Exponential-Potential Scalar Field Universes II: The Inhomogeneous Models

Details Exponential-Potential Scalar Field Universes II: The Inhomogeneous Models Exponential-Potential Scalar Field Universes II: The Inhomogeneous Models

1993-09-14

arxiv.org/abs/gr-qc/9309014v1

Phys.Rev.D48:4669-4675,1993

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

18 pages, Plain LaTeX, 2 Figures to be sent on request, to appear in Phys. Rev. D., report 2

Scientific paper

10.1103/PhysRevD.48.4669

We obtain exact solutions for the Einstein equations with an exponential-potential scalar field (\(V=\Lambda e^{k\phi}\)) which represent simple inhomogeneous generalizations of Bianchi I cosmologies. Studying these equations numerically we find that in most of the cases there is a certain period of inflationary behaviour for \(k^2<2\). We as well find that for \(k^2>2\) the solutions homogenize generically at late times. Yet, {\em none of the solutions} isotropize. For some particular values of the integration constants we find a multiple inflationary behaviour for which the deceleration and the inflationary phases interchange each other several times during the history of the model.

Affiliated with

Also associated with

No associations

Rating

Exponential-Potential Scalar Field Universes II: The Inhomogeneous Models 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 Exponential-Potential Scalar Field Universes II: The Inhomogeneous Models, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Exponential-Potential Scalar Field Universes II: The Inhomogeneous Models will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-98207