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

^*この研究の対応する著者

研究成果: Article › 査読

34 被引用数 (Scopus)

抄録

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.

本文言語	English
ページ（範囲）	707-712
ページ数	6
ジャーナル	Progress of Theoretical Physics
巻	114
号	3
DOI	https://doi.org/10.1143/PTP.114.707
出版ステータス	Published - 2005 9月
外部発表	はい

ASJC Scopus subject areas

物理学および天文学（その他）

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10.1143/PTP.114.707

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

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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

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