Simulation of the Event Reconstruction of Ultra High Energy Cosmic Neutrinos with Askaryan Radio Array
Askaryan Radio Array (ARA), a large-scale radio Cherenkov observatory which scientists propose to develop in Antarctica, aims at discovering the origin and evolution of the cosmic accelerators that produce the highest energy cosmic rays by means of observing the ultra high energy (UHE) cosmogenic ne...
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ftdatacite:10.48550/arxiv.1002.0023 2023-05-15T14:02:37+02:00 Simulation of the Event Reconstruction of Ultra High Energy Cosmic Neutrinos with Askaryan Radio Array Sun, Shang-Yu Chen, Pisin Huang, Melin 2010 https://dx.doi.org/10.48550/arxiv.1002.0023 https://arxiv.org/abs/1002.0023 unknown arXiv arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ High Energy Astrophysical Phenomena astro-ph.HE Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences Preprint Article article CreativeWork 2010 ftdatacite https://doi.org/10.48550/arxiv.1002.0023 2022-04-01T15:02:10Z Askaryan Radio Array (ARA), a large-scale radio Cherenkov observatory which scientists propose to develop in Antarctica, aims at discovering the origin and evolution of the cosmic accelerators that produce the highest energy cosmic rays by means of observing the ultra high energy (UHE) cosmogenic neutrinos. To optimize ARA's angular resolution of the incoming UHE neutrinos, which is essential for pointing pack to its source, the relation between the reconstruction capabilities of ARA and its design is studied. It is found that with the noise effect taken into account, in order to make this neutrino angular resolution as good as possible and detection efficiency as high as possible, the optimal choice for ARA geometry would be the station spacing of 1.6 km and the antenna spacing of 40 m. : 7 pages, 12 figures, presented at the CosPA Symposium, Melbourne, Australia, November 2009 Report Antarc* Antarctica DataCite Metadata Store (German National Library of Science and Technology) |
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DataCite Metadata Store (German National Library of Science and Technology) |
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High Energy Astrophysical Phenomena astro-ph.HE Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences |
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High Energy Astrophysical Phenomena astro-ph.HE Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences Sun, Shang-Yu Chen, Pisin Huang, Melin Simulation of the Event Reconstruction of Ultra High Energy Cosmic Neutrinos with Askaryan Radio Array |
topic_facet |
High Energy Astrophysical Phenomena astro-ph.HE Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences |
description |
Askaryan Radio Array (ARA), a large-scale radio Cherenkov observatory which scientists propose to develop in Antarctica, aims at discovering the origin and evolution of the cosmic accelerators that produce the highest energy cosmic rays by means of observing the ultra high energy (UHE) cosmogenic neutrinos. To optimize ARA's angular resolution of the incoming UHE neutrinos, which is essential for pointing pack to its source, the relation between the reconstruction capabilities of ARA and its design is studied. It is found that with the noise effect taken into account, in order to make this neutrino angular resolution as good as possible and detection efficiency as high as possible, the optimal choice for ARA geometry would be the station spacing of 1.6 km and the antenna spacing of 40 m. : 7 pages, 12 figures, presented at the CosPA Symposium, Melbourne, Australia, November 2009 |
format |
Report |
author |
Sun, Shang-Yu Chen, Pisin Huang, Melin |
author_facet |
Sun, Shang-Yu Chen, Pisin Huang, Melin |
author_sort |
Sun, Shang-Yu |
title |
Simulation of the Event Reconstruction of Ultra High Energy Cosmic Neutrinos with Askaryan Radio Array |
title_short |
Simulation of the Event Reconstruction of Ultra High Energy Cosmic Neutrinos with Askaryan Radio Array |
title_full |
Simulation of the Event Reconstruction of Ultra High Energy Cosmic Neutrinos with Askaryan Radio Array |
title_fullStr |
Simulation of the Event Reconstruction of Ultra High Energy Cosmic Neutrinos with Askaryan Radio Array |
title_full_unstemmed |
Simulation of the Event Reconstruction of Ultra High Energy Cosmic Neutrinos with Askaryan Radio Array |
title_sort |
simulation of the event reconstruction of ultra high energy cosmic neutrinos with askaryan radio array |
publisher |
arXiv |
publishDate |
2010 |
url |
https://dx.doi.org/10.48550/arxiv.1002.0023 https://arxiv.org/abs/1002.0023 |
genre |
Antarc* Antarctica |
genre_facet |
Antarc* Antarctica |
op_rights |
arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
op_doi |
https://doi.org/10.48550/arxiv.1002.0023 |
_version_ |
1766272928442220544 |