The Radio Cerenkov Technique for Ultra-High Energy Neutrino Detection

Abstract

I review the status of the Radio Cerenkov detection technique in searches for ultra-high energy (UHE) neutrinos of cosmic origin. After outlining the physics motivations for UHE neutrino searches, I give an overview of the status of current and proposed experiments in the field.

Proceedings of the 6th International Workshop on Ring Imaging Cherenkov Counters (RICH2007), Trieste, Italy 15 - 20 October 2007

References in corpus (6)

• First Year Performance of The IceCube Neutrino Telescope
• RICE Limits on the Diffuse Ultra-High Energy Neutrino Flux
• Constraints on Cosmic Neutrino Fluxes from the ANITA Experiment
• Observations of the Askaryan Effect in Ice
• First results of the Instrumentation Line for the deep-sea ANTARES neutrino telescope
• BAIKAL Experiment: main results obtained with the neutrino telescope NT200

Cited by in corpus (2)

• SUSY Renormalization Group Effects in Ultra High Energy Neutrinos
• High energy astrophysics with the next generation of radio astronomy facilities