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Consequences of thermal fluctuations of well-known black holes in modified gravity

Abdul Jawad

2020Classical and Quantum Gravity32 citationsDOIOpen Access PDF

Abstract

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 η , massive parameter m and non-abelian hair ν .

Topics & Concepts

PhysicsCanonical ensembleBlack hole (networking)Heat capacityThermalMassive gravityHelmholtz free energyMicro black holeGrand canonical ensembleAdS black holeBlack hole thermodynamicsThermal fluctuationsConstant (computer programming)Hawking radiationClassical mechanicsQuantum electrodynamicsExtremal black holeMicrocanonical ensembleThermodynamicsPhase transitionCosmological constantEntropy (arrow of time)Gibbs free energyCharged black holeLimit (mathematics)Binary black holeStability (learning theory)Quantum mechanicsBlack Holes and Theoretical PhysicsAstrophysical Phenomena and ObservationsNoncommutative and Quantum Gravity Theories