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.

12 pages, 6 figues

References in corpus (3)

• `Hidden' Symmetries of Higher Dimensional Rotating Black Holes
• Charged Rotating Black Holes in Odd Dimensions
• Completely integrable sector in 5D Einstein-Maxwell gravity and derivation of the dipole black ring solutions

Cited by in corpus (11)

• `Hidden' Symmetries of Higher Dimensional Rotating Black Holes
• Higher-Dimensional Black Holes: Hidden Symmetries and Separation of Variables
• Electromagnetic Properties of Kerr-Anti-de Sitter Black Holes
• Thermodynamics of rotating solutions in (n+1)-dimensional Einstein-Maxwell-dilaton gravity
• Magnetic Branes in $(n+1)$-dimensional Einstein-Maxwell-dilaton gravity
• Rotating Spacetimes with Asymptotic Non-Flat Structure and the Gyromagnetic Ratio
• Generating technique for $U(1{)}^{3}5D$ supergravity
• Harrison transformation and charged black objects in Kaluza-Klein theory
• Rotating Black Holes in Einstein-Maxwell-Dilaton Gravity
• Rotating nonuniform black string solutions
• Asymptotically flat charged rotating dilaton black holes in higher dimensions