2003/03/04 by Christian Spiering · 1 citation
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Dark Matter and Cosmic Phenomena #Neutrino Physics Research #astro-ph
paper · pdf · doi:10.1016/s0920-5632(03)90957-1
published as J.Phys. G29 (2003) 843-852; Nucl.Phys.Proc.Suppl. 125 (2003) 1-10 · 11 pages, 15 figures. Talk given at the 18th European Cosmic Ray Conference, Moscow 2002, and the 8th Topical Seminar on Innovative Particle and Radiation Detectors, Siena 2002
arxiv created 2003/03/04 · openalex publication_date 2003/09/01 · arxiv updated 2009/12/01 · openalex created_date 2017/04/07 · openalex updated_date 2026/07/28
The next ten years promise to be a particularly exciting decade for high energy neutrino astrophysics. The frontier of TeV and PeV energy is presently being tackled by large, expandable arrays constructed in open water or ice. Detectors tailored to record acoustic, radio, fluorescence or air shower signatures from neutrino interactions at PeV-EeV energy are being designed in parallel. During the next decade, the sensitivity to neutrinos from TeV to EeV energies may improve by 2 to 3 orders of magnitude. This talk reviews methods, status and prospects of detectors and sketches a scenario for the experimental progress.