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We study the evolution of a five-dimensional rotating black hole emittingscalar field radiation via the Hawking process for arbitrary initial values ofthe two rotation parameters $a$ and $b$. It is found that any such black holewhose initial rotation parameters are both nonzero evolves toward an asymptoticstate  $a/M^{1/2}=b/M^{1/2}={\rm const}(\neq 0)$, where this constant is independentof the initial values of $a$ and $b$.Comment: 6 pages, 6 figure

The Fate of a Five-Dimensional Rotating Black Hole via Hawking Radiation