We study multidimensional cosmology to obtain the wavefunction of the unive
rse using wormhole dominance proposal. Using a prescription for time we obt
ain the,Schrodinger-Wheeler-DeWitt equation without any reference to WD equ
ation and WKB ansatz for WD wavefunction. It is found that the Hartle-Hawki
ng or wormhole-dominated boundary conditions serve as a seed for inflation
as well as for Gaussian type ansatz to Schrodinger-Wheeler-DeWitt equation.