The fate of a five-dimensional rotating black hole via hawking radiation

Hidefumi Nomura; Shijun Yoshida; Makoto Tanabe; Kei Ichi Maeda

doi:10.1143/PTP.114.707

The fate of a five-dimensional rotating black hole via hawking radiation

Hidefumi Nomura^*, Shijun Yoshida, Makoto Tanabe, Kei Ichi Maeda

^*Corresponding author for this work

Research output: Contribution to journal › Article › peer-review

34 Citations (Scopus)

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

Original language	English
Pages (from-to)	707-712
Number of pages	6
Journal	Progress of Theoretical Physics
Volume	114
Issue number	3
DOIs	https://doi.org/10.1143/PTP.114.707
Publication status	Published - 2005 Sept
Externally published	Yes

ASJC Scopus subject areas

Physics and Astronomy (miscellaneous)

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10.1143/PTP.114.707

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title = "The fate of a five-dimensional rotating black hole via hawking radiation",

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.",

author = "Hidefumi Nomura and Shijun Yoshida and Makoto Tanabe and Maeda, {Kei Ichi}",

year = "2005",

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AU - Tanabe, Makoto

AU - Maeda, Kei Ichi

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N2 - 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.

AB - 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.

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The fate of a five-dimensional rotating black hole via hawking radiation

Abstract

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