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RADIO TELESCOPES AS THE DETECTORS OF SUPER HIGH-ENERGY NEUTRIONS
Pages 87-90

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From page 87...
... ZHELEZNYKH, Institute for Nuclear Research The registration of super-high-energy neutrinos is a very difficult and also very important problem that requires construction of detectors with large effective target masses. In 1961, Aska~yan pouted out me possibility of registering cascades in dense media by the Cherenkov radioemission of an excess of negative charges in the cascades which arose in interaction between high energy particles and the atoms of medium.
From page 88...
... Therefore, the integration time cannot be less than T`li~p = 1/^f~li5p, and so we shall observe usually spreaded pulses. On the other hand, it will be possible to use multichannel receivers with the total (effective)
From page 89...
... Unfortunately, at present there is no good prediction of high-energy neutrinos fluxes. However, many modern models of the universe, for example the models with superconductive cosmic strings or with supermassive particles (monopoles, maximons)
From page 90...
... However, proton interactions will be observed only near the edge of a lunar disk, whereas neutrino interactions will occur at every part of the disk with approximately the same probability. There is additional difficulty concerning the registration of such relativel`,r rare sporadic radio pulses in the presence of different kinds of interference.


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