- #176
neopolitan
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JesseM said:Because I still don't understand what you mean when you say the expansion is the passage of time. Put it this way, do you accept that GR allows for the possibility of a non-expanding universe (either static or contracting) where time still passes? If you accept that GR allows for the possibility, is your idea of interpreting the expansion as the passage of time meant to say that GR is wrong that this is a possibility?
This is maybe a point where we need to be clear about our terms.
How would the passage of time be experienced in a non-expanding universe? Would it be experienced?
Would the passage of time be reversed in a contract so that from inside such a universe it still seems to expand?
Wasn't the idea of a static universe http://www.astrophysicsspectator.com/commentary/commentary20041020.html" (not my words, apparently his, but as far as I can tell it is hearsay)?
A http://www.americanscientist.org/template/AssetDetail/assetid/18638/" directed at string theory is that it explains too much, to the extent that (perhaps exaggerating a little) even if the universe was completely different, with laws of physics quite unlike ours, string theory could explain it. Such (interpretations of) theories lose predictive power.
I would have thought that a beauty of (stardard interpretations of) GR would be that GR explains the universe as it is. What you seem to be saying is that GP would also explain the universe if it were different, if it were static or contracting.
It seems that there is http://www-theory.phys.utas.edu.au/theory/qftfest/public.pdf" that universal expansion is actually increasing, rather than slowing down. If, as far as we can tell, the universe has always expanded and there are no indications that this expansion is on its way to stopping - what benefit is there in an interpretation of GR which indicates that it's ok to have a static or contracting universe?
It is entirely possible that I have misinterpreted JesseM and so I look forward to a clarification.
cheers,
neopolitan
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