Simultaneous Hamiltonian Treatment of Class a Spacetimes and Reduction of Degrees of Freedom at the Quantum Level

We consider the quantization of a general spatially homogeneous space-time belonging to an arbitrary but fixed Class A Bianchi type. Exploiting the information furnished by the quantum version of the momentum constraints, we use as variables the two simplest scalar contractions of C βγ and γαβ as well as the determinant of γαβ . We thus arrive at an equation for the wave function in terms of these quantities. This fact enables us to treat in a uniform manner all Class A cosmologies. For these spacetimes the Langrangian used correctly reproduces Einstein’s equations. We also discuss the imposition of simplifying ansatzen at the quantum level in a way that respects the scalings of the quadratic Hamiltonian constraint.