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A Covariant Version of Verlinde's Emergent Gravity

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arxiv 1703.01415 v3 pith:4DSPMFZY submitted 2017-03-04 gr-qc

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keywords covariantdarkemergentgravitymatterverlindeversionallows
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A generally covariant version of Erik Verlinde's emergent gravity model is proposed. The Lagrangian constructed here allows an improved interpretation of the underlying mechanism. It suggests that de-Sitter space is filled with a vector-field that couples to baryonic matter and, by dragging on it, creates an effect similar to dark matter. We solve the covariant equation of motion in the background of a Schwarzschild space-time and obtain correction terms to the non-covariant expression. Furthermore, we demonstrate that the vector field can also mimic dark energy.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 77 citations worldwide. Full citation record

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    A single relativistic scalar field with a Bekenstein-type kinetic term and a mass-generating term reproduces deep-MOND acceleration in the weak-field limit and predicts stronger-than-MOND light bending.

  3. Slowly Rotating Neutron Stars in Aether Scalar-Tensor Theory

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    In Aether Scalar-Tensor theory, slowly rotating neutron stars obey approximate universal moment-of-inertia versus compactness relations that deviate from general relativity and are fit with parameter-dependent formulae.

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