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

Preprint

3 May 1995

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.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.

Keywords

HIGH ENERGY NEUTRINO
NEUTRINO DETECTION
RADIOWAVE METHOD
EXPECTED EVENT
ANTARCTICA
NEUTRINOS
DIFFUSE
SHOWER

All Related Versions

Version 1, 1995-05-03, ArXiv
Published version: Astroparticle Physics, 4 (1), 55.

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