Starobinsky model in Schrodinger description

In the Starobinsky inflationary model inflation is driven by quantum correc tions to the vacuum Einstein equation. We reduce the Wheeler-DeWitt equatio n corresponding to the Starobinsky model to a Schrodinger form containing t ime. The Schrodinger equation is solved with a Gaussian ansatz. Using the p rescription for the normalization constant of the wave function given in ou r previous work, we show that the Gaussian ansatz demands Hawking type init ial conditions for the wave function of the universe. The wormholes induce randomness in initial states suggesting a basis for time-contained descript ion of the Wheeler-DeWitt equation.