Non-geodesic observer congruences in covariant cosmology produce redshift dipoles with non-trivial distance dependence beyond standard kinematic boosts.
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Redshift drift for tilted observers consists of an FLRW background term plus directional corrections from peculiar expansion, projected shear, and acceleration along the line of sight.
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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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Expected redshift drift for tilted observers
Redshift drift for tilted observers consists of an FLRW background term plus directional corrections from peculiar expansion, projected shear, and acceleration along the line of sight.