Post-Newtonian cosmological dynamics of plane-parallel perturbations and back-reaction
Eleonora Villa, Sabino Matarrese, Davide Maino

TL;DR
This paper develops a post-Newtonian framework for analyzing non-linear relativistic cosmological dynamics of plane-parallel dust perturbations, extending the Zel'dovich approximation to include relativistic effects and assessing back-reaction.
Contribution
It introduces an exact post-Newtonian extension of the Zel'dovich solution for plane-parallel perturbations, incorporating relativistic effects into cosmological structure formation models.
Findings
Derived the exact post-Newtonian metric for plane-parallel perturbations.
Extended the Zel'dovich approximation to include relativistic corrections.
Estimated relativistic back-reaction effects on cosmic expansion.
Abstract
We study the general relativistic non-linear dynamics of self-gravitating irrotational dust in a cosmological setting, adopting the comoving and synchronous gauge, where all the equations can be written in terms of the metric tensor of spatial hyper-surfaces orthogonal to the fluid flow. Performing an expansion in inverse powers of the speed of light, we obtain the post-Newtonian equations, which yield the lowest-order relativistic effects arising during the non-linear evolution. We then specialize our analysis to globally plane-parallel configurations, i.e. to the case where the initial perturbation field depends on a single coordinate. The leading order of our expansion, corresponding to the "Newtonian background", is the Zel'dovich approximation, which, for plane-parallel perturbations in the Newtonian limit, represents an exact solution. This allows us to find the exact analytical…
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