Stability of black holes based on horizon thermodynamics
From MaRDI portal
Publication:526326
DOI10.1016/j.physletb.2015.10.061zbMath1360.83039arXiv1511.03508OpenAlexW2107476421MaRDI QIDQ526326
Publication date: 10 May 2017
Published in: Physics Letters. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1511.03508
Related Items
Thermodynamic geometries analysis of charged black holes with barrow entropy ⋮ Horizon thermodynamics from Einstein's equation of state ⋮ Universality of \(P - V\) criticality in horizon thermodynamics ⋮ Electric Black Holes in a Model of Nonlinear Electrodynamics ⋮ The Hawking-Page-like phase transition from FRW spacetime to McVittie black hole ⋮ Thermodynamic phase transition and global stability of the regular Hayward black hole surrounded by quintessence ⋮ Phase transition and thermodynamic stability of topological black holes in Hořava–Lifshitz gravity ⋮ Revisit on the thermodynamic stability of the noncommutative Schwarzschild black hole ⋮ Consequences of thermal fluctuations of well-known black holes in modified gravity ⋮ Fractional-order phase transition of charged AdS black holes ⋮ Horizon thermodynamics in fourth-order gravity ⋮ GUP effect on thermodynamical properties of the noncommutative rotating BTZ black hole ⋮ Entropy of Higher-Dimensional Charged de Sitter Black Holes and Phase Transition ⋮ Charged and non-charged black hole solutions in mimetic gravitational theory ⋮ Thermodynamic properties of modified hairy and BTZ black holes ⋮ Thermodynamics of dynamical wormholes
Cites Work
- Unnamed Item
- Thermodynamics of phase transition in higher dimensional AdS black holes
- The four laws of black hole mechanics
- Corrected form of the first law of thermodynamics for regular black holes
- Thermodynamics of horizons: de Sitter black holes and reentrant phase transitions
- Thermodynamics of Spacetime: The Einstein Equation of State
- Classical and quantum thermodynamics of horizons in spherically symmetric spacetimes
