Cosmography of f(R) - brane cosmology
arXiv:1010.1547 · doi:10.1103/PhysRevD.82.103526
Abstract
Cosmography is a useful tool to constrain cosmological models, in particular dark energy models. In the case of modified theories of gravity, where the equations of motion are generally quite complicated, cosmography can contribute to select realistic models without imposing arbitrary choices a priori. Indeed, its reliability is based on the assumptions that the universe is homogeneous and isotropic on large scale and luminosity distance can be "tracked" by the derivative series of the scale factor a(t). We apply this approach to induced gravity brane-world models where an f(R)-term is present in the brane effective action. The virtue of the model is to self-accelerate the normal and healthy DGP branch once the f(R)-term deviates from the Hilbert-Einstein action. We show that the model, coming from a fundamental theory, is consistent with the LCDM scenario at low redshift. We finally estimate the cosmographic parameters fitting the Union2 Type Ia Supernovae (SNeIa) dataset and the distance priors from Baryon Acoustic Oscillations (BAO) and then provide constraints on the present day values of f(R) and its second and third derivatives.
9 pages, 3 figures, to appear in Phys. Rev. D
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- Eddington-Born-Infeld cosmology: a cosmographic approach, a tale of doomsdays and the fate of bound structures
- Observational Constraints and Cosmological Implications of Scalar-Tensor Gravity
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- Transit String Dark Energy Models in Gravity
- ΛCDM suitably embedded in f(R) with a non-minimal coupling to matter
- Brane cosmology in teleparallel and gravity
- Cosmography in F(G) modified gravity