We study supersymmetric models that include a viable dark matter
candidate and that generate the observed baryon asymmetry of the Universe
at the electro-weak phase transition. We focus on the possibility of
probing these models with searches for the permanent electric dipole
moment (EDM) of the electron, with direct and indirect dark matter
searches, and with high energy colliders. We point out that the lightest
neutralino might play a key role for the generation of both baryonic and
dark matter. Current constraints on the flux of energetic neutrinos from
the Sun already put significant bounds on the available parameter space.
Detectable signals are predicted in EDM searches, future neutrino
telescopes, ton-sized direct detection experiments as well as, possibly,
at the Large Hadron Collider and at a future International Linear
Collider. This ensamble of probes makes ours a testable framework for the
origin of both the dark matter and the baryonic matter-antimatter
asymmetry in the Universe. Finally, we outline future directions in the
exploration of non-minimal supersymmetric setups, and the related
experimental and cosmological probes.