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Prog. Theor. Phys. Vol. 114 No. 3 (2005) pp. 707-712

[ Full Text PDF : FREE ACCESS (197K) ]

Letters

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

Hidefumi Nomura,1,* Shijun Yoshida,1,** Makoto Tanabe1,*** and Kei-ichi Maeda1,2,3,****

1Department of Physics, Waseda University, Tokyo 169-8555, Japan
2Advanced Research Institute for Science and Engineering, Waseda University, Tokyo 169-8555, Japan
3Waseda Institute for Astrophysics, Waseda University, Tokyo 169-8555, Japan

(Received May 10, 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/M1/2 = b/M1/2 = const (≠0), where this constant is independent of the initial values of a and b.


URL : http://ptp.ipap.jp/link?PTP/114/707/
DOI : 10.1143/PTP.114.707


*E-mail: nomura@gravity.phys.waseda.ac.jp
**E-mail: shijun@waseda.jp
***E-mail: tanabe@gravity.phys.waseda.ac.jp
****E-mail: maeda@gravity.phys.waseda.ac.jp

[ Full Text PDF : FREE ACCESS (197K) ] Citation:

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Citing Article(s) :

  1. Progress of Theoretical Physics Vol. 128 No. 2 (2012) pp. 227-241 :
    Scalar Spheroidal Harmonics in Five Dimensional Kerr-(A)dS
    H. T. Cho, Alan S. Cornell, Jason Doukas and Wade Naylor

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