Quantum Evolution of the Bianchi Type I Model

Abstract

The behaviour of the flat anisotropic model of the Universe with a scalar field is explored within the framework of quantum cosmology. The principal moment of the account of an anisotropy is the presence either negative potential barrier or positive repelling wall. In the first case occur the above barrier reflection of the wave function of the Universe, in the second one there is bounce off a potential wall. The further evolution of the Universe represents an exponential inflating with fast losses of an anisotropy and approach to the standard cosmological scenario.

Latex, 18 pages, 5 figures

References in corpus (1)

• Open Inflation Without False Vacua

Cited by in corpus (4)

• Classical and Quantum Features of the Mixmaster Singularity
• Bianchi type I model with two interacting scalar fields
• Cosmological volume acceleration in dust epoch: using scaling solutions and variable cosmological term $\Lambda (t)$ within an anisotropic cosmological model
• Tunneling of the Closed Friedmann Universe with Generation of Scalar Waves