arXiv · hep-th/0606005
Rotating Einstein-Maxwell-Dilaton Black Holes in D Dimensions
Abstract
We construct exact charged rotating black holes in Einstein-Maxwell-dilaton theory in $D$ spacetime dimensions, $D \ge 5$, by embedding the $D$ dimensional Myers-Perry solutions in $D+1$ dimensions, and performing a boost with a subsequent Kaluza-Klein reduction. Like the Myers-Perry solutions, these black holes generically possess $N=[(D-1)/2]$ independent angular momenta. We present the global and horizon properties of these black holes, and discuss their domains of existence.
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Jutta Kunz, Dieter Maison, Francisco Navarro-Lerida, Jan Viebahn. 2006-06-01. Rotating Einstein-Maxwell-Dilaton Black Holes in D Dimensions. https://doi.org/10.1016/j.physletb.2006.06.024
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