On the detection of cosmic high-energy neutrinos

Details On the detection of cosmic high-energy neutrinos On the detection of cosmic high-energy neutrinos

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...287..713v&link_type=abstract

Astronomy and Astrophysics 287, 713-715 (1994)

Astronomy and Astrophysics

Astrophysics

Cosmology: Dark Matter, Observations, Sun: Particle Emission, Elementary Particles

Scientific paper

In connection with plans to construct new giant underground/underwater installations, possible experiments for searching for neutralinos as a dark matter candidate are widely discussed currently. We show that high energy neutrinos generated by cosmic rays in the Sun could be a considerable background for such experiments. These fluxes are higher than atmospheric neutrino fluxes in some energy intervals but only installations of Giga-DUMAND type with good angle resolution (better than 0.5deg) are able to register at the Earth muons from these neutrinos.

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