The measured Higgs mass value 125 GeV suggests that the standard model of particle physics may be
a UV-complete theory all the way up to Planck scale. This suggests that we may have to re-evaluate
some long-standing theoretical concepts such as the gauge unification and the hierarchy problem.
However, the questions of the nature of the dark matter, dark energy and of the origin of the baryon
asymmetry remain unsolved in the SM. An obvious questino then is, can we solve these problems and
still maintain UV-completeness in (simple) extensios of the SM (without complex constructs such as
supersymmetry or technicolor)?
I will discuss the DM and baryogenesis problems in a bottom up approach in the context of scalar
extensions of the SM. Baryogenesis in these models occurs at electroweak phase transition and so I
will give a brief, qualitative overview of the electroweak baryogenesis mechanism. I will argue that
by far the worst problem for this model building scheme is providing sufficient charge-parity
violation. A possible way out is to combine the two, such that the CP-violation comes from Dark
sector and may involve the DM particle directly.