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18 April 2024
 
  » arxiv » astro-ph/9705189

 Article overview


Sadco: Hydroacoustic Detection of Super-High Energy Cosmic Neutrinos
L. G. Dedenko ; A. V. Furduev ; Ya. S. Karlik ; J. G. Learned ; A. A. Mironovich ; V. D. Svet ; I. M. Zheleznykh ;
Date 23 May 1997
Subject astro-ph
Affiliation Institute for Nuclear Research of Russian Academy of Sciences, Moscow, Russia, N. N. Andreev Acoustic Institute, Moscow, Russia, Central Research Institute ``Morfizpribor’’, St.Petersburg, Russia, Department of Physics and Astronomy, Un
AbstractAn 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.
Source arXiv, astro-ph/9705189
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