  An attractive class of SUSY-breaking mechanisms predicts a photino mass of
order 1 GeV. Relic photinos can naturally account for the observed dark matter.
Detection of these light photinos is discussed and contrasted with conventional
WIMPs. In this scenario the gluino mass is about 100 MeV. The lightest
gluino-containing baryon could account for the recently observed ultra-high
energy cosmic rays, which violate the GZK bound.
