Complementary role of the pressure in the black hole thermodynamics
arXiv:1303.0491 · doi:10.1103/PhysRevD.87.067502
Abstract
In black hole thermodynamics of certain models, the thermodynamic first law may contain the pressure term. The corresponding entropy follows the area law whereas the thermodynamic energy is not the same with the black hole mass. If the pressure can be decomposed into two parts and recombined with the original thermodynamic quantities, then the thermodynamic energy becomes the black hole mass and the entropy satisfying the area law turns out to be the corrected entropy called the Wald entropy, respectively.
arXiv commentv2. version to appear in PRD; 7 pages, references added
References in corpus (11)
- Thermodynamics of Spacetime: The Einstein Equation of State
- Black Hole Entropy is Noether Charge
- Gauss-Bonnet Black Holes in AdS Spaces
- Twenty Years of the Weyl Anomaly
- Geometric Classification of Conformal Anomalies in Arbitrary Dimensions
- Thermodynamic route to Field equations in Lanczos-Lovelock Gravity
- Thermodynamic Behavior of Field Equations for f(R) Gravity
- Black Holes in Gravity with Conformal Anomaly and Logarithmic Term in Black Hole Entropy
- Quantum Tunneling and Trace Anomaly
- Horizon Thermodynamics and Gravitational Field Equations in Horava-Lifshitz Gravity
- Emergent perspective of Gravity and Dark Energy
Cited by in corpus (6)
- Einstein gravity with Gauss-Bonnet entropic corrections
- Thermodynamics of Conformal Anomaly Corrected Black Holes in AdS Space
- Universality of P-V Criticality in Horizon Thermodynamics
- Thermodynamic approach to field equations in Lovelock gravity and f(R) gravity revisited
- Horizon thermodynamics in fourth-order gravity
- Thermodynamics from field equations for black holes with multiple horizons