Rotating Einstein-Maxwell-dilaton black holes in D dimensions

We construct exact charged rotating black holes in Einstein-Maxwell-dilaton theory in D spacetime dimensions, D⩾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.