Hunting For Cosmogenic Neutrinos With The Arianna Experiment
The discovery of cosmogenic neutrinos is going to be a major milestone in high-energy neutrino astronomy. Due to the low flux of cosmogenic neutrinos effective volumes of at least an order of magnitude improvement of the size of the IceCube detector are needed. As optical methods are cost-prohibitiv...
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ftdatacite:10.5281/zenodo.1302899 2023-05-15T13:57:00+02:00 Hunting For Cosmogenic Neutrinos With The Arianna Experiment GLASER, Christian 2018 https://dx.doi.org/10.5281/zenodo.1302899 https://zenodo.org/record/1302899 unknown Zenodo https://dx.doi.org/10.5281/zenodo.1302898 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.1302899 https://doi.org/10.5281/zenodo.1302898 2021-11-05T12:55:41Z The discovery of cosmogenic neutrinos is going to be a major milestone in high-energy neutrino astronomy. Due to the low flux of cosmogenic neutrinos effective volumes of at least an order of magnitude improvement of the size of the IceCube detector are needed. As optical methods are cost-prohibitive at these scales, the radio technique is most promising. The ARIANNA detector aims to detect neutrinos with energies above 1016 eV by instrumenting 0.5 Teratons of ice with a surface array of a thousand independent radio detector stations in Antarctica. Several pilot stations are currently operating successfully at the Moore's Bay site (Ross Ice Shelf) and at the South Pole. We will demonstrate the capabilities of the detector by reconstructing the signal direction and polarization from in-ice pulser studies and via the detection of the more abundant cosmic-ray air showers. Furthermore, we will discuss the science capabilities of ARIANNA. Still Image Antarc* Antarctica Ice Shelf Ross Ice Shelf South pole South pole DataCite Metadata Store (German National Library of Science and Technology) Ross Ice Shelf South Pole |
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The discovery of cosmogenic neutrinos is going to be a major milestone in high-energy neutrino astronomy. Due to the low flux of cosmogenic neutrinos effective volumes of at least an order of magnitude improvement of the size of the IceCube detector are needed. As optical methods are cost-prohibitive at these scales, the radio technique is most promising. The ARIANNA detector aims to detect neutrinos with energies above 1016 eV by instrumenting 0.5 Teratons of ice with a surface array of a thousand independent radio detector stations in Antarctica. Several pilot stations are currently operating successfully at the Moore's Bay site (Ross Ice Shelf) and at the South Pole. We will demonstrate the capabilities of the detector by reconstructing the signal direction and polarization from in-ice pulser studies and via the detection of the more abundant cosmic-ray air showers. Furthermore, we will discuss the science capabilities of ARIANNA. |
format |
Still Image |
author |
GLASER, Christian |
spellingShingle |
GLASER, Christian Hunting For Cosmogenic Neutrinos With The Arianna Experiment |
author_facet |
GLASER, Christian |
author_sort |
GLASER, Christian |
title |
Hunting For Cosmogenic Neutrinos With The Arianna Experiment |
title_short |
Hunting For Cosmogenic Neutrinos With The Arianna Experiment |
title_full |
Hunting For Cosmogenic Neutrinos With The Arianna Experiment |
title_fullStr |
Hunting For Cosmogenic Neutrinos With The Arianna Experiment |
title_full_unstemmed |
Hunting For Cosmogenic Neutrinos With The Arianna Experiment |
title_sort |
hunting for cosmogenic neutrinos with the arianna experiment |
publisher |
Zenodo |
publishDate |
2018 |
url |
https://dx.doi.org/10.5281/zenodo.1302899 https://zenodo.org/record/1302899 |
geographic |
Ross Ice Shelf South Pole |
geographic_facet |
Ross Ice Shelf South Pole |
genre |
Antarc* Antarctica Ice Shelf Ross Ice Shelf South pole South pole |
genre_facet |
Antarc* Antarctica Ice Shelf Ross Ice Shelf South pole South pole |
op_relation |
https://dx.doi.org/10.5281/zenodo.1302898 |
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.1302899 https://doi.org/10.5281/zenodo.1302898 |
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1766264613584764928 |