Kerr solution

Kerr solution

[′kər sə‚lü·shən]
(relativity)
A solution to Einstein's field equations that describes a rotating, uncharged, axisymmetric black hole.
McGraw-Hill Dictionary of Scientific & Technical Terms, 6E, Copyright © 2003 by The McGraw-Hill Companies, Inc.
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Carter [13] generalized the Kerr solution by describing a rotating black hole in a four-dimensional de Sitter or anti-de Sitter background.
The Quantization of a Kerr-AdS Black Hole
Valiente Kroon have developed a method based on properties of the Kerr solution, a time-independent solution to the equations of General Relativity.
Event horizon could help determine evolutionary stage of a black hole
The Kerr solution, in Boyer-Lindquist coordinates and relativistic units is,
By (47) the correct expression for the Kerr solution (31) is,
On the ramifications of the Schwarzschild space-time metric

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