Astronomy and Astrophysics – Astrophysics
Scientific paper
2008-02-21
Phys.Rev.D77:123515,2008
Astronomy and Astrophysics
Astrophysics
9 pages, 4 figures. New comments and references included. Final version to appear in Phys.Rev. D
Scientific paper
10.1103/PhysRevD.77.123515
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.
Dobado Antonio
la Cruz-Dombriz A. de
Maroto Antonio L.
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