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New perspective for black hole thermodynamics in Gauss–Bonnet–Born–Infeld massive gravity

机译:高斯-邦内-博恩-因费尔德大重力中黑洞热力学的新视角

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Following an earlier study regarding Einstein–Gauss–Bonnet-massive black holes in the presence of a Born–Infeld nonlinear electromagnetic field (Hendi, arXiv:1510.00108, 2016), we study thermodynamical structure and critical behavior of these black holes through various methods in this paper. Geometrical thermodynamics is employed to give a picture regarding the phase transition of these black holes. Next, a new method is used to derive critical pressure and radius of the horizon of these black holes. In addition, Maxwell equal area law is employed to study the Van der Waals like behavior of these black holes. Moreover, the critical exponents are calculated and by using Ehrenfest equations, the type of phase transition is determined.
机译:在先前关于存在Born-Infeld非线性电磁场的情况下有关爱因斯坦-高斯-贝涅斯质量黑洞的研究(Hendi,arXiv:1510.00108,2016)之后,我们通过多种方法研究了这些黑洞的热力学结构和临界行为。这张纸。采用几何热力学来给出有关这些黑洞的相变的图像。接下来,使用一种新方法来推导这些黑洞的临界压力和地平线半径。另外,麦克斯韦等面积定律被用来研究范德瓦尔斯像这些黑洞的行为。此外,计算临界指数并通过使用埃伦菲斯特方程确定相变的类型。

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