It has recently been suggested that the acceleration of the Universe can be explained as the backreaction effect of superhorizon perturbations using second order perturbation theory. If this mechanism is correct, it should also apply to a hypothetical, gedanken universe in which the subhorizon perturbations are absent. In such a gedanken universe it is possible to compute the deceleration parameter $q_0$ measured by comoving observers using local covariant Taylor expansions rather than using second order perturbation theory. The result indicates that second order corrections to $q_0$ are present, but shows that any negative corrections to $q_0$ are constrained to be of order the square the peculiar velocity on Hubble scales today. We argue ...
In the context of second order perturbation theory, cosmological backreaction is seen to rescale bot...
The analysis of the data from the distant supernovae (A.Riess et al, Astron.J. {\bf 116}, 1009, (198...
In this paper we consider the relation between the volume deceleration parameter obtained within the...
We investigate the recent suggestions by Barausse et al. and Kolb et al. that the acceleration of th...
We elaborate on the proposal that the observed acceleration of the Universe is the result of the bac...
A new cosmological era began with the discovery of accelerating expansion of the Universe. The devia...
The possible slowing down of cosmic acceleration was widely studied. However, judgment on this effec...
We study backreaction in dust universes using exact equations which do not rely on perturbation theo...
We study the accelerated expansion phase of the universe by using the kinematic approach. In particu...
Large-scale bulk peculiar motions introduce a characteristic length scale, inside which the local ki...
AbstractThe energy conditions provide a very promising model-independent study of the current accele...
We consider light propagation in an inhomogeneous irrotational dust universe with vanishing cosmolog...
The existence of cosmological perturbations of wavelength larger than the Hubble radius is a generic...
We introduce a new asymptotic ansatz for spherical perturbations of the Standard Model of C...
It is a well-known fact that the Newtonian description of dynamics within Galaxies for its known mat...
In the context of second order perturbation theory, cosmological backreaction is seen to rescale bot...
The analysis of the data from the distant supernovae (A.Riess et al, Astron.J. {\bf 116}, 1009, (198...
In this paper we consider the relation between the volume deceleration parameter obtained within the...
We investigate the recent suggestions by Barausse et al. and Kolb et al. that the acceleration of th...
We elaborate on the proposal that the observed acceleration of the Universe is the result of the bac...
A new cosmological era began with the discovery of accelerating expansion of the Universe. The devia...
The possible slowing down of cosmic acceleration was widely studied. However, judgment on this effec...
We study backreaction in dust universes using exact equations which do not rely on perturbation theo...
We study the accelerated expansion phase of the universe by using the kinematic approach. In particu...
Large-scale bulk peculiar motions introduce a characteristic length scale, inside which the local ki...
AbstractThe energy conditions provide a very promising model-independent study of the current accele...
We consider light propagation in an inhomogeneous irrotational dust universe with vanishing cosmolog...
The existence of cosmological perturbations of wavelength larger than the Hubble radius is a generic...
We introduce a new asymptotic ansatz for spherical perturbations of the Standard Model of C...
It is a well-known fact that the Newtonian description of dynamics within Galaxies for its known mat...
In the context of second order perturbation theory, cosmological backreaction is seen to rescale bot...
The analysis of the data from the distant supernovae (A.Riess et al, Astron.J. {\bf 116}, 1009, (198...
In this paper we consider the relation between the volume deceleration parameter obtained within the...