  A brief summary of the application of coherent states in the examination of
quantum dynamics of cosmological models is given. We discuss quantization maps,
phase space probability distributions and semiclassical phase spaces. The
implementation of coherent states based on the affine group resolves the
hardest singularities, renders self-adjoint Hamiltonians without boundary
conditions and provides a completely consistent semi-classical description of
the involved quantum dynamics. We consider three examples: the closed Friedmann
model, the anisotropic Bianchi Type I model and the deep quantum domain of the
Bianchi Type IX model.
