DavidK said:
Consider two frames of reference moving relative each other. In one of the frames the CMB is fully isotropic, i.e., it looks the same in all directions. In the other frame however, the CMB should be red shifted in one direction and blue shifted in the other direction. Thus, the first frame can be considered to be at rest relative the CMB, and therefore, in some sense, constitutes a preferred Lorentz frame.
That is perfectly correct.
It is not forbidden to have preferred frames in that sense.
One way to think about why it can be is to say this to yourself:
special relativity says that the LAWS of physics must be Lor. inv.
So we expect the EQUATIONS like the Maxwell eqns. to be Lor. inv.
But we do not expect particular SOLUTIONS of those equations to have this same symmetry.
So, well, the universe is a particular solution to the Einstein General Relativity equation. This solution is approximately the Friedman solution (called various things, Friedman-Lemaitre, FRW metric, various names...)
this particular solution, call it Friedman solution or whatever you like, is NOT Lorentz invariant. It has a concept of being at REST which was already discovered by Hubble back in 1930s (if I remember history right) long before people knew about CMB!
One can be at rest with respect to the expansion------sometimes they call it being at rest with respet to the "Hubble flow". So that the recession speed of distant galaxies looks the same in all directions.
That idea of being at rest turns out to be the SAME as being at rest with respect to the CMB, as you described.
If you are not at rest then it will look to you as if the galaxies in one direction are receding FASTER from you than the galaxies the same distance away in the opposite direction.
If you adjust your velocity so the Hubble expansion looks the same in all directions, then you will also find that the CMB looks on average the same in all directions (I mean has no dipole, it still can have small irregularities but think of them as averaged out).