Dark energy problem: from phantom theory to modified Gauss-Bonnet gravity

Details Dark energy problem: from phantom theory to modified Gauss-Bonnet gravity Dark energy problem: from phantom theory to modified Gauss-Bonnet gravity

2005-10-21

arxiv.org/abs/hep-th/0510183v2

J.Phys.A39:6627-6634,2006

Physics

High Energy Physics

High Energy Physics - Theory

LaTeX 8 pages, prepared for the Proceedings of QFEXT'05, minor correctons, references added

Scientific paper

10.1088/0305-4470/39/21/S62

The solution of dark energy problem in the models without scalars is presented. It is shown that late-time accelerating cosmology may be generated by the ideal fluid with some implicit equation of state. The universe evolution within modified Gauss-Bonnet gravity is considered. It is demonstrated that such gravitational approach may predict the (quintessential, cosmological constant or transient phantom) acceleration of the late-time universe with natural transiton from deceleration to acceleration (or from non-phantom to phantom era in the last case).

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