Perturbative Charged Rotating 5D Einstein-Maxwell Black Holes

Understand

We present perturbative charged rotating 5D Einstein-Maxwell black holes with spherical horizon topology.

• The electric charge Q is the perturbative parameter, the perturbations being performed up to 4th order.
• The expressions for the relevant physical properties of these black holes are given.
• The gyromagnetic ratio g, in particular, is explicitly shown to be non-constant in higher order, and thus to deviate from its lowest order value, g=3.