Thermodynamics of spacetime: The Einstein equation of state.
Explore this paper's citation graph
Summary
The Einstein equation is derived from the form of black hole entropy together with the fundamental relation δ Q=TdS connecting heat, entropy, and temperature, and its validity is seen to depend on the existence of local equilibrium conditions.
- Type
- article
- Published
- 1995-04-04
- Cited by
- 2,325
- References
- 7
- Access
- Open access
- OpenAlex
- https://openalex.org/W2052723426
- Semantic Scholar
- https://api.semanticscholar.org/CorpusID:13223728
Keywords
Physics, Spacetime, Einstein, Unruh effect, Mathematical physics
References
Cited by
- Does an accelerated electron radiate Unruh radiation
- Comment on 'Quantization of Black Holes', by Xiao-Gang He and Bo-Qiang Ma (arXiv:1003.2510[hep-th])
- Testing of Dark Energy and a Solution of the Cosmological Constant Problem
- κ-Rindler space
- Komar energy and Smarr formula for noncommutative inspired Schwarzschild black hole
- On The Thermodynamics Of General Relativity
- Maximum Force Derived from Special Relativity, the Equivalence Principle and the Inverse Square Law
- Holographic Theory of Accelerated Observers, the S-matrix, and the Emergence of Effective Field Theory
- Signal Space and the Schwarzschild Black Hole
- Toolbox for reconstructing quantum theory from rules on information acquisition
- On Whether or not Non-Gravitational Interaction Can Occur in the Absence of Gravity
- Generalized second law of thermodynamics in f(T) gravity with entropy corrections
- Thermodynamics in hybrid metric-Palatini gravity
- Why Things Fall
- Lectures on quantum gravity
- Holographic Space-time Models in 1 + 1 Dimensions
- Experimental observation of Minkowski spacetime melting
- Statistical Mechanics Derived From Quantum Mechanics
- Quantum Fluctuations and Space-time Horizons
- Electro-gravity via geometric chrononfield
Related papers
- Comments on anomaly versus WKB/tunneling methods for calculating Unruh radiation
- Effect of spacetime dimensions on quantum entanglement between two uniformly accelerated atoms
- Einstein universe as a moving fluid cosmology
- Noncompact n-dimensional Einstein spaces as attractors for the Einstein flow
- On super quasi Einstein manifold
- Einstein's 1912-1913 struggles with Gravitation Theory: Importance of Static Gravitational Fields Theory
- Negatively curved Einstein metrics on ramified covers of closed four-dimensional hyperbolic manifolds
- Cosmology and Description of Local Space-Time Properties by Einstein's Equations
- Einstein以前のEinstein--Einsteinを読む (Einsteinと基礎物理学 )