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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Main Author: Spiering, Christian
Format: Report
Language:English
Published: Deutsches Elektronen-Synchrotron, DESY, Hamburg 2017
Subjects:
South Pole
South pole
Online Access:https://dx.doi.org/10.3204/pubdb-2018-01180
http://bib-pubdb1.desy.de/record/400212
id ftdatacite:10.3204/pubdb-2018-01180
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spelling 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
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language 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
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