Christian Spiering 2003 J. Phys. G: Nucl. Part. Phys. 29 843 doi:10.1088/0954-3899/29/5/306
Christian Spiering
Show affiliationsThe next ten years promise to be a particularly exciting decade for high energy neutrino astrophysics. The frontier of TeV and PeV energies 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 two to three orders of magnitude. This paper reviews the methods, status and prospects of detectors and sketches a scenario for the experimental progress.
95.30.Cq Elementary particle processes
01.30.Rr Surveys and tutorial papers; resource letters
Accelerators, beams and electromagnetism
Instrumentation and measurement
Issue 5 (May 2003)
Received 10 October 2002, in final form 10 January 2003
Published 9 April 2003
Christian Spiering 2003 J. Phys. G: Nucl. Part. Phys. 29 843
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