  We examine spinfoam cosmology by use of a simple graph adapted to homogeneous
cosmological models. We calculate dynamics in the isotropic limit, and provide
the framework for the aniostropic case. The dynamical behaviour is calculating
transition amplitudes between holomorphic coherent states on a single node
graph. The resultant dynamics is peaked on solutions which have no support on
the zero volume state, indicating that big bang type singularities are avoided
within such models.
