  Intrinsic time quantum geometrodynamics resolved `the problem of time' and
bridged the deep divide between quantum mechanics and canonical quantum gravity
with a Schrodinger equation which describes evolution in intrinsic time
variable. In this formalism, Einstein's general relativity is a particular
realization of a wider class of theories. Explicit classical black hole and
cosmological solutions and the motion of test particles are derived and
analyzed in this work in the context of constant three-curvature solutions in
intrinsic time geometrodynamics; and we exemplify how this formalism yields
results which agree with the predictions of Einstein's theory.
