Bianchi Type I Cosmology in N=2, D=5 Supergravity

Details Bianchi Type I Cosmology in N=2, D=5 Supergravity Bianchi Type I Cosmology in N=2, D=5 Supergravity

1999-12-21

arxiv.org/abs/hep-th/9912192v2

Phys.Rev. D61 (2000) 104017

Physics

High Energy Physics

High Energy Physics - Theory

revised version to appear in PRD

Scientific paper

10.1103/PhysRevD.61.104017

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.

Affiliated with

Also associated with

No associations

Rating

Bianchi Type I Cosmology in N=2, D=5 Supergravity does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Bianchi Type I Cosmology in N=2, D=5 Supergravity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Bianchi Type I Cosmology in N=2, D=5 Supergravity will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-44357