Warping effects in strongly perturbed metrics
Marco Frasca, Riccardo Maria Liberati, Massimiliano Rossi

TL;DR
This paper presents an exact solution for the leading order Einstein equations under strong perturbations, revealing an exponential warp factor affecting the 4-velocity in a spherically symmetric Schwarzschild metric.
Contribution
It provides a novel exact solution for strongly perturbed Einstein equations, demonstrating the warp effect on 4-velocity in spherical symmetry.
Findings
Warp factor always exceeds one
Exact solution for the leading order Einstein equations
Numerical examples illustrating the warp effect
Abstract
A technique devised some years ago permits to study a theory in a regime of strong perturbations. This translates into a gradient expansion that, at the leading order, can recover the BKL solution in general relativity. We solve exactly the leading order Einstein equations in a spherical symmetric case, assuming a Schwarzschild metric under the effect of a time-dependent perturbation, and we show that the 4-velocity in such a case is multiplied by an exponential warp factor when the perturbation is properly applied. This factor is always greater than one. We will give a closed form solution of this factor for a simple case. Some numerical examples are also given.
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