Radiowave Method of High Energy Neutrino Detection: calculation of the expected event rate
arXiv:hep-ph/9505218 · doi:10.1016/0927-6505(95)00019-D
Abstract
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 sq.km area established in Central Antarctica.
arXiv commentTo be published by Astroparticle Physics, LaTeX file, 11 pages
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