Radiowave Method of High Energy Neutrino Detection: Calculation of Expected Event Rate

The sensitivity of an ice radiowave detector to the anticipated high energy neutrino fluxes is calculated on the basis of a detailed threshold analysis and computation of the shower production rate. We show that diffuse neutrinos from Active Galactic Nuclei could be detectable in a radio detector of...

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Main Authors: A. L. Provorov, I. M. Zheleznykh
Other Authors: The Pennsylvania State University CiteSeerX Archives
Format: Text
Language:English
Published: 1993
Subjects:
Antarc*
Antarctica
Online Access:http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.346.9943
http://arxiv.org/pdf/hep-ph/9505218v1.pdf
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spelling ftciteseerx:oai:CiteSeerX.psu:10.1.1.346.9943 2023-05-15T13:56:06+02:00 Radiowave Method of High Energy Neutrino Detection: Calculation of Expected Event Rate A. L. Provorov I. M. Zheleznykh The Pennsylvania State University CiteSeerX Archives 1993 application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.346.9943 http://arxiv.org/pdf/hep-ph/9505218v1.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.346.9943 http://arxiv.org/pdf/hep-ph/9505218v1.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://arxiv.org/pdf/hep-ph/9505218v1.pdf text 1993 ftciteseerx 2016-01-08T00:08:56Z The sensitivity of an ice radiowave detector to the anticipated high energy neutrino fluxes is calculated on the basis of a detailed threshold analysis and computation of the shower production rate. We show that diffuse neutrinos from Active Galactic Nuclei could be detectable in a radio detector of 1 km 2 area established in Central Antarctica. 1 Text Antarc* Antarctica Unknown
institution Open Polar
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language English
description The sensitivity of an ice radiowave detector to the anticipated high energy neutrino fluxes is calculated on the basis of a detailed threshold analysis and computation of the shower production rate. We show that diffuse neutrinos from Active Galactic Nuclei could be detectable in a radio detector of 1 km 2 area established in Central Antarctica. 1
author2 The Pennsylvania State University CiteSeerX Archives
format Text
author A. L. Provorov
I. M. Zheleznykh
spellingShingle A. L. Provorov
I. M. Zheleznykh
Radiowave Method of High Energy Neutrino Detection: Calculation of Expected Event Rate
author_facet A. L. Provorov
I. M. Zheleznykh
author_sort A. L. Provorov
title Radiowave Method of High Energy Neutrino Detection: Calculation of Expected Event Rate
title_short Radiowave Method of High Energy Neutrino Detection: Calculation of Expected Event Rate
title_full Radiowave Method of High Energy Neutrino Detection: Calculation of Expected Event Rate
title_fullStr Radiowave Method of High Energy Neutrino Detection: Calculation of Expected Event Rate
title_full_unstemmed Radiowave Method of High Energy Neutrino Detection: Calculation of Expected Event Rate
title_sort radiowave method of high energy neutrino detection: calculation of expected event rate
publishDate 1993
url http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.346.9943
http://arxiv.org/pdf/hep-ph/9505218v1.pdf
genre Antarc*
Antarctica
genre_facet Antarc*
Antarctica
op_source http://arxiv.org/pdf/hep-ph/9505218v1.pdf
op_relation http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.346.9943
http://arxiv.org/pdf/hep-ph/9505218v1.pdf
op_rights Metadata may be used without restrictions as long as the oai identifier remains attached to it.
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