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- Inhomogeneous_cosmology abstract "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. a homogeneous metric, only holds as long as the perturbations are not too large, and N-body simulations use Newtonian gravity which is only a good approximation when speeds are low and gravitational fields are weak.".
- Inhomogeneous_cosmology wikiPageID "11522684".
- Inhomogeneous_cosmology wikiPageLength "2275".
- Inhomogeneous_cosmology wikiPageOutDegree "11".
- Inhomogeneous_cosmology wikiPageRevisionID "682393902".
- Inhomogeneous_cosmology wikiPageWikiLink Back-reaction.
- Inhomogeneous_cosmology wikiPageWikiLink Category:Physical_cosmology.
- Inhomogeneous_cosmology wikiPageWikiLink Dark_energy.
- Inhomogeneous_cosmology wikiPageWikiLink Einstein_field_equations.
- Inhomogeneous_cosmology wikiPageWikiLink Einsteins_field_equations.
- Inhomogeneous_cosmology wikiPageWikiLink Homogeneity_and_heterogeneity.
- Inhomogeneous_cosmology wikiPageWikiLink Kantowski-Sachs_metric.
- Inhomogeneous_cosmology wikiPageWikiLink Lemaître–Tolman_metric.
- Inhomogeneous_cosmology wikiPageWikiLink Metric_tensor_(general_relativity).
- Inhomogeneous_cosmology wikiPageWikiLink Perturbation_theory.
- Inhomogeneous_cosmology wikiPageWikiLink Physical_cosmology.
- Inhomogeneous_cosmology wikiPageWikiLink Stephani_metric.
- Inhomogeneous_cosmology wikiPageWikiLinkText "Inhomogeneous cosmology".
- Inhomogeneous_cosmology wikiPageWikiLinkText "inhomogeneous cosmological model".
- Inhomogeneous_cosmology wikiPageWikiLinkText "inhomogeneous cosmological models".
- Inhomogeneous_cosmology wikiPageWikiLinkText "inhomogeneous cosmologies".
- Inhomogeneous_cosmology wikiPageWikiLinkText "inhomogeneous universe".
- Inhomogeneous_cosmology hasPhotoCollection Inhomogeneous_cosmology.
- Inhomogeneous_cosmology wikiPageUsesTemplate Template:Reflist.
- Inhomogeneous_cosmology subject Category:Physical_cosmology.
- Inhomogeneous_cosmology type Physic.
- Inhomogeneous_cosmology type Sub-discipline.
- Inhomogeneous_cosmology comment "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.".
- Inhomogeneous_cosmology label "Inhomogeneous cosmology".
- Inhomogeneous_cosmology sameAs m.02rgrmd.
- Inhomogeneous_cosmology sameAs Q6033847.
- Inhomogeneous_cosmology sameAs Q6033847.
- Inhomogeneous_cosmology wasDerivedFrom Inhomogeneous_cosmology?oldid=682393902.
- Inhomogeneous_cosmology isPrimaryTopicOf Inhomogeneous_cosmology.