Rotating Black Holes in Einstein-Maxwell-Dilaton Gravity

Abstract

We present a new class of slowly rotating black hole solutions in $(n+1)$-dimensional $(n\ge 3)$ Einstein-Maxwell-dilaton gravity in the presence of Liouville-type potential for the dilaton field and an arbitrary value of the dilaton coupling constant. Because of the presence of the dilaton field, the asymptotic behaviour of these solutions are neither flat nor (A)dS. In the absence of a dilaton field, our solution reduces to the $(n+1)$-dimensional Kerr-Newman modification thereof for small rotation parameter \cite{Aliev2}. We also compute the angular momentum and the gyromagnetic ratio of these rotating dilaton black holes.

9 pages, 7 figures, references added, to appear in Phys. Rev. D

References in corpus (3)

• Thermodynamics of charged topological dilaton black holes
• Slowly Rotating Charged Gauss-Bonnet Black holes in AdS Spaces
• Slowly Rotating Dilaton Black hole In Anti-de Sitter Spacetime

Cited by in corpus (2)

• Higher dimensional slowly rotating dilaton black holes in AdS spacetime
• Asymptotically flat charged rotating dilaton black holes in higher dimensions