Non-geodesic observer congruences in covariant cosmology produce redshift dipoles with non-trivial distance dependence beyond standard kinematic boosts.
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Peculiar velocities grow proportionally to time in the Einstein-de Sitter era but experience progressive suppression and eventual decay in the Lambda-dominated phase, with residual growth persisting to the present day.
The 1+3 covariant formalism reproduces the standard result for peculiar velocity growth in cosmology and does not imply anomalous bulk flows or apparent acceleration.
citing papers explorer
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Redshift Dipoles from Non-Geodesic Observer Congruences in Covariant Cosmology
Non-geodesic observer congruences in covariant cosmology produce redshift dipoles with non-trivial distance dependence beyond standard kinematic boosts.
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Peculiar velocities in the $\Lambda$CDM universe
Peculiar velocities grow proportionally to time in the Einstein-de Sitter era but experience progressive suppression and eventual decay in the Lambda-dominated phase, with residual growth persisting to the present day.
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Cosmological peculiar velocities in general relativity
The 1+3 covariant formalism reproduces the standard result for peculiar velocity growth in cosmology and does not imply anomalous bulk flows or apparent acceleration.