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Thermodynamics of Slowly Rotating Charged Black Holes in Anti-de Sitter Einstein–Gauss–Bonnet Gravity |
| ZOU De-Cheng1, YANG Zhan-Ying1**, YUE Rui-Hong2**
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1Department of Physics, Northwest University, Xi'an 710069
2Faculty of Science, Ningbo University, Ningbo 315211
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| Cite this article: |
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ZOU De-Cheng, YANG Zhan-Ying, YUE Rui-Hong 2011 Chin. Phys. Lett. 28 020402 |
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Abstract By using a new approach, we demonstrate the analytic expressions for slowly rotating Gauss–Bonnet charged black hole solutions with one non-vanishing angular momentum in higher-dimensional anti-de Sitter spaces. Up to linear order of the rotating parameter a, the mass, Hawking temperature and entropy of the charged black holes get no corrections from rotation.
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04.20.Cv
04.50.-h
12.25.+e
04.65.+e
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Received: 20 September 2010
Published: 30 January 2011
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| PACS: |
04.20.Cv
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(Fundamental problems and general formalism)
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04.50.-h
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(Higher-dimensional gravity and other theories of gravity)
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12.25.+e
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04.65.+e
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(Supergravity)
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