Primtall said:
ok, a hypersphere ( with t as radius ? ). I've heard one theorist speculate that its more like a double doughnut with the expansion pouring out into one and the contraction being sucked into the other. Think i like this one better as it conforms with Newton (action/reaction). But with the rate of expansion increasing I'm still perflexed about the infinite/finite question. but thks for the explanation , b rgds
The hypersphere is a common model for the case of finite spatial volume assuming overall positive curvature. A lower bound for the radius* has been estimated in one of the NASA reports ( WMAP 5th year data, Komatsu et al).
There is no simple relation between the radius and the age of the universe. It's probably not a good idea to think of the radius as a time coordinate.
Of course the U could be infinite spatial volume---this hasn't been ruled out. the way to get a numerical grip on the question is to estimate the curvature. But more refined measurement of curvature is needed. So far one can say that IF the curvature is positive and we are in the hypersphere case then with 95% certainty the curvature is LESS than a certain amount.
this corresponds to the radius of curvature being AT LEAST a certain length (with 95% certainty). And that lower bound turned out, according to Komatsu et al WMAP5 report, to be around 100 billion light years.
So by getting a quantitative handle on the curvature you get a quantitative handle on the current spatial volume of the universe
in that case. IF it is finite at all, and if we are in the positive curve situation, then the radius is AT LEAST a certain amount.
It is still very iffy and preliminary. Better measurement is in progress but it could be a few years, or even many years, before we have a good grip on this curvature number, and thus on the radius in the hypersphere case. I'm clueless as to what to expect.
I like thinking about the hypersphere case but its still just a speculative exercise. I'll get a link to Komatsu et al in case you want to check it out.
Wow, I simply googled "Komatsu WMAP 5" and it came up first hit!
http://arxiv.org/abs/0803.0547
If interested, look at Table 2 on page 4 where it says "curvature radius". If the notation conventions are unfamiliar, ask.
The column to pick is WMAP+BAO+SN because that uses all the available data, not only WMAP but also galaxy counts at various distances and also supernovae. The number h can be taken to be h = 0.7. It is a way of letting people adjust according to their latest figure for the Hubble parameter. If you think the right figure is 71 km/s per Mpc then use h = 0.71. So then you see that in the positive curvature case R > 22 h-1 Gpc. That is roughly 100 billion ly. Just a lower bound, could be much larger.