Cosmological viability of f(R)-gravity as an ideal fluid and its compatibility with a matter dominated phase
arXiv:astro-ph/0604431 · doi:10.1016/j.physletb.2006.06.034
Abstract
We show that f(R)-gravity can, in general, give rise to cosmological viable models compatible with a matter-dominated epoch evolving into a late accelerated phase. We discuss the various representations of f(R)-gravity as an ideal fluid or a scalar-tensor gravity theory, taking into account conformal transformations. We point out that mathematical equivalence does not correspond, in several cases, to the physical equivalence of Jordan frame and Einstein frame. Finally, we show that wide classes of f(R)-gravity models, including matter and accelerated phases, can be phenomenologically reconstructed by means of observational data. In principle, any popular quintessence models could be "reframed" as an f(R)-gravity model.
arXiv comment11 pages, 1 figure
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- Hubble Diagrams in the Jordan and Einstein Frames
- Inflationary attractors and gravity
- The general expression for in a charged cylindrical spacetime with diverse dimensions
- Phenomenological modification of horizon temperature
- Asymptotically Schwarzschild solutions in extension of general relativity
- A Matter with an effective EoS interacting with a tachynic field in an accelerating Universe
- An exact solution of the higher-order gravity in standard radiation-dominated era
- Scalar-tensor cosmologies in a minisuperspace formulation: a case study
- Signature of gravity via Lemaître-Tolman-Bondi inhomogeneous perturbations
- Loop-corrected scalar potentials and late-time acceleration in f(R) gravity
- Correspondence between modified gravity and 5D Ricci-flat cosmologies
- Energy momentum tensor of a non-minimally coupled scalar from the equivalence of the Einstein and Jordan frames
- Thermodynamics of irreversible particle creation phenomena and its cosmological consequence
- A Viable model for modified gravity
- f(R) cosmological solutions with varying speed of light
- Accelerating Kaluza-Klein Universe in Modified Theory of Gravitation
- The Coincidence Problem in Holographic f(R) Gravity
- A Note on Gravitational Memory in F(R)-theories and their Equivalent Scalar-Tensor Theories
- Recovery of fluctuation spectrum evolution from tomographic shear spectra
- Density perturbation and cosmological evolution in the presence of magnetic field in gravity models
- Quasar continuum spectrum disfavors black holes with a magnetic monopole charge
- Gravastars in a Non-minimally Coupled Gravity with Electromagnetism
- An effective fluid description of scalar-vector-tensor theories under the sub-horizon and quasi-static approximations
- Energy Conditions in Palatini Approach to Modified Gravity
- On the structural stability of a simple cosmological model in theory of gravity
- Power-law and Logarithmic Entropy Corrected Holographic Dark Energy Models in Brans-Dicke Cosmology with Granda-Oliveros Cut-Off
- Quantum cosmology in teleparallel gravity with a boundary term
- Parametrization of Born-Infeld Type Phantom Dark Energy Model