Schroedinger Wheeler-DeWitt Equation In Multidimensional Cosmology
arXiv:gr-qc/9906009 · doi:10.1142/S0218271801001372
Abstract
We study multidimensional cosmology to obtain the wavefunction of the universe using wormhole dominance proposal. Using a prescription for time we obtain the Schroedinger-Wheeler-DeWitt equation without any reference to WD equation and WKB ansatz for WD wavefunction. It is found that the Hartle-Hawking or wormhole-dominated boundary conditions serve as a seed for inflation as well as for Gaussian type ansatz to Schroedinger-Wheeler-DeWitt equation.
10 Pages, LaTeX, no figure