High-Energy Neutrino Astronomy: where do we stand, where do we go?
50 years Baksan Laboratory, Baksan, Russia, 22 Nov 2017 - 22 Nov 2017; 20 pp. (2017). : With the identification of a diffuse flux of astrophysical ('cosmic') neutrinos in the TeV-PeV energy range, IceCube has opened a new window to the Universe. However, the corresponding cosmic landscape...
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ftdatacite:10.3204/pubdb-2018-01180 2023-05-15T18:22:17+02:00 High-Energy Neutrino Astronomy: where do we stand, where do we go? Spiering, Christian 2017 https://dx.doi.org/10.3204/pubdb-2018-01180 http://bib-pubdb1.desy.de/record/400212 en eng Deutsches Elektronen-Synchrotron, DESY, Hamburg Text Report report ScholarlyArticle 2017 ftdatacite https://doi.org/10.3204/pubdb-2018-01180 2021-11-05T12:55:41Z 50 years Baksan Laboratory, Baksan, Russia, 22 Nov 2017 - 22 Nov 2017; 20 pp. (2017). : With the identification of a diffuse flux of astrophysical ('cosmic') neutrinos in the TeV-PeV energy range, IceCube has opened a new window to the Universe. However, the corresponding cosmic landscape is still uncharted: so far, the observed flux does not show any clear association with known source classes. In the present talk, I sketch the way from Baikal-NT200 to IceCube and summarize IceCube's recent astrophysics results. Finally, I describe the present projects to build even larger detectors: GVD in Lake Baikal, KM3NeT in the Mediterranean Sea and IceCube-Gen2 at the South Pole. These detectors will allow studying the high-energy neutrino sky in much more detail than the present arrays permit. Report South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole |
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English |
description |
50 years Baksan Laboratory, Baksan, Russia, 22 Nov 2017 - 22 Nov 2017; 20 pp. (2017). : With the identification of a diffuse flux of astrophysical ('cosmic') neutrinos in the TeV-PeV energy range, IceCube has opened a new window to the Universe. However, the corresponding cosmic landscape is still uncharted: so far, the observed flux does not show any clear association with known source classes. In the present talk, I sketch the way from Baikal-NT200 to IceCube and summarize IceCube's recent astrophysics results. Finally, I describe the present projects to build even larger detectors: GVD in Lake Baikal, KM3NeT in the Mediterranean Sea and IceCube-Gen2 at the South Pole. These detectors will allow studying the high-energy neutrino sky in much more detail than the present arrays permit. |
format |
Report |
author |
Spiering, Christian |
spellingShingle |
Spiering, Christian High-Energy Neutrino Astronomy: where do we stand, where do we go? |
author_facet |
Spiering, Christian |
author_sort |
Spiering, Christian |
title |
High-Energy Neutrino Astronomy: where do we stand, where do we go? |
title_short |
High-Energy Neutrino Astronomy: where do we stand, where do we go? |
title_full |
High-Energy Neutrino Astronomy: where do we stand, where do we go? |
title_fullStr |
High-Energy Neutrino Astronomy: where do we stand, where do we go? |
title_full_unstemmed |
High-Energy Neutrino Astronomy: where do we stand, where do we go? |
title_sort |
high-energy neutrino astronomy: where do we stand, where do we go? |
publisher |
Deutsches Elektronen-Synchrotron, DESY, Hamburg |
publishDate |
2017 |
url |
https://dx.doi.org/10.3204/pubdb-2018-01180 http://bib-pubdb1.desy.de/record/400212 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_doi |
https://doi.org/10.3204/pubdb-2018-01180 |
_version_ |
1766201668763910144 |