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Can a non-local model of gravity reproduce Dark Matter effects in agreement with MOND?

I analyze the possibility of reproducing MONDian Dark Matter effects by using a non-local model of gravity. The model was used before in order to recreate screening effects for the Cosmological Constant ($Λ$) value. Although the model in the weak-field approximation (in static coordinates) can reproduce the field equations in agreement with the AQUAL Lagrangian, the solutions are scale dependent and cannot reproduce the same dynamics in agreement with MOND.

preprint2013arXivOpen access
Ivan Arraut
gr-qc
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Ivan Arraut

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