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Entropic corrections to Newton's law

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arxiv 1003.1998 v1 pith:CWHKRFKO submitted 2010-03-09 hep-th

classification hep-th
keywords correctiongravitycorrectionsnewtonconstructiondeviationsformmodel
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It has been known for some time that there is a deep connection between thermodynamics and gravity, with perhaps the most dramatic implication that the Einstein equations can be viewed as a thermodynamic equation of state. Recently Verlinde has proposed a model for gravity with a simple statistical mechanical interpretation that is applicable in the non-relatvistic regime. After critically analyzing the construction, we present a strong consistency check of the model. Specifically, we consider two well-motivated corrections to the area-entropy relation, the log correction and the volume correction, and follow Verlinde's construction to derive corrections to Newton's law of gravitation. We show that the deviations from Newton's law stemming from the log correction have the same form as the lowest order quantum effects of perturbative quantum gravity, and the deviations stemming from the volume correction have the same form as some modified Newtonian gravity models designed to explain the anomalous galactic rotation curves.

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Cited by 2 Pith papers

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

  1. Static Black Holes and Iyer-Wald Entropy in $f(\mathcal{R},\mathcal{K})$ Gravity

    gr-qc 2026-07 accept novelty 6.0 of 10

    In f(R,K) gravity with f=-X^{1-n}, first-order Schwarzschild corrections yield Iyer–Wald entropy S = S_BH + λ Υ_n S_BH^{n+1}.

  2. From modified Tsallis-Renyi entropy to a MOND-like force law, Bekenstein bound, and Landauer principle for black holes

    gr-qc 2025-05 reject novelty 3.0 of 10

    Modified Renyi entropy produces a modified force with a MOND-like interpolating function, but the force decays as 1/R^4, not MOND's 1/R, and the Bekenstein bound check reduces to a definitional inequality.

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