New Measurement Of The Flavor Composition Of High-Energy Neutrino Events With Contained Vertices In Icecube
The IceCube Neutrino Observatory at the South Pole detects Cherenkov light from charged particles produced in neutrino interactions. At the highest energies, the neutrino flux is of cosmic origin, but its astrophysical sources are yet unknown. A measurement of the flavor ratio on Earth can provide i...
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ftdatacite:10.5281/zenodo.1301121 2023-05-15T18:22:16+02:00 New Measurement Of The Flavor Composition Of High-Energy Neutrino Events With Contained Vertices In Icecube STACHURSKA, Juliana 2018 https://dx.doi.org/10.5281/zenodo.1301121 https://zenodo.org/record/1301121 unknown Zenodo https://dx.doi.org/10.5281/zenodo.1301122 Open Access Creative Commons Attribution 4.0 https://creativecommons.org/licenses/by/4.0 info:eu-repo/semantics/openAccess CC-BY Text Poster article-journal ScholarlyArticle 2018 ftdatacite https://doi.org/10.5281/zenodo.1301121 https://doi.org/10.5281/zenodo.1301122 2021-11-05T12:55:41Z The IceCube Neutrino Observatory at the South Pole detects Cherenkov light from charged particles produced in neutrino interactions. At the highest energies, the neutrino flux is of cosmic origin, but its astrophysical sources are yet unknown. A measurement of the flavor ratio on Earth can provide important constraints on sources and production mechanisms. In this poster we present the measurement of the flavor composition performed on IceCube's High-Energy Starting Event (HESE) sample with a livetime of 7 years. We are directly sensitive to each neutrino flavor via the single cascade, track and double cascade event topologies, the latter being the topology only produced in tau-neutrino interactions above an energy threshold of ~100 TeV. Still Image South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole |
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The IceCube Neutrino Observatory at the South Pole detects Cherenkov light from charged particles produced in neutrino interactions. At the highest energies, the neutrino flux is of cosmic origin, but its astrophysical sources are yet unknown. A measurement of the flavor ratio on Earth can provide important constraints on sources and production mechanisms. In this poster we present the measurement of the flavor composition performed on IceCube's High-Energy Starting Event (HESE) sample with a livetime of 7 years. We are directly sensitive to each neutrino flavor via the single cascade, track and double cascade event topologies, the latter being the topology only produced in tau-neutrino interactions above an energy threshold of ~100 TeV. |
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Still Image |
author |
STACHURSKA, Juliana |
spellingShingle |
STACHURSKA, Juliana New Measurement Of The Flavor Composition Of High-Energy Neutrino Events With Contained Vertices In Icecube |
author_facet |
STACHURSKA, Juliana |
author_sort |
STACHURSKA, Juliana |
title |
New Measurement Of The Flavor Composition Of High-Energy Neutrino Events With Contained Vertices In Icecube |
title_short |
New Measurement Of The Flavor Composition Of High-Energy Neutrino Events With Contained Vertices In Icecube |
title_full |
New Measurement Of The Flavor Composition Of High-Energy Neutrino Events With Contained Vertices In Icecube |
title_fullStr |
New Measurement Of The Flavor Composition Of High-Energy Neutrino Events With Contained Vertices In Icecube |
title_full_unstemmed |
New Measurement Of The Flavor Composition Of High-Energy Neutrino Events With Contained Vertices In Icecube |
title_sort |
new measurement of the flavor composition of high-energy neutrino events with contained vertices in icecube |
publisher |
Zenodo |
publishDate |
2018 |
url |
https://dx.doi.org/10.5281/zenodo.1301121 https://zenodo.org/record/1301121 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_relation |
https://dx.doi.org/10.5281/zenodo.1301122 |
op_rights |
Open Access Creative Commons Attribution 4.0 https://creativecommons.org/licenses/by/4.0 info:eu-repo/semantics/openAccess |
op_rightsnorm |
CC-BY |
op_doi |
https://doi.org/10.5281/zenodo.1301121 https://doi.org/10.5281/zenodo.1301122 |
_version_ |
1766201650452627456 |