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Relativistic corrections to the rotation curves of disk galaxies

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arxiv 2004.05905 v2 pith:UOJNOMLM submitted 2020-04-10 astro-ph.GA gr-qc

Alexandre Deur This is my paper · ORCID
classification astro-ph.GAgr-qc
keywords diskgalacticmethodrelativisticcorrectionscurvesgalaxieslarge
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We present a method to investigate relativistic effects arising from large masses. The method is non-perturbative and employs a mean-field approximation and gravitational lensing. Using this method and a basic model of disk galaxy, we find that relativistic corrections to the rotation curves of disk galaxies are significant at large galactic radii. The model predicts a strong correlation between the inferred galactic dark mass and the galactic disk thickness, which we verified using two separate sets of observational data.

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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. Significance of Gravitational Nonlinearities on the Dynamics of Disk Galaxies

    astro-ph.GA 2019-08 reject novelty 6.0 of 10

    Baryonic matter alone, with gravitational self-interaction treated as a 1/r force in disks, reproduces the observed radial acceleration relation and yields an acceleration scale matching MOND.

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