paper

Cosmological equivalence between the Finsler-Randers space-time and the DGP gravity model

arXiv:1301.4327 · doi:10.1103/PhysRevD.87.043506

Abstract

We perform a detailed comparison between the Finsler-Randers cosmological model and the Dvali, Gabadadze and Porrati braneworld model. If we assume that the spatial curvature is strictly equal to zero then we prove the following interesting proposition: {\it despite the fact that the current cosmological models have a completely different geometrical origin they share exactly the same Hubble expansion}. This implies that the Finsler-Randers model is cosmologically equivalent with that of the DGP model as far as the cosmic expansion is concerned. At the perturbative level we find that the Finsler-Randers growth index of matter perturbations is which is somewhat lower than that of DGP gravity () implying that the growth factor of the Finsler-Randers model is slightly different () from the one provided by the DGP gravity model.

6 pages, 2 figures, accepted for publication in Phys. Rev. D. (typos corrected, published version)

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