Dynamics of perturbations in Gurzadyan-Xue cosmological models
arXiv:astro-ph/0610197 · doi:10.1142/S021827180801195X
Abstract
Perturbation theory within Newtonian approximation is presented for cosmological models with varying physical constants. Analytical solutions for perturbations dynamics are obtained for each Gurzadyan-Xue model with pressureless matter and radiation. We found that perturbations grow during entire expansion within GX models, including curvature- and vacuum-dominated stage when they cease to grow in the standard cosmological model.
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