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About: De Sitter–Schwarzschild metric     Goto   Sponge   NotDistinct   Permalink

An Entity of Type : yago:WikicatExactSolutionsInGeneralRelativity, within Data Space : dbpedia.demo.openlinksw.com associated with source document(s)

Type: yago:Abstraction100002137yago:Matter100020827yago:Mixture114586258yago:Part113809207yago:PhysicalEntity100001930yago:Relation100031921yago:Solution114589223yago:Substance100019613yago:WikicatExactSolutionsInGeneralRelativity New Facet based on Instances of this Class

In general relativity, the de Sitter–Schwarzschild solution describes a black hole in a causal patch of de Sitter space. Unlike a flat-space black hole, there is a largest possible de Sitter black hole, which is the Nariai spacetime. The Nariai limit has no singularities, the cosmological and have the same area, and they can be mapped to each other by a discrete reflection symmetry in any causal patch.