作者: Shahram Panahiyan , Shahram Panahiyan , Seyed Hossein Hendi , Jie-Xiong Mo , Behzad Eslam Panah
DOI: 10.1140/EPJC/S10052-016-4410-4
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摘要: 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 thermodynamical structure and critical behavior these through various methods this paper. Geometrical thermodynamics is employed to give picture phase transition holes. Next, new method used derive pressure radius horizon In addition, Maxwell equal area law Van der Waals like Moreover, exponents are calculated by using Ehrenfest equations, type determined.