Speaker
Description
A possible explanation of the origin of baryon asymmetry in the universe is provided by electroweak (EW) baryogenesis, where the asymmetry is generated during a first-order phase transition. This can be realized in the presence of new physics that modify the Higgs dynamics.
Non minimal Composite Higgs models based on the coset SO(6)/SO(5) offer a suitable extension of the SM Higgs sector that can realize baryogenesis.
The scalar sector of the theory is enriched by an additional scalar singlet field that triggers a ``two-step'' EW phase transition and introduces additional sources of CP-violation.
In this talk I will discuss the dynamics of the two-step phase transition,
with particular focus on the conditions needed for baryogenesis.
An important requirement is the breaking of a discrete
The current bounds on the electric dipole moments of the electron and the neutron impose very mild constraints on the amount of