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.
Articles by others on the same topic
There are currently no matching articles.