pith. sign in

arxiv: gr-qc/9906009 · v1 · pith:VS2U2DEXnew · submitted 1999-06-03 · 🌀 gr-qc

Schroedinger Wheeler-DeWitt Equation In Multidimensional Cosmology

classification 🌀 gr-qc
keywords equationansatzcosmologymultidimensionalobtainschroedinger-wheeler-dewittwavefunctionboundary
0
0 comments X
read the original 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.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.