The fate of (phantom) dark energy universe with string curvature corrections

Details The fate of (phantom) dark energy universe with string curvature corrections The fate of (phantom) dark energy universe with string curvature corrections

2005-04-19

arxiv.org/abs/hep-th/0504154v2

Phys.Lett.B619:193,2005

Physics

High Energy Physics

High Energy Physics - Theory

6 pages and 3 figures, discussion on dynamically evolving dilaton and modulus included, references added, version to appear in

Scientific paper

10.1016/j.physletb.2005.06.017

We study the evolution of (phantom) dark energy universe by taking into account the higher-order string corrections to Einstein-Hilbert action with a fixed dilaton. While the presence of a cosmological constant gives stable de-Sitter fixed points in the cases of heterotic and bosonic strings, no stable de-Sitter solutions exist when a phantom fluid is present. We find that the universe can exhibit a Big Crunch singularity with a finite time for type II string, whereas it reaches a Big Rip singularity for heterotic and bosonic strings. Thus the fate of dark energy universe crucially depends upon the type of string theory under consideration.

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