Perturbative Charged Rotating 5D Einstein-Maxwell Black Holes
arXiv:0706.0591 · doi:10.1007/s10714-010-1033-1
Abstract
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. Comparison of the perturbative analytical solutions with their non-perturbative numerical counterparts shows remarkable agreement.
RevTeX style, 4 pages, 5 figures
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- Charged rotating Kaluza-Klein multi-black holes and multi-black strings in five-dimensional Einstein-Maxwell theory
- Bertotti-Robinson solutions of D=5 Einstein-Maxwell-Chern-Simons-Lambda theory
- Extremal Myers-Perry black holes in Born-Infeld-dilaton theory
- Angular momentum-area proportionality of extremal charged black holes in odd dimensions
- Charged Rotating Black Holes in Higher Dimensions
- A note on the Kerr-Newman metric in five dimensions
- On well-posedness and algebraic type of the five-dimensional charged rotating black hole with two equal-magnitude angular momenta