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Radiowave Method of High Energy Neutrino Detection: calculation of the expected event rate

A. L. Provorov, I. M. Zheleznykh

hep-pharXiv:hep-ph/9505218

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.

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