OK, now maybe this is a simple question, and I'm just thinking about it all mixed up. But it's been bugging me lately (too many Hubble telescope pictures I guess), and I know there are a few competent physics folk on this board, so here goes.
1) Standard "inflation" cosmology posits that the universe expands from a singularity.
2) Light (and other E-M) travels at a finite speed; the farther away something appears, the "older" it is.
3) Thus, if the Hubble limit were to somehow "catch up" to the point where we could see EM from the beginning of time, we would be looking back at the same point from all directions.
4) Spacetime seems therefore be curved, in the manner of a sphere, but 4-dimensional; similarly, any way you travel "North", you're going towards the North pole
but only if you follow the curvature of the earth.
5) So here's the situation:
X is the singularity event
O is the Observer planet (Earth?)
Ed and Fred are looking into space with their telescopes
from the north and south poles, respectively....
Ed
X---------<----O--->---------X
Fred
Both see X, by looking far enough into the past from
opposite directions. But X is a singularity!
Ed
/------<----O--->------\
| Fred |
v v
| |
\------>----X----<-----/
6) So couldn't we quantify, based on the "age" of the universe and the angular limit to which we could look "back in time" to see the same light repeated, just how curved space is in terms of radians per light-year, or some such?
7) A thought experiment, then: suppose you're living on a planet in a smaller universe which stopped expanding after, say, 10 years. Its Omega constant is 1.0, which IIRC means it reaches a stable inflationary state. You look out into space with your telescope and see the singularity after 10 years. 10 years after that, if you looked into the telescope again, you could see YOURSELF looking back at you 10 years ago! Is this an accurate description?