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On Emergent Gravity, Black Hole Entropy and Galactic Rotation Curves

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arxiv 1802.08533 v1 pith:LFCGMNSI submitted 2018-02-23 gr-qc hep-th

I. Díaz-Saldaña , J. C. López-Domínguez , M. Sabido This is my paper · ORCID
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keywords blackcurvesderiveforcegalacticgravitationalgravityhole
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In this work we derive a generalized Newtonian gravitational force and show that it can account for the anomalous galactic rotation curves. We derive the entropy-area relationship applying the Feynman-Hibbs procedure to the supersymmetric Wheeler-DeWitt equation of the Schwarzschild black hole. We obtain the modifications to the Newtonian gravitational force from the entropic formulation of gravity.

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Cited by 1 Pith paper

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  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}.

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