I have been studying Birkhoff's theorem and, separately, co-moving coordinates.
One of the final steps in Birkhoff's theorem (from Weinberg's GR pg. 337) is to redefine the time coordinate to absorb the $f(t)$ that arises, as $$t' = \int^{t}f(t)^{1/2}dt$$ Where $t$ is the time coordinate (which has incidentally been redefined already once through the derivation, but clearing this up will clear up the previous changes as well).
Why is this $f(t)$ able to be redefined away like this?
Co-moving coordinates, like used in FRW cosmology, are defined such that the cosmic fluid is in free-fall, and thus, $d\tau = dt$. If we did not define the FRW metric as co-moving, it might mean the $g_{00}$ term is a function of coordinate time. This would in turn mean that an object at a constant spatial point would have a proper time that diverges from the coordinate time.
What would this mean physically? (To have the proper time diverge from coordinate time as a function of time)