Jun 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002naap.conf..103d&link_type=abstract
NON-ACCELERATOR ASTROPARTICLE PHYSICS. Proceedings of the Sixth School. Held 9-20 July 2001 in ICTP, Trieste, Italy. Edited by R
Physics
Scientific paper
Neutrino astronomy is one of the frontier of the high energy astrophysics. I discuss how to build a neutrino telescope and which requirements such a detector must fulfil. A measurable flux of astrophysical neutrinos is predicted by several models for a detector at the cubic kilometer scale. The way pursued until now in building such huge apparatuses is Cherenkov light detection in water or in ice. There have been attempts to build neutrino telescopes and also some projects are yet under construction or under way to start. This situation is reviewed and also techniques alternatives to the Cherenkov light detection are mentioned.
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