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DBpedia 2015-10

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Matches in DBpedia 2015-10 for { ?s ?p "Inhomogeneous cosmology usually means the study of structure in the universe by means of exact solutions of Einstein's field equations (i.e. metrics) or by spatial or spacetime averaging methods. Such models are not homogeneous, but contain enough matter to be possible cosmological models, typically without dark energy, or models of cosmological structures such as voids or galaxy clusters. In contrast, perturbation theory, which deals with small perturbations from e.g."@en }

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