Robust approach to f(R) gravity
arXiv:1006.5747 · doi:10.1103/PhysRevD.83.024039
Abstract
We consider metric f(R) theories of gravity without mapping them to their scalar-tensor counterpart, but using the Ricci scalar itself as an "extra" degree of freedom. This approach avoids then the introduction of a scalar-field potential that might be ill defined (not single valued). In order to explicitly show the usefulness of this method, we focus on static and spherically symmetric spacetimes and deal with the recent controversy about the existence of extended relativistic objects in certain class of f(R) models.
5 pages; 2 figures (4 panels); minor corrections to match the published version; panel added
References in corpus (21)
- f(R) Theories Of Gravity
- f(R) theories
- Introduction to Modified Gravity and Gravitational Alternative for Dark Energy
- Is Cosmic Speed-Up Due to New Gravitational Physics?
- Modified gravity with negative and positive powers of the curvature: unification of the inflation and of the cosmic acceleration
- Disappearing cosmological constant in f(R) gravity
- Class of viable modified gravities describing inflation and the onset of accelerated expansion
- Can modified gravity explain accelerated cosmic expansion?
- The future evolution and finite-time singularities in -gravity unifying the inflation and cosmic acceleration
- A Singularity Problem with f(R) Dark Energy
- Relativistic stars in f(R) gravity, and absence thereof
- The existence of relativistic stars in f(R) gravity
- Relativistic stars in f(R) and scalar-tensor theories
- Relativistic stars in f(R) gravity
- Can higher curvature corrections cure the singularity problem in f(R) gravity?
- Power-law cosmic expansion in f(R) gravity models
- Viable Singularity-Free f(R) Gravity Without a Cosmological Constant
- Delicate f(R) gravity models with disappearing cosmological constant and observational constraints on the model parameters
- A new framework for studying spherically symmetric static solutions in f(R) gravity
- The Cauchy problem of f(R) gravity
- Modified gravity as realistic candidate for dark energy, inflation and dark matter
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