Journal
PHYSICAL REVIEW LETTERS
Volume 90, Issue 3, Pages -Publisher
AMERICAN PHYSICAL SOC
DOI: 10.1103/PhysRevLett.90.031101
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In the context of the averaging problem in relativistic cosmology, we provide a key to the interpretation of cosmological parameters by taking into account the actual inhomogeneous geometry of the Universe. We discuss the relation between bare cosmological parameters determining the cosmological model and the parameters interpreted by observers with a Friedmannian bias, which are dressed by the smoothed-out geometrical inhomogeneities of the surveyed spatial region.
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