  In this review we focus on the main cosmological implications of the Group
Field Theory approach, according to which an effective continuum macroscopic
dynamics can be extracted from the underlying formalism for quantum gravity.
Within this picture what counts is the collective behaviour of a large number
of quanta of geometry. The resulting state is a condensate-like structure made
of "pre-geometric" excitations of the Group Field Theory field over a no-space
vacuum. Starting from the kinematics and dynamics, we offer an overview of the
way in which Group Field Theory condensate cosmology treats solutions for the
homogeneous and isotropic universe. These solutions including a bounce, share
with other quantum cosmological approaches the resolution of the singularity
characterizing general relativity. Contrary to what is usually done in quantum
cosmology, in GFT cosmology no preliminary symmetry reduction is needed for
this purpose. We conclude with a discussion of the limits and future
perspectives of the Group Field Theory approach.
