We study backreaction in dust universes using exact equations which do not rely on perturbation theory, concentrating on theoretical and observational constraints. In particular, we discuss the recent suggestion (in hep-th/0503117) that superhorizon perturbations could explain present-day accelerated expansion as a useful example which can be ruled out. We note that a backreaction explanation of late-time acceleration will have to involve spatial curvature and subhorizon perturbations.Peer reviewe
Li N. Cosmological backreaction : from the local Hubble expansion rate to dark energy. Bielefeld (Ge...
A simple discussion on the backreaction of inhomogeneities in cosmology, focusing on the possibility...
We investigate the recent suggestions by Barausse et al. and Kolb et al. that the acceleration of th...
We study backreaction in dust universes using exact equations which do not rely on perturbation theo...
One possible explanation for the present observed acceleration of the Universe is the breakdown of h...
Abstract The spatially averaged inhomogeneous Universe includes a kinematical backreaction term $${\...
We consider the effect of inhomogeneities on the expansion of the Einstein–de Sitter universe. We fi...
In the context of second order perturbation theory, cosmological backreaction is seen to rescale bot...
We discuss the physics of backreaction-driven accelerated expansion. We explain how large-scale smoo...
We study backreaction analytically using the parabolic Lemaître–Tolman–Bondi universe as a toy model...
We review the effect of the formation of nonlinear structures on the expansion rate, spatial curvatu...
If the FRW metric is a good approximation on large scales, then the distance and the expansion rate,...
The predictions of homogeneous and isotropic cosmological models with ordinary matter and gravity ar...
It has recently been suggested that the acceleration of the Universe can be explained as the backrea...
Cosmological backreaction has been suggested as an explanation of dark energy and is heavily dispute...
Li N. Cosmological backreaction : from the local Hubble expansion rate to dark energy. Bielefeld (Ge...
A simple discussion on the backreaction of inhomogeneities in cosmology, focusing on the possibility...
We investigate the recent suggestions by Barausse et al. and Kolb et al. that the acceleration of th...
We study backreaction in dust universes using exact equations which do not rely on perturbation theo...
One possible explanation for the present observed acceleration of the Universe is the breakdown of h...
Abstract The spatially averaged inhomogeneous Universe includes a kinematical backreaction term $${\...
We consider the effect of inhomogeneities on the expansion of the Einstein–de Sitter universe. We fi...
In the context of second order perturbation theory, cosmological backreaction is seen to rescale bot...
We discuss the physics of backreaction-driven accelerated expansion. We explain how large-scale smoo...
We study backreaction analytically using the parabolic Lemaître–Tolman–Bondi universe as a toy model...
We review the effect of the formation of nonlinear structures on the expansion rate, spatial curvatu...
If the FRW metric is a good approximation on large scales, then the distance and the expansion rate,...
The predictions of homogeneous and isotropic cosmological models with ordinary matter and gravity ar...
It has recently been suggested that the acceleration of the Universe can be explained as the backrea...
Cosmological backreaction has been suggested as an explanation of dark energy and is heavily dispute...
Li N. Cosmological backreaction : from the local Hubble expansion rate to dark energy. Bielefeld (Ge...
A simple discussion on the backreaction of inhomogeneities in cosmology, focusing on the possibility...
We investigate the recent suggestions by Barausse et al. and Kolb et al. that the acceleration of th...