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Observations of the expansion rate of the universe at late times disagree by a factor of 1.5-2 with the prediction of homogeneous and isotropic models based on ordinary matter and gravity.
The statistics of peaks of Gaussian random fields
Bardeen J M, Bond J R, Kaiser N and Szalay A S, · 1986
Earlier work this paper cites.
Relativistic cosmology: its nature, aims and problems
Ellis G F R, · 1987
Earlier work this paper cites.
Structure formation in the universe
Padmanabhan T, · 1993
Earlier work this paper cites.
The Structure of Scientific Revolutions
Kuhn T S, · 1996
Earlier work this paper cites.
Moon-Earth-Sun: The oldest three-body problem
Gutzwiller M C, · 1998
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On average properties of inhomogeneous fluids in general relativity I: dust cosmologies
Buchert T, · 2000
Cited alongside, same era.
Dark energy from backreaction
Räsänen S, · 2004
Cited alongside, same era.
Cosmic homogeneity demonstrated with luminous red galaxies
Hogg D W et al · 2005
Cited alongside, same era.
The universe seen at different scales
Ellis G F R and Buchert T, · 2005
Later among the works it cites.
Cosmological acceleration from structure formation
Räsänen S, · 2006
Later among the works it cites.
Fluctuations of the luminosity distance
Bonvin C, Durrer R and Gasparini M A, · 2006
Later among the works it cites.
Evaluating backreaction with the peak model of structure formation
Räsänen S, · 2008
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