Kerr black holes

Kerr black holes are, in theory, the space-time region outside of a black hole. Kerr black holes were first proposed in 1963, and for nearly 60 were not mathematically proven to have stability. In other words, an inevitably perturbance to a Kerr black hole.

Relying on proof by contradiction, on May 30 three researchers posted online a 912-page paper a mathematical analysis to show "that slowly rotating Kerr black holes are indeed stable."[1]

## References[edit]

1. ↑ https://www.quantamagazine.org/black-holes-finally-proven-mathematically-stable-20220804/

v • d • e

Theory of Relativity

Theories|

Special Relativity • General Relativity • Quantitative Introduction to General Relativity

Geometry|

Differential geometry • Spacetime • Minkowski space

Controversy and disproofs|

Counterexamples to Relativity • Pioneer anomaly • Action-at-a-distance (especially Quantum entanglement)• Objections to Einstein's theories of relativity

Liberal pseudoscience|

Black holes • Dark matter • Moral relativism • Wormholes

See also|

Classical mechanics • Law of Universal Gravitation • Quantum mechanics • Quantifying Order