  The neutralino, the lightest stable supersymmetric particle, is a strong
theoretical candidate for the missing astronomical "dark matter". Depending on
their annihilation cross section, relic neutralinos from early formation of the
Universe trapped in orbits around massive objects may currently be annihilating
at measurable rates. The Minimal Supersymmetric extension of the Standard Model
predicts that the gamma rays emerging from one of the annihilation modes will
give a distinct monochromatic signal with energy between 100GeV and 10TeV,
depending on the neutralino mass. An additional "continuum" spectrum signal of
photons will be produced by the decay of secondaries produced in the
non-photonic annihilation modes.
  Milagro is an air shower array which uses the water Cherenkov technique and
is capable of detecting TeV gamma rays from the direction of the Sun with an
angular resolution of less than a degree. It is the first instrument capable of
establishing a limit on the gamma-ray flux from neutralino annihilations near
the Sun.
  In this report results of a search for neutralino to photon annihilation with
the Milagro gamma-ray observatory are presented.
