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We present perturbative charged rotating 5D Einstein-Maxwell black holes withspherical horizon topology. The electric charge Q is the perturbativeparameter, the perturbations being performed up to 4th order. The expressionsfor the relevant physical properties of these black holes are given. Thegyromagnetic ratio g, in particular, is explicitly shown to be non-constant inhigher order, and thus to deviate from its lowest order value, g=3. Comparisonof the perturbative analytical solutions with their non-perturbative numericalcounterparts shows remarkable agreement.

Perturbative Charged Rotating 5D Einstein-Maxwell Black Holes