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Dynamics of scalar perturbations in f(R,T) gravity | F. G. Alvarenga
; A. de la Cruz-Dombriz
; M. J. S. Houndjo
; M. E. Rodrigues
; D. Sáez-Gómez
; | Date: |
7 Feb 2013 | Abstract: | In the context of f(R,T) theories of gravity, we study the evolution of
scalar cosmological perturbations in the metric formalism. According to
restrictions on the background evolution, a specific model within these
theories is assumed in order to guarantee the standard continuity equation.
Using a completely general procedure, we find the complete set of differential
equations for the matter density perturbations. 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,T) Lagrangians the quasi-static approximation yields to very
different results from the ones derived in the frame of the Concordance Lambda
CDM model. | Source: | arXiv, 1302.1866 | Services: | Forum | Review | PDF | Favorites |
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