Assuming the spatially flat FRW metric for simplicity: ds2=c2dt2−a(t)2(dx2+dy2+dz2)
Light freely propagating along the x-direction follows the null geodesic with spacetime interval ds=0. Therefore for small finite co-ordinate intervals Δt and Δx along the null geodesic we have the relationship: c Δta(t)=Δx
Now let us imagine a model of a clock that consists of a rigid ruler of fixed proper length Δl with an optical fiber attached along it.
Let us assume that the rigid ruler is co-moving with the expansion of the Universe.
Let us suppose that each tick of the clock consists of a light pulse sent down the optic fiber (assuming refractive index 1 for simplicity) which takes a constant time interval Δτ given by: Δτ=Δlc
Is this reasoning correct?
Answer
Firstly, notice that the Frequency of light used to measure time will not remain constant. I wont use this but do take note.
Secondly notice that If the object is rigid, then and One end is fixed at x = 0, then the other end in the co-ordinate systems used will be at
Δx=ΔLa(t)
So Now light using equation 1 from your question we get
Δt=a(t)∗Δxc=ΔLc
So both clocks reproduce cosmological time as expected.
I hope I understood your arguments correctly. I think the flaw in the argument is you cannot allow for both the rod to be rigid and its ends to be co-moving at the same time.
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