arXiv · 1308.3716
Gravitational Dynamics From Entanglement "Thermodynamics"
Abstract
In a general conformal field theory, perturbations to the vacuum state obey the relation δS = δE, where δS is the change in entanglement entropy of an arbitrary ball-shaped region, and δE is the change in "hyperbolic" energy of this region. In this note, we show that for holographic conformal field theories, this relation, together with the holographic connection between entanglement entropies and areas of extremal surfaces and the standard connection between the field theory stress tensor and the boundary behavior of the metric, implies that geometry dual to the perturbed state satisfies Einstein's equations expanded to linear order about pure AdS.
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Nima Lashkari, Michael B. McDermott, Mark Van Raamsdonk. 2013-08-22. Gravitational Dynamics From Entanglement "Thermodynamics". https://doi.org/10.1007/jhep04(2014)195
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