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The Fate of a Five-Dimensional Rotating Black Hole via Hawking Radiation (2005)

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 $b$.. Comment: 6 pages, 6 figures

Publication details
Download http://arxiv.org/abs/hep-th/0502179
Repository arXiv (United States)
Keywords High Energy Physics - Theory, General Relativity and Quantum Cosmology
Type text