Charged rotating black holes in dilaton gravity

Abstract

We consider charged black holes with curved horizons, in five dimensional dilaton gravity in the presence of Liouville-type potential for the dilaton field. We show how, by solving a pair of coupled differential equations, infinitesimally small angular momentum can be added to these static solutions to obtain charged rotating dilaton black hole solutions. In the absence of dilaton field, the non-rotating version of the solution reduces to the five dimensional Reissner-Nordström black hole, and the rotating version reproduces the five dimensional Kerr-Newman modification thereof for small rotation parameter. We also compute the angular momentum and the angular velocity of these rotating black holes which appear at the first order.

5 pages, to appear in Int. J. Mod. Phys. A

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Cited by in corpus (11)

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• Slowly Rotating Charged Gauss-Bonnet Black holes in AdS Spaces
• Thermodynamical properties of topological Born-Infeld-dilaton black holes
• Higher dimensional slowly rotating dilaton black holes in AdS spacetime
• Rotating Black Holes in Einstein-Maxwell-Dilaton Gravity
• Extremal Charged Rotating Dilaton Black Holes in Odd Dimensions
• Asymptotically flat charged rotating dilaton black holes in higher dimensions
• Slowly rotating Einstein-Maxwell-dilaton black hole and some aspects of its thermodynamics
• An Infinite Number of Static Soliton Solutions to the 5D Einstein-Maxwell Equations with a Dilaton Field
• Charged Rotating Kaluza-Klein Black Holes in Dilaton Gravity
• Higher Dimensional Charged Rotating Dilaton Black Holes