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The Bekenstein-Hawking Entropy of Higher-Dimensional Rotating Black Holes

Zheng Ze Ma
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Abstract

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.

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Zheng Ze Ma. 2006-05-24. The Bekenstein-Hawking Entropy of Higher-Dimensional Rotating Black Holes. https://doi.org/10.1143/ptp.115.863

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