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Ruppeiner geometry and 2D dilaton gravity in the thermodynamics of black holes

机译:黑洞热力学中的Ruppeiner几何和2D Dilaton引力

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We study the geometric approach to the black hole thermodynamics. The geometric description of the equilibrium thermodynamics comes from Ruppeiner geometry based on a metric on the thermodynamic state space. For this purpose, we consider the Reissner-Nordstrom-AdS (RN-AdS) black hole which provides two different ensembles: canonical ensemble for fixed-charge case and grand canonical ensemble for fixed-potential case. Two cases are independent and cannot be mixed into each other. Hence, we calculate different Ruppeiner curvatures for two ensembles. However, we could not find the consistent behaviors of Ruppeiner curvature corresponding to those of heat capacity. Alternatively, we propose the curvature scalar in the 2D dilaton gravity approach which shows the features of extremal, Davies and minimum temperature points of RN-AdS black hole, clearly. (c) 2008 Elsevier B.V. All rights reserved.
机译:我们研究了黑洞热力学的几何方法。平衡热力学的几何描述来自Ruppeiner几何,其基于热力学状态空间的度量。为此,我们考虑使用Reissner-Nordstrom-AdS(RN-AdS)黑洞,该黑洞提供两种不同的合奏:固定电荷情况的正则合奏和固定电位情况的大正则合奏。两种情况是独立的,不能相互混合。因此,我们为两个合奏计算不同的Ruppeiner曲率。但是,我们无法找到鲁珀因纳曲率与热容相对应的一致行为。另外,我们提出了二维dilaton引力方法中的曲率标量,它清楚地显示了RN-AdS黑洞的极值,戴维斯和最低温度点的特征。 (c)2008 Elsevier B.V.保留所有权利。

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