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In a baryon-symmetric universe, the baryon asymmetry observed for visiblematter is matched by an equal and opposite asymmetry for dark matter, therebyclosely connecting the number densities of both types of matter. This is anecessary step towards the goal of explaining the mystery of why the visibleand dark matter densities are observed to be similar. In this talk, a way ofproducing such a universe from bubble nucleation during a first-order phasetransition is reviewed. The process is an analog of electroweak baryogenesis.

Unified origin for visible and dark matter in a baryon-symmetric universe from a first-order phase transition