Charged Rotating AdS Black Holes with Chern-Simons coupling

Understand

We obtain a perturbative solution for rotating charged black holes in 5-dimensional Einstein-Maxwell-Chern-Simons theory with a negative cosmological constant.

• We start from a small undeformed Kerr-AdS solution and use the electric charge as a perturbative parameter to build up black holes with equal-magnitude angular momenta up to forth order.
• These black hole solutions are described by three parameters, the charge, horizon radius and horizon angular velocity.
• We determine the physical quantities of these black holes and study their dependence on the parameters of black holes and arbitrary Chern-Simons coefficient.