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Nevertheless there is the observable Hubble redshift, i.e., an electromagnetic wave emitted very long ago from a far-distant galaxy has a higher frequency at emission than at observation, and you have a redshift-distance relation making the Hubble Law. It's just the free-em-field solution of Maxwell's equations in a FLRW spacetime.PeterDonis said:It suffers a coordinate effect that many cosmologists misleadingly refer to as "redshift", but it suffers no actual effect at all unless it interacts with something.
To expand on "no actual effect at all": what seems "pretty clear" to me is that the only invariant thing you can say about the wave packet's propagation in the absence of interaction is that the wave vector is parallel transported along the null geodesic worldline of the light ray, and "parallel transport" along a geodesic translates to "unchanged".