Rotating black hole

ID: rotating-black-hole

A rotating black hole, also known as a Kerr black hole, is a type of black hole characterized by its rotation around an axis. The concept was first formulated by mathematician Roy P. Kerr in 1963. Unlike non-rotating (Schwarzschild) black holes, which are spherically symmetric, rotating black holes have an axial symmetry and are described by more complex mathematical structures.

New to topics? Read the docs here!