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arXiv · 1104.1181

The cosmology of an holographic induced gravity model with curvature effects

Mariam Bouhmadi-Lopez·Ahmed Errahmani·Taoufiq Ouali
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Abstract

We present an holographic model of the Dvali-Gabadadze-Porrati scenario with a Gauss-Bonnet term in the bulk. We concentrate on the solution that generalises the normal Dvali-Gabadadze-Porrati branch. It is well known that this branch cannot describe the late-time acceleration of the universe even with the inclusion of a Gauss-Bonnet term. Here, we show that this branch in the presence of a Gauss-Bonnet curvature effect and an holographic dark energy with the Hubble scale as the infra-red cutoff can describe the late-time acceleration of the universe. It is worthwhile to stress that such an energy density component cannot do the same job on the normal Dvali-Gabadadze-Porrati branch (without Gauss-Bonnet modifications) nor in a standard 4-dimensional relativistic model. The acceleration on the brane is also presented as being induced through an effective dark energy which corresponds to a balance between the holographic one and geometrical effects encoded through the Hubble parameter.

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Mariam Bouhmadi-Lopez, Ahmed Errahmani, Taoufiq Ouali. 2011-09-19. The cosmology of an holographic induced gravity model with curvature effects. https://doi.org/10.1103/physrevd.84.083508

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