The viability of theories with matter coupled to the Ricci scalar
arXiv:0805.1160 · doi:10.1016/j.physletb.2008.05.050
Abstract
Recently there has been a proposal for modified gravitational f(R) actions which include a direct coupling between the matter action and the Ricci scalar, R. Of particular interest is the specific case where both the action and the coupling are linear in R. It is shown that such an action leads to a theory of gravity which includes higher order derivatives of the matter fields without introducing more dynamics in the gravity sector and, therefore, cannot be a viable theory for gravitation.
typos corrected, published version
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- Nonminimal coupling of perfect fluids to curvature
- Modified gravity with arbitrary coupling between matter and geometry
- Generalized curvature-matter couplings in modified gravity
- Nonminimal curvature-matter coupled wormholes with matter satisfying the null energy condition
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- Bouncing Cosmologies in Palatini Gravity
- Surface singularities in Eddington-inspired Born-Infeld gravity
- On the consistency of universally non-minimally coupled theories
- Extended gravity with generalized scalar field and kinetic term dependences
- Galactic rotation curves in modified gravity with non-minimal coupling between matter and geometry
- Palatini formulation of modified gravity with a nonminimal curvature-matter coupling
- Initial and final de Sitter universes from modified gravity
- Geodesic deviation, Raychaudhuri equation, and tidal forces in modified gravity with an arbitrary curvature-matter coupling
- Dynamical Aspects of Generalized Palatini Theories of Gravity
- Re-examination of Polytropic Spheres in Palatini f(R) Gravity
- Noncommutative geometry inspired black holes in Rastall gravity
- Gödel-type universes in Palatini f(R) gravity
- Future dynamics in f(R) theories
- Cassini and extra force constraints to nonminimally coupled gravity with screening mechanism
- Observational constraints on generic models of non-minimal curvature-matter coupling
- The ghost of vector fields in compact stars