  Spherically symmetric space-times provide many examples for interesting black
hole solutions, which classically are all singular. Following a general
program, space-like singularities in spherically symmetric quantum geometry, as
well as other inhomogeneous models, are shown to be absent. Moreover, one sees
how the classical reduction from infinitely many kinematical degrees of freedom
to only one physical one, the mass, can arise, where aspects of quantum
cosmology such as the problem of initial conditions play a role.
