Dynamics of Gravity as Thermodynamics on the Spherical Holographic Screen
arXiv:1007.4331 · doi:10.1103/PhysRevD.83.021501
Abstract
The dynamics of general Lovelock gravity, viewed on an arbitrary spherically symmetric surface as a holographic screen, is recast as the form of some generalized first law of thermodynamics on the screen. From this observation together with other two distinct aspects, where exactly the same temperature and entropy on the screen arise, it is argued that the thermodynamic interpretation of gravity is physically meaningful not only on the horizon, but also on a general spherically symmetric screen.
10 pages, revtex4; v2: minor corrections, references added? v3: the summary paragraph replaced by the discussion of the general static case, minor corrections/clarifications/modifications, references added, match the published version
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- Fundamental Constants, Entropic Gravity and Nonextensive Equipartition Theorem
- Negative Temperature Pressure in Black Holes
- Thermodynamic extended phase space and criticality of black holes at Pure Lovelock gravity
- A topological charge of black holes
- Revisiting the Second Law and Weak Cosmic Censorship Conjecture in High-Dimensional Charged-AdS Black Hole: an Additional Assumption
- A New Phase Transition Related to the Black Hole's Topological Charge
- Gravitational thermodynamics and universal holographic duality in dynamical spacetimes