deployment of current prototype detectors to search for UHE neutrinos in Antarctica, Lake Baikal in Russia, and the Mediterranean. The prototype detectors have also the important central purpose of determining whether or not UHE neutrinos do in fact exist in nature by observation of at least a few UHE neutrino-induced leptons with properties that are not consistent with expected backgrounds. We discuss here the criteria for a prototype detector to accomplish that purpose in a convincing way even if the UHE neutrino flux is substantially lower than predicted at present. Text Antarc* Antarctica Unknown |
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ftciteseerx |
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English |
| description |
Necessary technical experience is being gained from successful construction and deployment of current prototype detectors to search for UHE neutrinos in Antarctica, Lake Baikal in Russia, and the Mediterranean. The prototype detectors have also the important central purpose of determining whether or not UHE neutrinos do in fact exist in nature by observation of at least a few UHE neutrino-induced leptons with properties that are not consistent with expected backgrounds. We discuss here the criteria for a prototype detector to accomplish that purpose in a convincing way even if the UHE neutrino flux is substantially lower than predicted at present. |
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The Pennsylvania State University CiteSeerX Archives |
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Text |
| author |
Joshua R. Klein |
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Joshua R. Klein Submitted to Astroparticle Physics |
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Joshua R. Klein |
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Joshua R. Klein |
| title |
Submitted to Astroparticle Physics |
| title_short |
Submitted to Astroparticle Physics |
| title_full |
Submitted to Astroparticle Physics |
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Submitted to Astroparticle Physics |
| title_full_unstemmed |
Submitted to Astroparticle Physics |
| title_sort |
submitted to astroparticle physics |
| publishDate |
1998 |
| url |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.258.1888 http://arxiv.org/pdf/astro-ph/9806152v1.pdf |
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Antarc* Antarctica |
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Antarc* Antarctica |
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http://arxiv.org/pdf/astro-ph/9806152v1.pdf |
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http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.258.1888 http://arxiv.org/pdf/astro-ph/9806152v1.pdf |
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Metadata may be used without restrictions as long as the oai identifier remains attached to it. |
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