Including dark matter or modified gravity enhances the effective charge-to-baryonic-mass ratio Q/M_bar by a factor of 10-30 at virial radii, producing structurally linked seed fields of ~10^{-23} G in high-redshift proto-galaxies that could probe the dark sector via distinct radial and mass-dependen
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4 Pith papers cite this work, alongside 862 external citations. Polarity classification is still indexing.
4
Pith papers citing it
862
external citations · OpenAlex
verdicts
UNVERDICTED 4representative citing papers
Pulsar timing tests the vector RAR but current measurements are dominated by the Solar acceleration, producing similar chi-squared fits to a constant-acceleration model.
Proposes that 10 years of 0.5 μas astrometry of Proxima Centauri can distinguish MOND from Newtonian gravity in the low-acceleration regime.
The Bullet Cluster exhibits the same residual missing mass discrepancy under MOND as other similar clusters, and this mass is collisionless and aligned with the galaxies.
citing papers explorer
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Gravitational-Electric Polarization as a Probe of Dark Matter and Modified Gravity
Including dark matter or modified gravity enhances the effective charge-to-baryonic-mass ratio Q/M_bar by a factor of 10-30 at virial radii, producing structurally linked seed fields of ~10^{-23} G in high-redshift proto-galaxies that could probe the dark sector via distinct radial and mass-dependen
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The Pulsar Radial Acceleration Relation
Pulsar timing tests the vector RAR but current measurements are dominated by the Solar acceleration, producing similar chi-squared fits to a constant-acceleration model.
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Directly testing gravity with Proxima Centauri
Proposes that 10 years of 0.5 μas astrometry of Proxima Centauri can distinguish MOND from Newtonian gravity in the low-acceleration regime.
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On the residual missing mass of the Bullet Cluster
The Bullet Cluster exhibits the same residual missing mass discrepancy under MOND as other similar clusters, and this mass is collisionless and aligned with the galaxies.