  We analyse the sensitivity of IceCube-DeepCore to annihilation of neutralino
dark matter in the solar core, generated within a 25 parameter version of the
minimally supersymmetric standard model (MSSM-25). We explore the
25-dimensional parameter space using scanning methods based on importance
sampling and using DarkSUSY 5.0.6 to calculate observables. Our scans produced
a database of 6.02 million parameter space points with neutralino dark matter
consistent with the relic density implied by WMAP 7-year data, as well as with
accelerator searches. We performed a model exclusion analysis upon these points
using the expected capabilities of the IceCube-DeepCore Neutrino Telescope. We
show that IceCube-DeepCore will be sensitive to a number of models that are not
accessible to direct detection experiments such as SIMPLE, COUPP and XENON100,
indirect detection using Fermi-LAT observations of dwarf spheroidal galaxies,
nor to current LHC searches.
