Extrinsic time is identified in most isotropic and homogeneous cosmolo
gical models by matching it with the ideal clock-a parametrized system
whose only ''degree of freedom'' is time. Once this matching is estab
lished, the cosmological models are quantized in the same way as the i
deal clock. The space of solutions of the Wheeler-DeWitt equation is t
urned into a Hilbert space by inserting a time-dependent operator in t
he inner product, yielding a unitary theory equivalent to the phase-sp
ace-reduced theory.