Rotating Gauss-Bonnet BTZ Black Holes

Understand

We obtain rotating black hole solutions to the novel 3D Gauss-Bonnet theory of gravity recently proposed.

• These solutions generalize the BTZ metric and are not of constant curvature.
• They possess an ergoregion and outer horizon, but do not have an inner horizon.
• We present their basic properties and show that they break the universality of thermodynamics present for their static charged counterparts, whose properties we also discuss.