Sadco: Hydroacoustic Detection of Super-High Energy Cosmic Neutrinos

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dc.creatorDedenko, L. G.
dc.creatorFurduev, A. V.
dc.creatorKarlik, Ya. S.
dc.creatorLearned, J. G.
dc.creatorMironovich, A. A.
dc.creatorSvet, V. D.
dc.creatorZheleznykh, I. M.
dc.date1997-05-23
dc.date.accessioned2026-07-07T02:23:26Z
dc.date.available2026-07-07T02:23:26Z
dc.descriptionAn attractive technique to explore for super-high-energy cosmic neutrino fluxes, via deep underwater acoustic detection, is discussed. Acoustic signals emitted by the neutrino induced cascades at large distances (10-50 km) from cascades are considered. It is argued that an existing hydroacoustic array of 2400 hydrophones, which is available in the Great Ocean near Kamchatka Peninsula, could be used as a base for an exploratory acoustic neutrino telescope SADCO (Sea Acoustic Detector of Cosmic Objects). The detection volume for registration of cascades with energies in the range of $10^{20-21} eV$ is estimated to be hundreds of cubic kilometers. Some models of extremely high energy elementary particle production in the Universe (for example the topological defect model) may be examined by such a detector. Tests of this technique are hoped for within a year.
dc.description4 pages, in LaTex and PS formats, 2 EPS figures, uses wrapfig.sty, times.sty, and mathptm.sty
dc.identifierhttps://arxiv.org/abs/astro-ph/9705189
dc.identifierhttp://arxiv.org/abs/astro-ph/9705189
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11245
dc.subjectAstrophysics
dc.titleSadco: Hydroacoustic Detection of Super-High Energy Cosmic Neutrinos
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