The Kerr–Newman–de–Sitter metric (KNdS) is the one of the most general stationary solutions of the Einstein–Maxwell equations in general relativity that...
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The Kerr–Newman metric is the most general asymptotically flat and stationary solution of the Einstein–Maxwell equations in general relativity that describes...
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when it was discovered by Roy Kerr.: 69–81 The natural extension to a charged, rotating black hole, the Kerr–Newman metric, was discovered shortly thereafter...
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} De Sitter space Anti-de Sitter space De Sitter universe Kerr–Newman–de–Sitter metric AdS/CFT correspondence R. Bousso (2003). "Adventures in de Sitter...
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Rotating black hole (redirect from Kerr-Newman rotating black hole)
field equation. There are two known exact solutions, the Kerr metric and the Kerr–Newman metric, which are believed to be representative of all rotating...
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analogous solution for a charged, rotating body is given by the Kerr–Newman metric. The metric was discovered between 1916 and 1921 by Hans Reissner, Hermann...
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refer to: KNDS-LP, American radio station in Fargo, North Dakota Kerr–Newman–de–Sitter metric, a solution of the Einstein–Maxwell equations Khandeshwar railway...
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Willem de Sitter (6 May 1872 – 20 November 1934) was a Dutch mathematician, physicist, and astronomer. Born in Sneek, de Sitter studied mathematics at...
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solution Reissner–Nordström metric (charged, non-rotating solution) Kerr metric (uncharged, rotating solution) Kerr–Newman metric (charged, rotating solution)...
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Reissner–Nordström metric. Rotating black holes are described by the Kerr metric and the Kerr–Newman metric.[further explanation needed] Other notable metrics are:...
15 KB (2,488 words) - 23:03, 29 December 2023