Phase transition and entropy force between two horizons in (n+2)-dimensional de Sitter space
arXiv:2004.06796
Abstract
In this paper, the effect of the space-time dimension on effective thermodynamic quantities in (n+2)-dimensional Reissoner-Nordstrom-de Sitter space has been stud ied. Based on derived effective thermodynamic quantities, conditions for the phase transition are obtained. The result shows that the accelerating cosmic expansion can be attained by the entropy force arisen from the interaction between horizons of black holes and our universe, which provides a possible way to explain the physical mechanism for the accelerating cosmic expansion.
Accepted by Advances in High Energy Physics
References in corpus (23)
- The Cosmological Constant and Dark Energy
- On the Origin of Gravity and the Laws of Newton
- P-V criticality of charged AdS black holes
- Multiple Reentrant Phase Transitions and Triple Points in Lovelock Thermodynamics
- Thermodynamics of de Sitter Black Holes: Thermal Cosmological Constant
- Superfluid Black Holes
- van der Waals like behaviour of topological AdS black holes in massive gravity
- Cardy-Verlinde Formula and Thermodynamics of Black Holes in de Sitter Spaces
- Entropic cosmology: a unified model of inflation and late-time acceleration
- Mechanical First Law of Black Hole Spacetimes with Cosmological Constant and Its Application to Schwarzschild-de Sitter Spacetime
- Thermodynamics of horizons: de Sitter black holes and reentrant phase transitions
- Phase transition of holographic entanglement entropy in massive gravity
- Holographic Van der Waals-like phase transition in the Gauss-Bonnet gravity
- Thermodynamics of phase transition in higher dimensional Reissner-Nordström-de Sitter black hole
- Critical Phenomena of Charged de Sitter Black Holes in Cavities
- Mass function and particle creation in Schwarzschild-de Sitter spacetime
- Deconfinement as an entropic self-destruction: a solution for the quarkonium suppression puzzle?
- Probing the relationship between the null geodesics and thermodynamic phase transition for rotating Kerr-AdS black holes
- Cosmography of KNdS Black Holes and Isentropic Phase Transitions
- Entropy of Kerr-de Sitter black hole
- Quantum treatment of Verlinde's entropic force conjecture
- A simple link of information entropy of quantum and classical systems with Newtonian dependence of Verlinde's entropic force
- Higher derivative corrections to the entropic force from holography