  We show how the large-scale cosmological dynamics can be obtained from the
hydrodynamics of isotropic group field theory condensate states in the
Gross-Pitaevskii approximation. The correct Friedmann equations are recovered
in the semi-classical limit for some choices of the parameters in the action
for the group field theory, and quantum gravity corrections arise in the
high-curvature regime causing a bounce which generically resolves the big-bang
and big-crunch singularities.
