Limits on the flux of energetic neutrinos from the sun

Details Limits on the flux of energetic neutrinos from the sun Limits on the flux of energetic neutrinos from the sun

Apr 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987phlb..188..388l&link_type=abstract

Physics Letters B, Volume 188, Issue 3, p. 388-392.

Physics

48

Scientific paper

A number of authors have proposed mechanisms by which the sun could be a strong source of energetic neutrinos. We search for an excess signal of penetrating neutral particles from the direction of the sun. We employ two data samples. One sample studies energies from 400 MeV to 2 GeV. The other studies vμ interactions above 2 GeV where the atmospheric background is lower. Our results are compared with the general background of atmospheric neutrinos from other directions. No significant excess has been found. These results can be used to set limits on possible dark matter candidates.

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