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A large fiber sensor network for an acoustic neutrino telescope

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Author: Buis, E.J. · Doppenberg, E.J.J. · Lahmann, R. · Toet, P.M.
Publisher: EDP Sciences
Source:Horandel, J.R.Lahmann, R.Scholten, O.Jong, S. deNahnhauer, R.Buitink, S., 7th International Conference on Acoustic and Radio EeV Neutrino Detection Activities, ARENA 2016, 7-10 June 2016, Groningen, The Netherlands, 135
EPJ Web of Conferences
Identifier: 756684
ISBN: 9782759890156
Article number: 06006
Keywords: High Tech Systems & Materials · Industrial Innovation · Nano Technology · OPT - Optics OM - Opto-Mechatronics · TS - Technical Sciences


The scientific prospects of detecting neutrinos with an energy close or even higher than the GKZ cut-off energy has been discussed extensively in literature. It is clear that due to their expected low flux,the detection of these ultra-high energy neutrinos (Eν > 1018 eV) requires a telescope larger than 100km3. Acoustic detection may provide a way to observe these ultra-high energy cosmic neutrinos, as sound that they induce in the deep sea when neutrinos lose their energy travels undisturbed for many kilometers. To realize a large scale acoustic neutrino telescope, dedicated technology must be developed that allows for a deep sea sensor network. Fiber optic hydrophone technology provides a promising means to establish a large scale sensor network with the proper sensitivity to detect the small signals from the neutrino interactions.