On Radio Detection of Ultra-High Energy Neutrinos in Antarctic Ice
Interactions of ultrahigh energy neutrinos of cosmological origin in large volumes of dense, radio-transparent media can be detected via coherent Cherenkov emission from accompanying electromagnetic showers. Antarctic ice meets the requirements for an efficient detection medium for a radio frequency...
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ftdatacite:10.48550/arxiv.astro-ph/9507078 2023-05-15T14:00:14+02:00 On Radio Detection of Ultra-High Energy Neutrinos in Antarctic Ice Frichter, George M. Ralston, John P. McKay, Douglas W. 1995 https://dx.doi.org/10.48550/arxiv.astro-ph/9507078 https://arxiv.org/abs/astro-ph/9507078 unknown arXiv https://dx.doi.org/10.1103/physrevd.53.1684 Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004 http://arxiv.org/licenses/assumed-1991-2003/ Astrophysics astro-ph High Energy Physics - Phenomenology hep-ph FOS Physical sciences article-journal Article ScholarlyArticle Text 1995 ftdatacite https://doi.org/10.48550/arxiv.astro-ph/9507078 https://doi.org/10.1103/physrevd.53.1684 2022-04-01T17:14:35Z Interactions of ultrahigh energy neutrinos of cosmological origin in large volumes of dense, radio-transparent media can be detected via coherent Cherenkov emission from accompanying electromagnetic showers. Antarctic ice meets the requirements for an efficient detection medium for a radio frequency neutrino telescope. We carefully estimate the sensitivity of realistic antennas embedded deep in the ice to 100 MHz - 1 GHz signals generated by predicted neutrino fluxes from active galactic nuclei. Our main conclusion is that a {\it single radio receiver} can probe a $\sim 1$ ${\rm km}^3$ volume for events with primary energy near 2 PeV and that the total number of events registered would be roughly 200 to 400 ${\rm year}^{-1}$ in our most conservative estimate. An array of such receivers would increase sensitivity dramatically. A radio neutrino telescope could directly observe and test our understanding of the most powerful particle accelerators in the universe, simultaneously testing the standard theory of particle physics at unprecedented energies. : 45 pages, 21 figures, uuencoded, gzipped, submitted to Phys. Rev. D, also available at http://poincare.math.ukans.edu/~frichter/radio.html (Shading in Figure 21 fixed) Text Antarc* Antarctic DataCite Metadata Store (German National Library of Science and Technology) Antarctic |
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Astrophysics astro-ph High Energy Physics - Phenomenology hep-ph FOS Physical sciences |
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Astrophysics astro-ph High Energy Physics - Phenomenology hep-ph FOS Physical sciences Frichter, George M. Ralston, John P. McKay, Douglas W. On Radio Detection of Ultra-High Energy Neutrinos in Antarctic Ice |
topic_facet |
Astrophysics astro-ph High Energy Physics - Phenomenology hep-ph FOS Physical sciences |
description |
Interactions of ultrahigh energy neutrinos of cosmological origin in large volumes of dense, radio-transparent media can be detected via coherent Cherenkov emission from accompanying electromagnetic showers. Antarctic ice meets the requirements for an efficient detection medium for a radio frequency neutrino telescope. We carefully estimate the sensitivity of realistic antennas embedded deep in the ice to 100 MHz - 1 GHz signals generated by predicted neutrino fluxes from active galactic nuclei. Our main conclusion is that a {\it single radio receiver} can probe a $\sim 1$ ${\rm km}^3$ volume for events with primary energy near 2 PeV and that the total number of events registered would be roughly 200 to 400 ${\rm year}^{-1}$ in our most conservative estimate. An array of such receivers would increase sensitivity dramatically. A radio neutrino telescope could directly observe and test our understanding of the most powerful particle accelerators in the universe, simultaneously testing the standard theory of particle physics at unprecedented energies. : 45 pages, 21 figures, uuencoded, gzipped, submitted to Phys. Rev. D, also available at http://poincare.math.ukans.edu/~frichter/radio.html (Shading in Figure 21 fixed) |
format |
Text |
author |
Frichter, George M. Ralston, John P. McKay, Douglas W. |
author_facet |
Frichter, George M. Ralston, John P. McKay, Douglas W. |
author_sort |
Frichter, George M. |
title |
On Radio Detection of Ultra-High Energy Neutrinos in Antarctic Ice |
title_short |
On Radio Detection of Ultra-High Energy Neutrinos in Antarctic Ice |
title_full |
On Radio Detection of Ultra-High Energy Neutrinos in Antarctic Ice |
title_fullStr |
On Radio Detection of Ultra-High Energy Neutrinos in Antarctic Ice |
title_full_unstemmed |
On Radio Detection of Ultra-High Energy Neutrinos in Antarctic Ice |
title_sort |
on radio detection of ultra-high energy neutrinos in antarctic ice |
publisher |
arXiv |
publishDate |
1995 |
url |
https://dx.doi.org/10.48550/arxiv.astro-ph/9507078 https://arxiv.org/abs/astro-ph/9507078 |
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Antarctic |
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Antarctic |
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Antarc* Antarctic |
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Antarc* Antarctic |
op_relation |
https://dx.doi.org/10.1103/physrevd.53.1684 |
op_rights |
Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004 http://arxiv.org/licenses/assumed-1991-2003/ |
op_doi |
https://doi.org/10.48550/arxiv.astro-ph/9507078 https://doi.org/10.1103/physrevd.53.1684 |
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