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Scale dependence of cosmological backreaction · Around

2007

Scale dependence of cosmological backreaction

Li, Nan, Schwarz, Dominik J.

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Due to the non-commutation of spatial averaging and temporal evolution, inhomogeneities and anisotropies (cosmic structures) influence the evolution of the averaged Universe via the cosmological backreaction mechanism.

We study the backreaction effect as a function of averaging scale in a perturbative approach up to higher orders.
We calculate the hierarchy of the critical scales, at which 10% effects show up from averaging at different orders.
The dominant contribution comes from the averaged spatial curvature, observable up to scales of 200 Mpc.

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