Indirect detection of heavy supersymmetric dark matter

Details Indirect detection of heavy supersymmetric dark matter Indirect detection of heavy supersymmetric dark matter

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991tapp.conf.....k&link_type=abstract

Presented at the International Conference on Trends in Astroparticle Physics, Santa Monica, 26 Nov. - 1 Dec. 1990

Physics

Dark Matter, Detection, Galactic Cosmic Rays, Supersymmetry, Annihilation Reactions, Halos, Neutrinos, Radiation Detectors

Scientific paper

If neutralinos reside in the galactic halo they will be captured in the Sun and annihilate therein producing high-energy neutrinos. Present limits on the flux of such neutrinos from underground detectors such as IMB and Kamiokande 2 may be used to rule out certain supersymmetric dark-matter candidates, while in many other supersymmetric models the rates are large enough that if neutralinos do reside in the galactic halo, observation of a neutrino signal may be possible in the near future.

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