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The Kerr metric or Kerr geometry describes the geometry of empty spacetime around a rotating uncharged axially symmetric black hole with a quasispherical event horizon. The Kerr metric is an exact solution of the Einstein field equations of general relativity; these equations are highly non-linear, which makes exact solutions very difficult to find.
Features, Metric & Relation to other exact solutions
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kerr black displaystyle metric hole mass rotating horizon solutions spacetime schwarzschild event solution geometry general moments ergosphere momentum vacuum relativity
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Kerr metric | is a | exact solution of the Einstein field equations of general relativity | 0.90 | text |
| Kerr metric | is a | generalization to a rotating body of the Schwarzschild metric | 0.90 | text |
| Kerr metric | is a | subgroup of the ten-dimensional Poincaré group which takes the two-dimensional locus of the singularity to itself | 0.90 | text |
| Kerr metric | is a | mathematical construct with negative mass | 0.90 | text |
| a neutron star | instance of | it should be able to be used as an exterior solution to model the gravitational field around a rotating massive object other than a black hole | 0.80 | text |
| or the Earth | instance of | it should be able to be used as an exterior solution to model the gravitational field around a rotating massive object other than a black hole | 0.80 | text |
| Kerr metric | related to Anti-universe region | The Kerr | 0.60 | section |
| Kerr metric | related to Anti-universe region | In | 0.60 | section |
| Kerr metric | related to Anti-universe region | Boyer-Lindquist | 0.60 | section |
| Kerr metric | related to Anti-universe region | As | 0.60 | section |
| Kerr metric | related to Boyer–Lindquist coordinates | The Kerr | 0.60 | section |
| Kerr metric | related to Boyer–Lindquist coordinates | The | 0.60 | section |
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