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

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

Author(s) -

Z. Z.

Publication year - 2006

Publication title -

progress of theoretical physics

Language(s) - English

Resource type - Journals

eISSN - 1347-4081

pISSN - 0033-068X

DOI - 10.1143/ptp.115.863

Subject(s) - physics , black hole thermodynamics , micro black hole , hawking radiation , hawking , entropy (arrow of time) , black hole (networking) , mathematical physics , extremal black hole , theoretical physics , quantum mechanics , classical mechanics , computer network , routing protocol , routing (electronic design automation) , computer science , link state routing protocol

A black hole can be regarded as a thermodynamic system described by a grandcanonical ensemble. In this paper, we study the Bekenstein-Hawking entropy ofhigher-dimensional rotating black holes using the Euclidean path-integralmethod of Gibbons and Hawking. We give a general proof demonstrating thatignoring quantum corrections, the Bekenstein-Hawking entropy is equal toone-fourth of its horizon area for general higher-dimensional rotating blackholes.Comment: 9 pages, Latex, v2: arxiv-id for the references supplemented, v3: accepted for publication by Progress of Theoretical Physic

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