The Bekenstein-Hawking Entropy of Higher-Dimensional Rotating Black Holes(Astrophysics and Relativity)

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概要

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• A black hole can be regarded as a thermodynamic system described by a grand canonical ensemble. In this paper, we study the Bekenstein-Hawking entropy of higher-dimensional rotating black holes using the Euclidean path-integral method of Gibbons and Hawking. We give a general proof demonstrating that ignoring quantum corrections, the Bekenstein-Hawking entropy is equal to one-fourth of its horizon area for general higher-dimensional rotating black holes.

• 理論物理学刊行会の論文
• 2006-05-25

著者

• Ma Zheng

  Department Of Physics Southeast University

• MA Zheng

  Department of Physics, Southeast University

関連論文

• The Bekenstein-Hawking Entropy of Higher-Dimensional Rotating Black Holes(Astrophysics and Relativity)

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