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

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.

Comments: To be published by Astroparticle Physics, LaTeX file, 11 pages