Alternative Detection Methods for Highest Energy Neutrinos
arXiv:astro-ph/0411715 · doi:10.1016/j.nuclphysbps.2005.01.135
Abstract
Several experimental techniques are currently under development, to measure the expected tiny fluxes of highest energy neutrinos above 10**18 eV. Projects in different stages of realisation are discussed here, which are based on optical and radio as well as acoustic detectors. For the detection of neutrino events in this energy range a combination of different detector concepts in one experiment seems to be most promising.
8 pages, 8 figures, to be published in Nuclear Physics B (Proceedings Supplement): Proceedings of the XXIst International Conference on Neutrino Physics and Astrophysics, Paris, June 14-19, 2004
References in corpus (5)
- Neutrinos from propagation of ultra-high energy protons
- Observation of the Askaryan Effect: Coherent Microwave Cherenkov Emission from Charge Asymmetry in High Energy Particle Cascades
- Detecting Radio Emission from Cosmic Ray Air Showers and Neutrinos with a Digital Radio Telescope
- Measurements of the Suitability of Large Rock Salt Formations for Radio Detection of High Energy Neutrinos
- Comparison of Optical, Radio, and Acoustical Detectors for Ultrahigh-Energy Neutrinos