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

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概要

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• 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>=const(≐̸0), where this constant is independent of the initial values of a and b.

• 理論物理学刊行会の論文
• 2005-09-25

著者

• MAEDA Keiichi

  Department of Earth Science and Astronomy, College of Arts and Science, University of Tokyo

• Maeda Keiichi

  Department Of Astronomy And Research Center For The Early Universe The University Of Tokyo

• Maeda Keiichi

  Department Of Physics Waseda University:advanced Research Institute For Science And Engineering Wase

• YOSHIDA Shijun

  Department of Physics, Hirosaki University

• Yoshida Shijun

  Department Of Physics Waseda University

• Yoshida Shijun

  Department Of Physics Hirosaki University

• NOMURA Hidefumi

  Department of Physics, Waseda University

• TANABE Makoto

  Department of Physics, Waseda University

• Nomura Hidefumi

  Department Of Physics Waseda University

• Tanabe Makoto

  Department Of Physics Waseda University

• Tanabe Makoto

  Department Of Chemistry Rikkyo University

• YOSHIDA Shijun

  Department of Physics, Waseda University

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