  In this letter, we show that the wino-Higgsino dark matter (DM) is detectable
in near future DM direct detection experiments for almost all consistent
parameter space in the spontaneously broken supergravity (SUGRA) if the muon
g-2 anomaly is explained by the wino-Higgsino loop diagrams. We also point out
that the present and future LHC experiments can exclude or confirm this SUGRA
explanation of the observed muon g-2 anomaly.
