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arXiv · hep-th/0502179

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

Hidefumi Nomura·Shijun Yoshida·Makoto Tanabe·Kei-ichi Maeda
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Abstract

We study the evolution of a five-dimensional rotating black hole emitting scalar field radiation via the Hawking process for arbitrary initial values of the two rotation parameters $a$ and $b$. It is found that any such black hole whose initial rotation parameters are both nonzero evolves toward an asymptotic state $a/M^{1/2}=b/M^{1/2}={\rm const}(\neq 0)$, where this constant is independent of the initial values of $a$ and $b$.

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Hidefumi Nomura, Shijun Yoshida, Makoto Tanabe, Kei-ichi Maeda. 2005-08-23. The Fate of a Five-Dimensional Rotating Black Hole via Hawking Radiation. https://doi.org/10.1143/ptp.114.707

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