Exact solutions in general relativity | Metric tensors

Kerr metric

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. (Wikipedia).

Kerr metric
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Related pages

Differential operator | Newman–Penrose formalism | Poincaré group | Schwarzschild metric | Unit vector | Coordinate system | Gravitational singularity | Noether's theorem | Mach's principle | Weyl tensor | Circular symmetry | Hamilton–Jacobi equation | Momentum | Electric charge | Exact solutions in general relativity | Static spacetime | Angular momentum | Ernst equation | Schwarzschild geodesics | E (mathematical constant) | Four-gradient | Colatitude | Lense–Thirring precession | Minkowski space | Nonlinear system | Neutron star | Belinski–Zakharov transform | Dust solution | Null vector | Cartesian coordinate system | Kerr–Newman metric | Isometry | Pi | Hartle–Thorne metric | Killing tensor | Rotating black hole | Schwarzschild coordinates | Four-momentum | Stationary spacetime | Closed timelike curve | Metric tensor | Static spherically symmetric perfect fluid | Einstein field equations | Covariance and contravariance of vectors | Line element | Reissner–Nordström metric | Oblate spheroidal coordinates | Rotational energy | Coordinate singularity | Newman–Janis algorithm | Petrov classification | Carter constant