Cosmological equivalence principle and the weak-field limit
David L. Wiltshire

TL;DR
This paper extends the strong equivalence principle to cosmology, linking density inhomogeneities to clock synchronization and suggesting modifications to Newtonian dynamics at large scales, with implications for understanding cosmic acceleration.
Contribution
It introduces the cosmological equivalence principle, connecting density contrasts to clock synchronization and proposing a scale for modified Newtonian dynamics based on backreaction models.
Findings
The relative deceleration scale matches the empirical MOND acceleration at low redshift.
Integrated effects lead to a 38% difference in clock rates between galaxies and voids.
The scale varies with redshift, affecting galaxy cluster dynamics and structure formation.
Abstract
The strong equivalence principle is extended in application to averaged dynamical fields in cosmology to include the role of the average density in the determination of inertial frames. The resulting cosmological equivalence principle is applied to the problem of synchronisation of clocks in the observed universe. Once density perturbations grow to give density contrasts of order one on scales of tens of megaparsecs, the integrated deceleration of the local background regions of voids relative to galaxies must be accounted for in the relative synchronisation of clocks of ideal observers who measure an isotropic cosmic microwave background. The relative deceleration of the background can be expected to represent a scale in which weak-field Newtonian dynamics should be modified to account for dynamical gradients in the Ricci scalar curvature of space. This acceleration scale is estimated…
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