Large-scale perturbations on the brane and the isotropy of the cosmological singularity
arXiv:hep-th/0408092 · doi:10.1103/PhysRevD.70.123517
Abstract
We present the complete set of propagation and constraint equations for the kinematic and non-local first order quantities which describe general linear inhomogeneous and anisotropic perturbations of a flat FRW braneworld with vanishing cosmological constant and decompose them in the standard way into their scalar, vector and tensor contributions. A detailed analysis of the perturbation dynamics is performed using dimensionless variables that are specially tailored for the different regimes of interest; namely, the low energy GR regime, the high energy regime and the dark energy regime. Tables are presented for the evolution of all the physical quantities, making it easy to do a detailed comparison of the past asymptotic behaviour of the perturbations of these models. We find results that exactly match those obtained in the analysis of the spatially inhomogeneous braneworld cosmologies presented recently; i.e., that isotropization towards the model occurs for .
arXiv comment13 pages, revtex4
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