Spacetime Equilibrium at Negative Temperature and the Attraction of Gravity
arXiv:1904.04843 · doi:10.1142/S0218271819440164
Abstract
We derive the Einstein equation from the condition that every small causal diamond is a variation of a flat empty diamond with the same free conformal energy, as would be expected for a near-equilibrium state. The attractiveness of gravity hinges on the negativity of the absolute temperature of these diamonds, a property we infer from the generalized entropy.
arXiv comment7 pages, Essay written for the Gravity Research Foundation 2019 Awards for Essays on Gravitation
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Cited by in corpus (11)
- Gravitational Thermodynamics of Causal Diamonds in (A)dS
- The minus sign in the first law of de Sitter horizons
- Thermodynamic ensembles with cosmological horizons
- Conformal Description of Near-Horizon Vacuum States
- Microcanonical Action and the Entropy of Hawking Radiation
- Strong-coupling dynamics and entanglement in de Sitter space
- Thermodynamics of spacetime and unimodular gravity
- The first law of differential entropy and holographic complexity
- From spacetime thermodynamics to Weyl transverse gravity
- Emergence of quadratic gravity from entanglement equilibrium
- Spacetime granularity from finite-dimensionality of local observable algebras