We construct a supersymmetric rotating black hole with asymptotically flat
four-dimensional spacetime times a circle, by superposing an infinite number of
BMPV black hole solutions at the same distance in one direction. The near
horizon structure is the same as that of the five-dimensional BMPV black hole.
The rotation of this black hole can exceed the Kerr bound in general relativity
(q≡a/G4M=1), if the size is small.Comment: 7 pages, 3 figures; v2: comparison with black ring removed, detailed
discussion of rotation added, refs. added, v3: minor corrections, version to
appear in PR