Rotating Einstein-Maxwell-Dilaton Black Holes in D Dimensions

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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.
12 pages, 6 figues

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High Energy Physics - Theory

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http://salesiana.dossiersoluciones.com/handle/123456789/189570

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/hep-th/0606005
 http://arxiv.org/abs/hep-th/0606005
 Phys.Lett.B639:95-100,2006
 doi:10.1016/j.physletb.2006.06.024

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arXiv