  In the Starobinsky inflationary model inflation is driven by quantum
corrections to the vacuum Einstein equation. We reduce the Wheeler-DeWitt
equation corresponding to the Starobinsky model to a Schroedinger form
containing time. The Schroedinger equation is solved with a Gaussian ansatz.
Using the prescription for the normalization constant of the wavefunction given
in our previous work, we show that the Gaussian ansatz demands Hawking type
initial conditions for the wavefunction of the universe. The wormholes induce
randomness in initial states suggesting a basis for time-contained description
of the Wheeler-DeWitt equation.
