  Strong dynamics constitutes one of the pillars of the standard model of
particle interactions, and it accounts for the bulk of the visible matter in
the universe. It is therefore a well posed question to ask if the rest of the
universe can be described in terms of new highly natural four-dimensional
strongly coupled theories. The goal of this brief summary is to provide, for
the first time, a coherent overview of how new strong dynamics can be employed
to address the relevant challenges in particle physics and cosmology from
composite Higgs dynamics to dark matter and inflation.
