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Cosmological observational analysis frequently assumes that the Universe is spatially flat.
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2005
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Cambridge, UK: Cambridge University Press, Nov., 2006
A. Krasiński, Inhomogeneous Cosmological Models · 2006
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S. Räsänen, Accelerated expansion from structure formation
2006
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2006
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T. Kai, H. Kozaki, K. Nakao, Y. Nambu, and C. Yoo, Can Inhomogeneities Accelerate the Cosmic Volume Expansion?
2007
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K. Bolejko, Evolution of cosmic structures in different environments in the quasispherical Szekeres model
2007
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C. G. Tsagas, A. Challinor, and R. Maartens, Relativistic cosmology and large-scale structure
2008
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A. Krasiński, Geometry and topology of the quasiplane Szekeres model
2008
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2014
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2015
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M. A. Nazer and D. L. Wiltshire, Cosmic microwave background anisotropies in the timescape cosmology
2015
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2015
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2015
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2015
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2016
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2016
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2016
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P. C. Stichel, Cosmological model with dynamical curvature
2016
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2016
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2016
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2016
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2017
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K. Bolejko, Emergence of spatial curvature
2017
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2017
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K. Bolejko, Cosmological backreaction within the Szekeres model and emergence of spatial curvature
2017
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G. Rácz, L. Dobos, R. Beck, I. Szapudi, and I. Csabai, Concordance cosmology without dark energy
2017
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2017
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H. J. Macpherson, P. D. Lasky, and D. J. Price, Inhomogeneous cosmology with numerical relativity
2017
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2018
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2018
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B. F. Roukema, Replacing dark energy by silent virialisation
2018
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K. Bolejko, Relativistic numerical cosmology with silent universes
2018
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2018
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2018
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2018
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