arXiv · hep-th/9503223
Multidimensional Classical and Quantum Cosmology with Perfect Fluid
Abstract
A cosmological model describing the evolution of n Ricci-flat spaces (n>1) in the presence of 1-component perfect-fluid and minimally coupled scalar field is considered. When the pressures in all spaces are proportional to the density, the Einstein and Wheeler-DeWitt equations are integrated for a large variety of parameters. Classical and quantum wormhole solutions are obtained for negative density. Some special classes of solutions, e.g. solutions with spontaneous and dynamical compactification, exponential and power-law inflations, are singled out. For positive density a third quantized cosmological model is considered and the Planckian spectrum of ``created universes'' is obtained.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
V. D. Ivashchuk, V. N. Melnikov. 2006-12-28. Multidimensional Classical and Quantum Cosmology with Perfect Fluid. https://arxiv.org/abs/hep-th/9503223
Cite the original work for its findings. Save a collection to share your selection of sources.