TrickyDicky
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marcus said:...there is, in cosmology, a practical idea of an "absolute" time, or at least pragmatically preferred time, that the standard Friedmann equation model runs on, and corresponds to stationary observers time.
General Relativity allows this. The point is we have a kind of landmark. The glow from the ancient matter. Matter is what makes the difference.
Nicely put Marcus. I'd like to add to your insightful phrase in my bold that maybe sometimes we get hung upon abstractions about Spacetime, but it's good to remember ourselves once in a while that spacetime is just a geometrical abstraction to describe the relations within matter in its broad meaning of mass-energy continuum. In this sense matter is all there is and surely what makes the difference.
About the stationary observers, they illustrate the way the GR equations were designed in a general covariant way to have 6 independent differential equations with 6 unknown quantities and another 4 unknown quantities that are arbitrarily fixed with the choice of coordinates.
This condition allows us to stablish the rest frame or stationary observers as we set the coordinate space and the coordinate time for a particular metric, and therefore we can determine a rest state wrt these coordinates so in this sense the fundamental observers appear not only in the "Friedmann model" but in any metric we might build from the GR equations.
In our cosmological model this rest frame is embodied by the CMB like you say, we measure our motion with respect to this radiation that fills the vacuum thru the universe.
This is for a very practical reason, the CMB are photons and we are able to detect them, quite easily (from 1965 at least), we could say the CMB is the "visible" part of the energy density of the vacuum, which is indirectly observe or "felt" as dark energy (and also as dark matter according to some models with inhomogeneities such as those of T. Buchert et al., but these models are not mainstream).