Thermodynamics of the Reissner-Nordström-de Sitter Spacetime with Quintessence
arXiv:2204.04470 · doi:10.1140/epjc/s10052-022-10729-8
Abstract
For Anti-de Sitte (AdS) black holes, the isochoric heat capacity of system is vanished, while the isobaric heat capacity is not. However, this situation does not hold on for de Sitter (dS) black holes. In this work, by introducing the interaction between the black hole horizon and the cosmological horizon of the Reissner-Nordström-de Sitter (RNdS) spacetime with quintessence, we discuss the phase transition of this system. The results show that the spacetime not only has the similar phase transition behavior to that of Van der Waals (VdW) system, and the non-vanishing isochoric heat capacity fulfills the whole thermodynamics system. Through the discussion of the entropic force between two horizons, we find out the role of entropic force in the evolution of spacetime. In addition, we also study the influence of various parameters on the phase transition and entropic force, which will provide a new method for exploring the interaction among black hole molecules from a micro perspective.
References in corpus (27)
- Multiple Reentrant Phase Transitions and Triple Points in Lovelock Thermodynamics
- Thermodynamics of de Sitter Black Holes: Thermal Cosmological Constant
- van der Waals like behaviour of topological AdS black holes in massive gravity
- Extended thermodynamics and microstructures of four-dimensional charged Gauss-Bonnet black hole in AdS space
- Phase transition and Thermodynamical geometry of Reissner-Nordström-AdS Black Holes in Extended Phase Space
- Mechanical First Law of Black Hole Spacetimes with Cosmological Constant and Its Application to Schwarzschild-de Sitter Spacetime
- Critical behaviour and microscopic structure of charged AdS black holes via an alternative phase space
- Thermodynamics of the Euler-Heisenberg-AdS black hole
- Intriguing microstructures of five-dimensional neutral Gauss-Bonnet AdS black hole
- Phase transitions and geothermodynamics of black holes in dRGT massive gravity
- Thermodynamics of Gauss-Bonnet-de Sitter Black Holes
- Critical Phenomena of Born-Infeld-de Sitter Black Holes in Cavities
- Continuous phase transition and microstructure of charged AdS black hole with quintessence
- Range of novel black hole phase transitions via massive gravity: Triple points and N-fold reentrant phase transitions
- On Einstein-non linear-Maxwell-Yukawa de-Sitter black hole thermodynamics
- Thermodynamic properties of higher-dimensional dS black holes in dRGT massive gravity
- Phase transition and microstructures of five-dimensional charged Gauss-Bonnet-AdS black holes in the grand canonical ensemble
- Critical behavior of charged AdS black holes surrounded by quintessence via an alternative phase space
- Critical behavior of AdS Gauss-Bonnet massive black holes in the presence of external string cloud
- Critical behavior of charged dilaton black holes in AdS space
- Dynamical and Thermal Stabilities of Nonlinearly Charged AdS Black Holes
- Ehrenfest's scheme and microstructure for regular-AdS black hole in the extended phase space
- Phase Structures and Transitions of Quintessence Surrounding RN Black Holes in a Grand Canonical Ensemble
- Analytic phase structures and thermodynamic curvature for the charged AdS black hole in alternative phase space
- Entropic force between two horizons of dilaton black holes with a power-Maxwell field
- Effect of the inner horizon on the black hole thermodynamics: Reissner-Nordström black hole and Kerr black hole
- Characteristic interaction potential of black hole molecules from the microscopic interpretation of Ruppeiner geometry
Cited by in corpus (4)
- Noncommutative Schwarzschild black hole surrounded by quintessence: Thermodynamics, Shadows and Quasinormal modes
- Thermodynamics and Shadows of quantum-corrected Reissner-Nordström black hole surrounded by quintessence
- Schwarzschild Black Hole Surrounded by Perfect Fluid Dark Matter in the presence of Quintessence Matter Field
- Quantum-corrected Schwarzschild AdS black hole surrounded by quintessence: Thermodynamics and Shadows