The feasibility of detecting neutrinos of cosmic origin by radio frequency Cherenkov radiation in Antarctic ice

Details The feasibility of detecting neutrinos of cosmic origin by radio frequency Cherenkov radiation in Antarctic ice The feasibility of detecting neutrinos of cosmic origin by radio frequency Cherenkov radiation in Antarctic ice

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aph.....5..255j&link_type=abstract

ASTROPARTICLE PHYSICS, Volume 5, Issue ASTROPARTICLE PHYSICS, p. 255-261.

Physics

9

Scientific paper

It has been suggested that high-energy neutrinos of cosmic origin, in the energy-range 1 TeV-1 PeV, interacting in the Antarctic ice, may be detected through the Cherenkov radio emission to which they indirectly give rise. The present article addresses two problems which do not seem to have been discussed previously in any detail. The first concerns various relevant features of the Antarctic ice. The second concerns radio interference, particularly as it applies to single, rare, and isolated pulses, each lasting only a few nanoseconds.

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