The kinematic component of the cosmological redshift
Micha{\l} Chodorowski (Copernicus Center)

TL;DR
This paper revises the interpretation of cosmological redshift, proposing a new method of velocity transport that distinguishes between kinematic and gravitational components, and clarifies the nature of recession velocities in cosmology.
Contribution
It introduces a new approach to transport velocity four-vectors along the geodesic, deriving a formula for the kinematic redshift component applicable to any FLRW cosmology.
Findings
The kinematic component of redshift differs from the relativistic Doppler formula.
Recession velocities at high redshift can approach the speed of light but are not true velocities.
Proper recession velocities can be superluminal but are not physically actual velocities.
Abstract
It is widely believed that the cosmological redshift is not a Doppler shift. However, Bunn & Hogg have recently pointed out that to settle properly this problem, one has to transport parallelly the velocity four-vector of a distant galaxy to the observer's position. Performing such a transport along the null geodesic of photons arriving from the galaxy, they found that the cosmological redshift is purely kinematic. Here we argue that one should rather transport the velocity four-vector along the geodesic connecting the points of intersection of the world-lines of the galaxy and the observer with the hypersurface of constant cosmic time. We find that the resulting relation between the transported velocity and the redshift of arriving photons is not given by a relativistic Doppler formula. Instead, for small redshifts it coincides with the well known non-relativistic decomposition of the…
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