Future High Energy Neutrino Telescopes

Abstract

This talk summarizes the main physics goals and basic methods of telescopes for high energy neutrinos. It reviews the present status of deep underwater telescopes and sketches the ICECUBE project as an example for a cube kilometer detector. It is suggested to develop techniques for radio and acoustic detection hand in hand with big optical arrays. These large arrays should be complemented by medium-size detectors in the Megaton range.

Talk given at the Int.Conf.on Neutrino Physics and Astrophysics, Sudbury 2000, 8 pages, 7 figures

References in corpus (3)

• The AMANDA Neutrino Telescope: Principle of Operation and First Results
• Comparison of Optical, Radio, and Acoustical Detectors for Ultrahigh-Energy Neutrinos
• Radiowave Method of High Energy Neutrino Detection: calculation of the expected event rate

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• The prompt lepton cookbook
• Discovering Long Wavelength Neutrino Oscillations in the Distorted Neutrino Spectrum of Galactic Supernova Remnants
• Simultaneous measurements of water optical properties by AC9 transmissometer and ASP-15 Inherent Optical Properties meter in Lake Baikal
• The prompt TeV-PeV atmospheric neutrino window
• Extragalactic neutrino background from very young pulsars surrounded by supernova envelopes