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...
| Main Authors: | , |
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| Format: | Text |
| Language: | English |
| Published: |
1993
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| Subjects: | |
| Online Access: | http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.346.9943 http://arxiv.org/pdf/hep-ph/9505218v1.pdf |
| Summary: | 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 |
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