Inverse problem - reconstruction of dark energy models

Abstract

We review how we can construct the gravity models which reproduces the arbitrary development of the universe. We consider the reconstruction in the Einstein gravity coupled with generalized perfect fluid, scalar-Einstein gravity, scalar-Einstein-Gauss-Bonnet gravity, Einstein-$F(G)$-gravity, and $F(R)$-gravity. Very explicit formulas are given to reconstruct the models, which could be used when we find the detailed data of the development of the universe by future observations. Especially we find the formulas using e-foldings, which has a direct relation with observed redshift. As long as we observe the time development of the Hubble rate $H$, there exists a variety of models describing the arbitrary development of universe.

LaTeX 11 pages, references are added, to appear in Proceedings of International Workshop on Dark Matter, Dark Energy and Matter-Antimatter Asymmetry, National Tsing Hua University, Hsinchu, Taiwan, November 20-21, 2009

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• Precision cosmology with Padé rational approximations: theoretical predictions versus observational limits
• Anisotropic Compact Stars in $f(G)$ Gravity
• The unification of inflation and late-time acceleration in the frame of $k$-essence
• Breaking the cosmological background degeneracy by two-fluid perturbations in f(R) gravity
• Hybrid star within $f(\mathcal{G})$ gravity