  We study dark matter physics in the Minimal Supersymmetric Standard Model
with non-universal gaugino masses at the unification scale. In this scenario,
the specific ratio of wino and gluino masses realizes the electro-weak scale
naturally and achieves 125 GeV Higgs boson mass. Then, relatively light
higgsino is predicted and the lightest neutral particle, that is dominantly
given by the neutral component of higgsino, is a good dark matter candidate.
The direct detection of the dark matter is sensitive to not only a higgsino
mass but also gaugino masses significantly. The upcoming XENON1T experiment
excludes the parameter region where bino or gluino is lighter than about 2.5
TeV if the higgsino and the gaugino mass parameters have same signs. We see
that the direct detection of dark matter gives stronger bound than the direct
search at the LHC experiment when higgsino sizably contributes to the dark
matter abundance
