2011

Observational constraints on inhomogeneous cosmological models without dark energy

Marra, Valerio, Notari, Alessio

Understand

It has been proposed that the observed dark energy can be explained away by the effect of large-scale nonlinear inhomogeneities.

In the present paper we discuss how observations constrain cosmological models featuring large voids.
We start by considering Copernican models, in which the observer is not occupying a special position and homogeneity is preserved on a very large scale.
We show how these models, at least in their current realizations, are constrained to give small, but perhaps not negligible in certain contexts, corrections to the cosmological observables.

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