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      Thermodynamics of Slowly Rotating Charged Black Holes in anti-de Sitter Einstein-Gauss-Bonnet Gravity

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          Abstract

          By using a new approach, we demonstrate analytic expressions for slowly rotating Gauss-Bonnet charged black holes with negative cosmological constant. Up to the 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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          String-generated gravity models.

          (1985)
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            Entropy of Lovelock Black Holes

            Ted Jacobson, Robert C. Myers (1993)
            A general formula for the entropy of stationary black holes in Lovelock gravity theories is obtained by integrating the first law of black hole mechanics, which is derived by Hamiltonian methods. The entropy is not simply one quarter of the surface area of the horizon, but also includes a sum of intrinsic curvature invariants integrated over a cross section of the horizon.
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              Rotating Dilaton Black Holes

              James H. Horne, Gary T. Horowitz (1992)
              It is shown that an arbitrarily small amount of angular momentum can qualitatively change the properties of extremal charged black holes coupled to a dilaton. In addition, the gyromagnetic ratio of these black holes is computed and an exact rotating black string solution is presented.
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                Author and article information

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                Publication date Created: 19 November 2010
                Article
                DOI: 10.1088/0256-307X/28/2/020402
                ArXiV ID: 1011.4348
                SO-VID: 38431c76-df46-4683-a40a-dfed8fc4af1c
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                http://arxiv.org/licenses/nonexclusive-distrib/1.0/

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                Journal reference Chin.Phys.Lett.28:020402,2011
                Comments 9 Pages, submitted to Chin. Phys. Lett
                Categories gr-qc hep-th

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