budrap said:
I am citing only Arp's observations of high redshift quasars in close proximity to and in some cases even apparent interaction with low redshift galaxies. I am not interested in discussing Arp's theories about the same. It is his theories that have been shown to be in error not the underlying observations.
Higher-resolution observations (e.g. from the HST) show that there is no reason to believe these are anything but chance correlations, and that there isn't actually any interaction. The information is available on the Internet if you're willing to look for it. Just pick a specific observation and go hunting.
budrap said:
However, assuming the existence of a "Universe" and consequently a universal reference frame that contains it and then applying the equations of GR to said "Universe" was indeed a "blunder" as you would have it.
That's just plain false, though. First, the results only become inconsistent between different reference frames when you start run into irregularities in the coordinate system (typically singularities). Thus taking, as a tentative hypothesis, the proposal that there exist reference frames for which the universe appears homogeneous and isotropic is a perfectly reasonable thing to do. You can't trust the behavior of the result in the vicinity of any singularities in the coordinate system (which would be at t=0), but other than that it doesn't mess anything up.
The question, then, is whether or not there actually
is a reference frame for which our universe is approximately homogeneous and isotropic. The second part to that is, today, trivial to answer, just by looking at the CMB. The CMB is uniform to about one part in one thousand in each direction. Once we take out the dipole of the CMB (presumably due to our own motion with respect to it), the CMB is uniform to about one part in one hundred thousand.
That is pretty darned isotropic.
So, the only question remains, is the assumption that there exists a reference frame for which our universe is also homogeneous valid? First, the default answer to this would most definitely be yes, for the simple reason that a universe that appears isotropic, but isn't actually homogeneous, would indicate that we are extremely near the center of an extremely big universe. And that is something that is rather ridiculous on its face. However, can we test it?
Indeed we can!
You see, for a while some cosmologists thought that it was possible to explain the acceleration of our universe due to our universe being isotropic but not homogeneous. This would indicate that we live near the center of a very large, underdense region (a void). Well, this hypothesis does provide some definite predictions that don't line up with observation, as seen here:
http://arxiv.org/abs/1007.3725
Thus, with all of the other observations that
do make sense when we keep the assumption of homogeneity, we can be pretty darned confident that this assumption is accurate. And since there are no singularities in the coordinate system far from t=0, we don't have to worry about it giving us incorrect results due to picking a bad coordinate system.
We should obviously be careful not to extrapolate it too far beyond our cosmological horizon, or too close to t=0. And we certainly wouldn't want to use these coordinates to attempt to describe behavior too close to overdense/underdense regions. But other than that it isn't a concern.
budrap said:
1. If by not valid you mean it doesn't make any sense we are in complete agreement. It is however a logical consequence of the Big Bang model and ducking that inconvenient fact doesn't change the necessary conclusion that the BB model leads straight back to an illogical absurdity.
The big bang model is not expected to be complete. General Relativity itself is the problem here: GR predicts that there will be a singularity in the finite past, almost no matter what sort of physical model we use. We expect that a correct theory of quantum gravity will correct this flaw in GR.
budrap said:
2. I'm not saying that they require a universal spacetime reference frame. I'm saying that they constitute a universal spacetime reference frame. Calling them comoving coordinates is simply a semantic dodge.
Except they don't. You're mixing different terms here. The very idea of a universal reference frame is one that if you are within a perfectly-insulated, closed container, you can tell how fast you are moving. Picking a particular coordinate system within which to do calculations doesn't change the fact that we can't do this. In the FRW universe, we would
still have to look outside to see the CMB, for instance. There would be no way to determine our motion without looking outside.