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Motivated by the absence of dark matter signals in direct detectionexperiments and the discovery of gravitational waves (GWs) at aLIGO, we discussthe possibility to explore a generic classes of scalar dark matter models usingthe complementary searches via phase transition gravitational waves and thefuture lepton collider signatures. We focus on the inert scalar multiplet darkmatter models and the mixed inert scalar dark matter models, which couldundergo a strong first-order phase transitions during the evolution of theearly universe, and might produce detectable phase transition GW signals atfuture GW experiments, such as eLISA, DECIGO and BBO. We find that the futureGW signature, together with circular electron-positron collider, could furtherexplore the model's blind spot parameter region, at which the dark matter-Higgscoupling is identically zero, thus avoiding the dark matter spin-independentdirect detection constraints.

Explore Inert Dark Matter Blind Spots with Gravitational Wave Signatures