Detectability of certain dark-matter candidates

Details Detectability of certain dark-matter candidates Detectability of certain dark-matter candidates

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985phrvd..31.3059g&link_type=abstract

Physical Review D (Particles and Fields), Volume 31, Issue 12, 15 June 1985, pp.3059-3063

Physics

508

Supersymmetry

Scientific paper

We consider the possibility that the neutral-current neutrino detector recently proposed by Drukier and Stodolsky could be used to detect some possible candidates for the dark matter in galactic halos. This may be feasible if the galactic halos are made of particles with coherent weak interactions and masses 1-106 GeV; particles with spin-dependent interactions of typical weak strength and masses 1-102 GeV; or strongly interacting particles of masses 1-1013 GeV.

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