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Entropy corrections to five-dimensional black holes and de Sitter spaces

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Abstract

It is shown that non-rotating black holes in three or four dimensions possess a canonical entropy. Recently study indicated that there were logarithmic corrections to Bekenstein–Hawking entropy in area with a uncertain coefficient which depends on specific models. In this paper, the thermal fluctuations on Bekenstein–Hawking entropy in five-dimensional topological AdS (TAds)-black holes and topological de Sitter (Tds) spaces will be considered based on a uniformly spaced area spectrum approach.

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Authors and Affiliations

  1. School of Physics and Optoelectronic, Dalian University of Technology, Dalian, 116024, People’s Republic of China

    Fujun Wang, Yuanxing Gui & Chunrui Ma

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  1. Fujun Wang
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  2. Yuanxing Gui
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  3. Chunrui Ma
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Correspondence to Yuanxing Gui.

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Wang, F., Gui, Y. & Ma, C. Entropy corrections to five-dimensional black holes and de Sitter spaces. Gen Relativ Gravit 40, 2649–2657 (2008). https://doi.org/10.1007/s10714-008-0644-2

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  • DOI: https://doi.org/10.1007/s10714-008-0644-2

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