Consequences of Thermal Fluctuations of Well-Known Black Holes in Modified Gravity

Abstract

Quantum fluctuation consequences have significant role in high-energy physics. These fluctuation often regarded as a correction of the infrared (IR) limit. Such correction contribute to the high-energy limit of thermodynamical quantities and the stability conditions of black holes. In this work, we analyze the thermal stability of black holes in the presence of thermal fluctuations. We consider AdS black hole in Born-Infeld massive gravity with non-abelian hair and the charged AdS black hole with a global monopole. We develop many thermodynamical quantities such as entropy, temperature, pressure, heat capacity of a system at constant volume and pressure, ratio between the heat capacities at constant pressure and volume, Gibbs free energy and Helmholtz free energy for both black holes. The critical behavior and phase transitions of black holes are also presented. We also observe the local and global stability of black holes in the grand canonical ensemble and canonical ensemble for the specific values of different parameters, such as, symmetry breaking parameter $\eta$, massive parameter $m$ and non-abelian hair $\nu$.

29 pages, 26 figures, Accepted in CQG for publication

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• Resummation of Massive Gravity
• Thermodynamics of Black Holes in Massive Gravity
• P-V criticality in the extended phase space of black holes in massive gravity
• van der Waals like behaviour of topological AdS black holes in massive gravity
• Quantum Fluctuations of a BTZ Black Hole in Massive Gravity
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• Reentrant phase transitions and triple points of topological AdS black holes in Born-Infeld-massive gravity
• Phase transition of a charged AdS black hole with a global monopole through geometrical thermodynamics

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