High-Energy Neutrino Astronomy: where do we stand, where do we go?

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 k...

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Main Author: Spiering, Christian
Format: Text
Language:unknown
Published: arXiv 2017
Subjects:
High Energy Astrophysical Phenomena astro-ph.HE
FOS Physical sciences
South Pole
South pole
Online Access:https://dx.doi.org/10.48550/arxiv.1711.08266
https://arxiv.org/abs/1711.08266
id ftdatacite:10.48550/arxiv.1711.08266
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spelling ftdatacite:10.48550/arxiv.1711.08266 2023-05-15T18:22:20+02:00 High-Energy Neutrino Astronomy: where do we stand, where do we go? Spiering, Christian 2017 https://dx.doi.org/10.48550/arxiv.1711.08266 https://arxiv.org/abs/1711.08266 unknown arXiv https://dx.doi.org/10.1134/s1063779618040536 arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences article-journal Article ScholarlyArticle Text 2017 ftdatacite https://doi.org/10.48550/arxiv.1711.08266 https://doi.org/10.1134/s1063779618040536 2022-04-01T10:18:46Z 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. : Talk given at the occasion of the 50th anniversary of the Baksan Laboratory Text 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 unknown
topic High Energy Astrophysical Phenomena astro-ph.HE
FOS Physical sciences
spellingShingle High Energy Astrophysical Phenomena astro-ph.HE
FOS Physical sciences
Spiering, Christian
High-Energy Neutrino Astronomy: where do we stand, where do we go?
topic_facet High Energy Astrophysical Phenomena astro-ph.HE
FOS Physical sciences
description 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. : Talk given at the occasion of the 50th anniversary of the Baksan Laboratory
format Text
author Spiering, Christian
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 arXiv
publishDate 2017
url https://dx.doi.org/10.48550/arxiv.1711.08266
https://arxiv.org/abs/1711.08266
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_relation https://dx.doi.org/10.1134/s1063779618040536
op_rights arXiv.org perpetual, non-exclusive license
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
op_doi https://doi.org/10.48550/arxiv.1711.08266
https://doi.org/10.1134/s1063779618040536
_version_ 1766201740579831808

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