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What is the Entropy in Entropic Gravity?

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arxiv 1601.07558 v3 pith:YJTJ2VRM submitted 2016-01-27 hep-th gr-qc

classification hep-thgr-qc
keywords gravityentropyequationariseseinsteinholographicquantumstate
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We investigate theories in which gravity arises as a consequence of entropy. We distinguish between two approaches to this idea: holographic gravity, in which Einstein's equation arises from keeping entropy stationary in equilibrium under variations of the geometry and quantum state of a small region, and thermodynamic gravity, in which Einstein's equation emerges as a local equation of state from constraints on the area of a dynamical lightsheet in a fixed spacetime background. Examining holographic gravity, we argue that its underlying assumptions can be justified in part using recent results on the form of the modular energy in quantum field theory. For thermodynamic gravity, on the other hand, we find that it is difficult to formulate a self-consistent definition of the entropy, which represents an obstacle for this approach. This investigation points the way forward in understanding the connections between gravity and entanglement.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Rotating traversable wormholes and particle dynamics in $f(R,T)$ gravity

    gr-qc 2026-05 unverdicted novelty 5.0 of 10

    Rotating traversable wormholes in f(R,T) gravity are supported by anisotropic fluid satisfying null and strong energy conditions in the slow-rotation approximation, with particle dynamics and gravitational lensing analyzed.

  2. From Quantum Correlations to Inflationary Tracking Scalar Field Evolution

    gr-qc 2026-08 reject novelty 4.0 of 10

    The author argues, via condensed-matter-style analogies, that the inflationary tracking condition emerges when the correlation length of primordial quantum degrees of freedom scales as a power of the Hubble radius.

  3. Holographic Ordering and Negative entropy in Non-equilibrium Euclidean Black Hole Path Integralsl

    hep-th 2025-07 reject novelty 4.0 of 10

    Gravitational attraction is presented as the gradient of a negative entropy deficit, equal to the red-shifted shell energy divided by Hawking temperature, applied to a black hole with a static thin shell.

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