Next generation neutrino detectors at the South Pole
Since the construction of IceCube was completed in 2010/11, the observatory has delivered several outstanding measurements in neutrino physics and multimessenger astronomy. Additionally, a series of new scientific questions and opportunities appeared. To address these, plans have been developed to e...
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ftdoajarticles:oai:doaj.org/article:ed74935a5394455d8210b8ff05878190 2023-05-15T18:22:01+02:00 Next generation neutrino detectors at the South Pole Kowalski Marek 2019-01-01T00:00:00Z https://doi.org/10.1051/epjconf/201920701005 https://doaj.org/article/ed74935a5394455d8210b8ff05878190 EN eng EDP Sciences https://www.epj-conferences.org/articles/epjconf/pdf/2019/12/epjconf_vlvnt2018_01005.pdf https://doaj.org/toc/2100-014X 2100-014X doi:10.1051/epjconf/201920701005 https://doaj.org/article/ed74935a5394455d8210b8ff05878190 EPJ Web of Conferences, Vol 207, p 01005 (2019) Physics QC1-999 article 2019 ftdoajarticles https://doi.org/10.1051/epjconf/201920701005 2022-12-31T15:28:19Z Since the construction of IceCube was completed in 2010/11, the observatory has delivered several outstanding measurements in neutrino physics and multimessenger astronomy. Additionally, a series of new scientific questions and opportunities appeared. To address these, plans have been developed to expand on the IceCube concept, targeting both lower and higher energies, as well as the central PeV-energy window at significantly improved sensitivity. In this contribution I will outline these plans. Article in Journal/Newspaper South pole Directory of Open Access Journals: DOAJ Articles South Pole EPJ Web of Conferences 207 01005 |
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Directory of Open Access Journals: DOAJ Articles |
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ftdoajarticles |
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English |
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Physics QC1-999 |
spellingShingle |
Physics QC1-999 Kowalski Marek Next generation neutrino detectors at the South Pole |
topic_facet |
Physics QC1-999 |
description |
Since the construction of IceCube was completed in 2010/11, the observatory has delivered several outstanding measurements in neutrino physics and multimessenger astronomy. Additionally, a series of new scientific questions and opportunities appeared. To address these, plans have been developed to expand on the IceCube concept, targeting both lower and higher energies, as well as the central PeV-energy window at significantly improved sensitivity. In this contribution I will outline these plans. |
format |
Article in Journal/Newspaper |
author |
Kowalski Marek |
author_facet |
Kowalski Marek |
author_sort |
Kowalski Marek |
title |
Next generation neutrino detectors at the South Pole |
title_short |
Next generation neutrino detectors at the South Pole |
title_full |
Next generation neutrino detectors at the South Pole |
title_fullStr |
Next generation neutrino detectors at the South Pole |
title_full_unstemmed |
Next generation neutrino detectors at the South Pole |
title_sort |
next generation neutrino detectors at the south pole |
publisher |
EDP Sciences |
publishDate |
2019 |
url |
https://doi.org/10.1051/epjconf/201920701005 https://doaj.org/article/ed74935a5394455d8210b8ff05878190 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_source |
EPJ Web of Conferences, Vol 207, p 01005 (2019) |
op_relation |
https://www.epj-conferences.org/articles/epjconf/pdf/2019/12/epjconf_vlvnt2018_01005.pdf https://doaj.org/toc/2100-014X 2100-014X doi:10.1051/epjconf/201920701005 https://doaj.org/article/ed74935a5394455d8210b8ff05878190 |
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https://doi.org/10.1051/epjconf/201920701005 |
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EPJ Web of Conferences |
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207 |
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01005 |
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