arXiv · gr-qc/9305016
Initial conditions and unitarity in unimodular quantum cosmology
Abstract
We consider quantization of the positive curvature Friedmann cosmology in the unimodular modification of Einstein's theory, in which the spacetime four-volume appears as an explicit time variable. The Hamiltonian admits self-adjoint extensions that give unitary evolution in the Hilbert space associated with the Schrödinger equation. The semiclassical estimate to the no-boundary wave function of Hartle and Hawking is found. If this estimate is accurate, there is a continuous flux of probability into the configuration space from vanishing three-volume, and the no-boundary wave function evolves nonunitarily. Generalizations of these results hold in a class of anisotropic cosmologies. (Talk given at the 5th Canadian Conference on General Relativity and Relativistic Astrophysics, Waterloo, Ontario, Canada, May 1993.)
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Alan Daughton, Jorma Louko, Rafael D. Sorkin. 1993-05-18. Initial conditions and unitarity in unimodular quantum cosmology. https://arxiv.org/abs/gr-qc/9305016
Cite the original work for its findings. Save a collection to share your selection of sources.