  The electroweak sector may play a crucial role in discovering supersymmetry.
We systematically investigate the patterns of the MSSM-like electroweakinos,
when the neutralino relic abundance $\Omega_\chi h^2\leq 0.12$, that is, also
admitting for multi-component Dark Matter, in a broad range of the parameter
space. We find that for a very large range of parameters the Direct Detection
experiments are/will be sensitive to underabundant neutralinos, in spite of the
strong rescaling of the flux factor. The second general conclusion is that the
bound $\Omega_\chi h^2\leq 0.12$ together with the LUX (XENON1T) limits for the
neutralino spin independent scattering cross sections constrain the
electroweakino spectrum so that the mass differences between the NLSP and the
LSP are smaller than 40 (10) GeV, respectively, with important implications for
the collider searches. The future Direct Detection experiments and the high
luminosity LHC run will probe almost the entire range of the LSP and NLSP mass
spectrum that is consistent with the bound $\Omega_\chi h^2\leq 0.12$.
