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Dark Energy and Dark Matter: Observations, Experiments and Theories
E. Pécontal, T. Buchert, Ph. Di Stefano and Y. Copin (eds)
EAS Publications Series, 36 (2009) 83-90
DOI: 10.1051/eas/0936010
Signatures of cosmological backreaction
N. Li and D.J. SchwarzFakultät für Physik, Universität Bielefeld, Universitätsstraße 25, 33615 Bielefeld, Germany; ;
li@physik.uni-bielefeld.de
dschwarz@physik.uni-bielefeld.de
Published online: 30 May 2009
Abstract
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
effects show up from averaging at different
orders, observable up to scales of
. The cosmic
variance of the local Hubble rate is
for spherical
regions of radius 40
. We compare our results to
the Hubble Space Telescope (HST) Key Project data.
© EAS, EDP Sciences 2009
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