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yuiop
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jonmtkisco said:...
It just seems to me that if you consider an SR recession of two rockets away from each other in an almost-empty FLRW universe, and the rockets use their motors to maintain their recession speed (relative to each other) as a function of time such that it exactly duplicates the (subluminal) relative motion of two comoving particles in an FLRW Omega(m)=1 universe, you'd get the same Doppler redshift over time as you would get between the two particles in the FLRW Omega(m)=1 universe at each respective proper distance. Maybe that's not true.
Jon
Wallace said:I'm pretty sure that's not true, but it would be interesting to see what the results would be. In the end though, to know for sure there's only one way, and that is to do the calculation. I think you're understanding this stuff pretty well, but as I've said before, to get to the next level you really need to start playing with the equations. Analogies and concepts will only get you so far and will lead you astray if you try and push them too far, which I think you are doing.
Try and re-create some of the results in the papers about this stuff, most of them go through from the basics and if you have Hartle that should give you all you need that isn't covered. I'd be interested to know the results from the thought experiment you mention above, but without cranking the handle we're just punching smoke to try and work out the answer just from 'mental pictures' alone. It's always better to know the result from an exact calculation, and then try and understand in simpler terms what the results are telling you. That's pretty much the format of most of the work on this. If you want to push something to an area not explicitly covered already then unfortunately I don't think there are any shortcuts to getting there.
I found this interesting question:
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Optional Problem 10: “Minkowski space in disguise” (hard!): Show by a clever choice of coordinates that the FRW metric with ΩΛ =Ωm =Ωγ =0, Ωk = 1 (this is the special case with a(t)= t, k = −1, corresponding to an empty and maximally open universe) is simply the Minkowski metric in disguise.
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in this problem set http://ocw.mit.edu/NR/rdonlyres/4973019C-C55D-43D0-81AF-6FDA7D4444C7/0/ps8.pdf that seems to be related to the issue you are discussing. Anyone able to answer that question?
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