On the evolution of density perturbations in f(R) theories of gravity

Abstract

In the context of $f(R)$ theories of gravity, we study the evolution of scalar cosmological perturbations in the metric formalism. Using a completely general procedure, we find the exact fourth-order differential equation for the matter density perturbations in the longitudinal gauge. In the case of sub-Hubble modes, the expression reduces to a second-order equation which is compared with the standard (quasi-static) equation used in the literature. We show that for general $f(R)$ functions the quasi-static approximation is not justified. However, for those functions adequately describing the present phase of accelerated expansion and satisfying local gravity tests, it provides a correct description for the evolution of perturbations.

9 pages, 4 figures. New comments and references included. Final version to appear in Phys.Rev. D

References in corpus (4)

• Models of f(R) Cosmic Acceleration that Evade Solar-System Tests
• Stability of Cosmological Solution in f(R) Models of Gravity
• The evolution of density perturbations in f(R) gravity
• Density perturbations in f(R) gravity theories in metric and Palatini formalisms