Kerrrotatie
Kerrrotatie refers to the phenomenon observed in the Kerr metric of general relativity, which describes a rotating black hole. Specifically, it is the effect where the spacetime around a Kerr black hole is dragged or twisted by its rotation. This means that any object or observer in the vicinity of the black hole will be forced to rotate along with the black hole, even if they are not directly interacting with it gravitationally.
This frame-dragging effect is a consequence of the black hole's angular momentum. The more rapidly a Kerr
The concept of Kerrrotatie has important implications for astrophysics, particularly in understanding the behavior of matter