Atmospheric Neutrino Oscillations in IceCube DeepCore
The DeepCore sub-array within the IceCube Neutrino Observatory is a densely instrumented region of Antarctic ice designed to observe atmospheric neutrino interactions above 5 GeV, via Cherenkov radiation. At these energies, Earth-crossing muon neutrinos have a high chance of oscillating away to tau...
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ftzenodo:oai:zenodo.org:4124129 2024-09-15T17:44:00+00:00 Atmospheric Neutrino Oscillations in IceCube DeepCore Kayla Leonard 2020-07-01 https://doi.org/10.5281/zenodo.4124129 unknown Zenodo https://zenodo.org/communities/neutrino2020-posters https://doi.org/10.5281/zenodo.4124128 https://doi.org/10.5281/zenodo.4124129 oai:zenodo.org:4124129 info:eu-repo/semantics/openAccess Creative Commons Attribution 4.0 International https://creativecommons.org/licenses/by/4.0/legalcode Neutrino 2020, Online info:eu-repo/semantics/conferencePoster 2020 ftzenodo https://doi.org/10.5281/zenodo.412412910.5281/zenodo.4124128 2024-07-27T04:48:36Z The DeepCore sub-array within the IceCube Neutrino Observatory is a densely instrumented region of Antarctic ice designed to observe atmospheric neutrino interactions above 5 GeV, via Cherenkov radiation. At these energies, Earth-crossing muon neutrinos have a high chance of oscillating away to tau neutrinos. These oscillations have been previously observed in DeepCore through both muon neutrino disappearance and tau neutrino appearance channels. This poster will present the status of the IceCube Collaboration's newest analysis of the atmospheric neutrino oscillation parameters using 8 years of data. In addition to several more years of data, this analysis benefits from recent significant efforts in improving background rejection, reconstruction techniques, modeling of systematic uncertainties, particle identification, and much more. Conference Object Antarc* Antarctic Zenodo |
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The DeepCore sub-array within the IceCube Neutrino Observatory is a densely instrumented region of Antarctic ice designed to observe atmospheric neutrino interactions above 5 GeV, via Cherenkov radiation. At these energies, Earth-crossing muon neutrinos have a high chance of oscillating away to tau neutrinos. These oscillations have been previously observed in DeepCore through both muon neutrino disappearance and tau neutrino appearance channels. This poster will present the status of the IceCube Collaboration's newest analysis of the atmospheric neutrino oscillation parameters using 8 years of data. In addition to several more years of data, this analysis benefits from recent significant efforts in improving background rejection, reconstruction techniques, modeling of systematic uncertainties, particle identification, and much more. |
format |
Conference Object |
author |
Kayla Leonard |
spellingShingle |
Kayla Leonard Atmospheric Neutrino Oscillations in IceCube DeepCore |
author_facet |
Kayla Leonard |
author_sort |
Kayla Leonard |
title |
Atmospheric Neutrino Oscillations in IceCube DeepCore |
title_short |
Atmospheric Neutrino Oscillations in IceCube DeepCore |
title_full |
Atmospheric Neutrino Oscillations in IceCube DeepCore |
title_fullStr |
Atmospheric Neutrino Oscillations in IceCube DeepCore |
title_full_unstemmed |
Atmospheric Neutrino Oscillations in IceCube DeepCore |
title_sort |
atmospheric neutrino oscillations in icecube deepcore |
publisher |
Zenodo |
publishDate |
2020 |
url |
https://doi.org/10.5281/zenodo.4124129 |
genre |
Antarc* Antarctic |
genre_facet |
Antarc* Antarctic |
op_source |
Neutrino 2020, Online |
op_relation |
https://zenodo.org/communities/neutrino2020-posters https://doi.org/10.5281/zenodo.4124128 https://doi.org/10.5281/zenodo.4124129 oai:zenodo.org:4124129 |
op_rights |
info:eu-repo/semantics/openAccess Creative Commons Attribution 4.0 International https://creativecommons.org/licenses/by/4.0/legalcode |
op_doi |
https://doi.org/10.5281/zenodo.412412910.5281/zenodo.4124128 |
_version_ |
1810491283173539840 |