Due to a misunderstanding of what I was asking, I'm re-asking this question (Is the Invariant interval S between the singularity and the present, the same for any point in space in an FLRW universe?) in a much more general sense
The invariant interval is defined as:
ds=√gμνdxμdxν
or rather (as per Hamilton's General Relativity, Black holes, and cosmology equation 2.13):
ds2=gμνdxμdxν
Because it is a scalar ds may be written as an exact differential form (As per Hamilton equation 2.11 referenced above):
ds=∂s∂xμdxμ
Where summation over \mu is implied. Note that (for geometric consistency) ∂s∂xμ can be identified with the metric:
ds2=(∂s∂xμdxμ)(∂s∂xνdxν)
=(∂s∂xμ∂s∂xν+∂s∂xν∂s∂xμ)dxμdxν
Which implies that:
(∂s∂xμ∂s∂xν+∂s∂xν∂s∂xμ)={∂s∂xμ,∂s∂xν}=gμν
But this expression is familiar, the generalized gamma matrices γμ are defined by:
{γμ,γν}=γμγν+γνγμ=2gμν
Which means that ∂s∂xμ can be identified with the generalized gamma matrices:
∂s∂xμ=1√2γμ
The second equation can also be written as:
ds=∂s∂xμdxμ=→∇s⋅d→r
Integrating now over some arbitrary interval {a,b}:
S=b∫a→∇s⋅d→r
Via the fundamental theorem of calculus, it is clear that the interval is independent of the path taken between the points {a,b}. Did I mess this up somewhere?
EDIT: Here's an approach not assuming s is an exact differential (as per the the objections voiced below)
The invariant interval is defined as:
ds=√gμνdxμdxν
or rather:
If we wish, this can be rearranged as:
0=dx⋅g⋅dx−ds2=dxμgμνdxν
One can write the metric tensor in terms of local basis:
gμν=eμ∙eν
Where ⋅ denotes the standard dot product and ∙ the tensor product. Used in the preceding equation, the above yields:
0=(eμdxμ)∙(eνdxν)−ds2
(note dx⋅e=dxμeμ) This can be simply factored to obtain:
0=(eμdxμ−ds)∙(eνdxν+ds)
0=(eμdxμ−ds)0=(eνdxν+ds)
Algebraically, this corresponds to the Clifford algebra as we have the relationship:
{eμ,eν}=eμeν+eνeμ=gμν
Which means that eμ can be identified with the generalized gamma matrice γμ:
eμ=1√2γμ
Taking either solution for ds individually, the integral for s between two nearby points appears to be independent of the path taken. Note that either solution to s individually could not be considered as proper time between events, but is simply a geometrical invariant.
The relationship between our starting equation and our two solutions now is entirely analogous to that between the Klein gordon equation and the Dirac equation. Solutions to the former are not necessarily solutions to the latter. Apparently no-one liked my first question using differential forms, so I wrote it up this way.
Also, if it eases concerns of undefined intervals, one can simply consider a flat space, since this argument itself is general.
Answer
I agree with ACM's answer; the conclusion is wrong, and there are many counterexamples.
For example, in the (+−−−) metric, the invariant interval ∫ds is equal to the proper time elapsed, for a purely timelike path. But we know that proper time depends on the path taken, for example in the twin paradox, where the moving twin comes back younger.
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