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The Kerr metric is a generalization to a rotating body of the Schwarzschild metric, discovered by Karl Schwarzschild in 1915, which described the geometry of spacetime around an uncharged, spherically symmetric, and non-rotating body.
Oct 8, 2014 · This paper celebrates the 50th anniversary of the discovery of the Kerr metric, the most general rotating black hole solution in general relativity. It covers the history, the properties, the applications, and the significance of the Kerr metric in astrophysics and quantum cosmology.
- Saul A. Teukolsky
- 2014
Definition: Kerr Metric. The Kerr metric is a metric for a spinning, spherical mass.
A draft chapter from a book project on the Kerr spacetime and rotating black holes, covering the mathematics and physics of the metric and its features. The chapter presents the line element in various coordinate systems and references some key papers and books on the topic.
- Matt Visser
- 2007
Learn about the Kerr metric, which describes rotating black holes with angular momentum and mass. Explore the horizons, orbits, and ergospheres of Kerr black holes in this undergraduate physics paper.
- 234KB
- 12
There are two known exact solutions, the Kerr metric and the Kerr–Newman metric, which are believed to be representative of all rotating black hole solutions, in the exterior region.
Jun 22, 2022 · The Kerr–Newman metric is the most general stationary solution of the Einstein-Maxwell equations in that describes the spacetime geometry in the region surrounding an electrically charged ...
