F(R) gravity in purely affine formulation
arXiv:0706.4474 · doi:10.1142/S0217751X08039773
Abstract
The purely affine, metric-affine and purely metric formulation of general relativity are dynamically equivalent and the relation between them is analogous to the Legendre relation between the Lagrangian and Hamiltonian dynamics. We show that one cannot construct a dynamically equivalent, purely affine Lagrangian from a metric-affine or metric F(R) Lagrangian, nonlinear in the curvature scalar. Thus the equivalence between the purely affine picture and the two other formulations does not hold for metric-affine and metric theories of gravity with a nonlinear dependence on the curvature, i.e. F(R) gravity does not have a purely affine formulation. We also show that this equivalence is restored if the metric tensor is conformally transformed from the Jordan to the Einstein frame, in which F(R) gravity turns into general relativity with a scalar field. This peculiar behavior of general relativity, among relativistic theories of gravitation, with respect to purely affine, metric-affine and purely metric variation could indicate the physicality of the Einstein frame. On the other hand, it could explain why this theory cannot interpolate among phenomenological behaviors at different scales.
7 pages; published version
References in corpus (17)
- Models of f(R) Cosmic Acceleration that Evade Solar-System Tests
- Modified f(R) gravity consistent with realistic cosmology: from matter dominated epoch to dark energy universe
- Cosmological viability of f(R)-gravity as an ideal fluid and its compatibility with a matter dominated phase
- Conditions for the cosmological viability of f(R) dark energy models
- Metric-affine f(R) theories of gravity
- Limit to General Relativity in f(R) theories of gravity
- Phantom crossing, equation-of-state singularities, and local gravity constraints in f(R) models
- The (pseudo)issue of the conformal frame revisited
- Solar System experiments do not yet veto modified gravity models
- The evolution of density perturbations in f(R) gravity
- f(R) gravity theories in Palatini formalism: cosmological dynamics and observational constraints
- Cosmological Constraints on f(R) Acceleration Models
- Stability of the Einstein static universe in f(R) gravity
- Violation of the Equivalence Principle in Modified Theories of Gravity
- Interacting dark energy in gravity
- Cosmological perturbations in Palatini modified gravity
- The Maxwell Lagrangian in purely affine gravity