Kerr Black Hole
in Boyer-Lindquist coordinates

Natural Constants:
\(M = G = c = 1\)

Horizons:
\( r_H^\pm = M \pm \sqrt{M^2 - a^2} \)

Ergosphere:
\( r_E^\pm = M \pm \sqrt{M^2 - a^2 \cos{\theta}^2} \)

Options
Outer Ergosphere
Outer Horizon
Inner Horizon
Inner Ergosphere
Ring Singularity

Kerr-Parameter: a =
Scale:
© Alexander Nieddu