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Nonlocal Metric Realizations of MOND

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arxiv 1403.6763 v1 pith:SUFTK5SE submitted 2014-03-26 astro-ph.CO astro-ph.GAgr-qchep-th

classification astro-ph.COastro-ph.GAgr-qchep-th
keywords equationsmondfieldmetricnonlocalalongargueclass
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I discuss relativistic extensions of MOND in which the metric couples normally to matter. I argue that MOND might be a residual effect from the vacuum polarization of infrared gravitons produced during primordial inflation. If so, MOND corrections to the gravitational field equations would be nonlocal. Nonocality also results when one constructs metric field equations which reproduce the Tully-Fisher relation, along with sufficient weak lensing. I give the full field equations for the simplest class of models, and I specialize these equations to the geometries relevant for cosmology. I conclude by sketching the direction of future studies.

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Cited by 1 Pith paper

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

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

    gr-qc 2025-05 conditional novelty 6.0 of 10

    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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