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

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. Geom...

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Bibliographic Details
Published in:The European physical journal. C, Particles and fields Particles and fields, 2016-10, Vol.76 (10), p.1, Article 571
Main Authors: Hendi, Seyed Hossein, Li, Gu-Qiang, Mo, Jie-Xiong, Panahiyan, Shahram, Panah, Behzad Eslam
Format: Article
Language:English
Subjects:
Astronomy
Astrophysics and Cosmology
Black holes
Elementary Particles
Hadrons
Heavy Ions
Measurement Science and Instrumentation
Nuclear Energy
Nuclear Physics
Physics
Physics and Astronomy
Quantum Field Theories
Quantum Field Theory
Regular Article - Theoretical Physics
String Theory
Thermodynamics
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Summary: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.
ISSN:1434-6044
1434-6052
DOI:10.1140/epjc/s10052-016-4410-4