arXiv · hep-th/9912192
Bianchi Type I Cosmology in N=2, D=5 Supergravity
Abstract
The dynamics and evolution of Bianchi type I space-times is considered in the framework of the four-dimensional truncation of a reduced theory obtained from the N=2,D=5 supergravity. The general solution of the gravitational field equations can be represented in an exact parametric form. All solutions have a singular behavior at the initial/final moment, except when the space-time geometry reduces to the isotropic flat case. Generically the obtained cosmological models describe an anisotropic, expanding or collapsing, singular Universe with a non-inflationary evolution for all times.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Chiang-Mei Chen, T. Harko, M. K. Mak. 2000-02-27. Bianchi Type I Cosmology in N=2, D=5 Supergravity. https://doi.org/10.1103/physrevd.61.104017
Cite the original work for its findings. Save a collection to share your selection of sources.