Leading NSI constraints from 8 years of IceCube TeV-scale atmospheric data

The IceCube Neutrino Observatory is a gigaton-scale Cherenkov detector located within the South Pole glacial ice. The detector's sensitivity to neutrino signals from GeV to PeV energies allows for probes into hypothetical energy-sensitive nonstandard interactions (NSI). Using the range of matte...

Full description

Bibliographic Details
Main Author: Grant Parker
Format: Conference Object
Language:unknown
Published: Zenodo 2022
Subjects:
South pole
Online Access:https://doi.org/10.5281/zenodo.6805552
id ftzenodo:oai:zenodo.org:6805552
record_format openpolar
spelling ftzenodo:oai:zenodo.org:6805552 2024-09-15T18:36:41+00:00 Leading NSI constraints from 8 years of IceCube TeV-scale atmospheric data Grant Parker 2022-07-07 https://doi.org/10.5281/zenodo.6805552 unknown Zenodo https://zenodo.org/communities/neutrino2022-posters https://doi.org/10.5281/zenodo.6805551 https://doi.org/10.5281/zenodo.6805552 oai:zenodo.org:6805552 info:eu-repo/semantics/openAccess Creative Commons Attribution 4.0 International https://creativecommons.org/licenses/by/4.0/legalcode info:eu-repo/semantics/conferencePoster 2022 ftzenodo https://doi.org/10.5281/zenodo.680555210.5281/zenodo.6805551 2024-07-25T09:12:26Z The IceCube Neutrino Observatory is a gigaton-scale Cherenkov detector located within the South Pole glacial ice. The detector's sensitivity to neutrino signals from GeV to PeV energies allows for probes into hypothetical energy-sensitive nonstandard interactions (NSI). Using the range of matter baselines provided by Earth, IceCube has been able to constrain neutral-current NSI by searching for deviations from the standard prediction of neutrino fluxes. With a 90% confidence interval of −0.0041 < εμτ < 0.0031, we present the world-leading constraints on the mu-tau flavor-changing parameter from a study 8 years of high-energy (500 GeV - 10 TeV) upgoing muon tracks. Conference Object South pole Zenodo
institution Open Polar
collection Zenodo
op_collection_id ftzenodo
language unknown
description The IceCube Neutrino Observatory is a gigaton-scale Cherenkov detector located within the South Pole glacial ice. The detector's sensitivity to neutrino signals from GeV to PeV energies allows for probes into hypothetical energy-sensitive nonstandard interactions (NSI). Using the range of matter baselines provided by Earth, IceCube has been able to constrain neutral-current NSI by searching for deviations from the standard prediction of neutrino fluxes. With a 90% confidence interval of −0.0041 < εμτ < 0.0031, we present the world-leading constraints on the mu-tau flavor-changing parameter from a study 8 years of high-energy (500 GeV - 10 TeV) upgoing muon tracks.
format Conference Object
author Grant Parker
spellingShingle Grant Parker
Leading NSI constraints from 8 years of IceCube TeV-scale atmospheric data
author_facet Grant Parker
author_sort Grant Parker
title Leading NSI constraints from 8 years of IceCube TeV-scale atmospheric data
title_short Leading NSI constraints from 8 years of IceCube TeV-scale atmospheric data
title_full Leading NSI constraints from 8 years of IceCube TeV-scale atmospheric data
title_fullStr Leading NSI constraints from 8 years of IceCube TeV-scale atmospheric data
title_full_unstemmed Leading NSI constraints from 8 years of IceCube TeV-scale atmospheric data
title_sort leading nsi constraints from 8 years of icecube tev-scale atmospheric data
publisher Zenodo
publishDate 2022
url https://doi.org/10.5281/zenodo.6805552
genre South pole
genre_facet South pole
op_relation https://zenodo.org/communities/neutrino2022-posters
https://doi.org/10.5281/zenodo.6805551
https://doi.org/10.5281/zenodo.6805552
oai:zenodo.org:6805552
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.680555210.5281/zenodo.6805551
_version_ 1810480384689831936

Similar Items