pHinds
sorry for all this, discard what you like..my last comments!
Regarding your Balloon Analogy website
I like it! Well done...It should get put in FAQ in these forums
[1] Should the balloon analogy be linked to the FLRW model?? I'm unsure.
Ich seems to think in a post here it is. I think you should mention there are not precise measures of distance and time in cosmology...we use conventions to allow us to make agreed upon measures, standard comparisons. But overall, the arbitray split between space and time of different observers leads to 'ambiguity' [using a word in the wiki reference].
Under "third local effect" :
The pennies don't change size (gravitationally bound systems don't expand and nothing inside of them expands), they just get farther apart and none of them are at the center.
Correct me, somebody, if I misinterpreted another thread discussion, but I thought that the FLRW model [homogeneous, isotropic] did NOT apply at galactic distances...too much lumpiness. In addition I thought nobody knows how to solve the EFE for representative galactic conditions...how to include the lumpiness in other words. So should we instead say something like 'gravitationally bound systems and things inside them are not thought to expand [or are generally not considered to exapnd] but we have no exact solution for such conditions. I'm not sure.
[3] In your description, Second Size shape:
Forget that the surface of the balloon is curved. That's NOT intended to be representative of the actual universe. It is actually more reasonable to think of a flat sheet of rubber that is being stretched equally in all directions.
Last sentence: Should this be qualified to space versus spacetime. Or say that curvature in time is not represented in the balloon analogy. We believe the universe is pretty flat spacewise, right? Is it time that is mostly curving on cosmological scales...or not??
[4] Cosmological Time: How do we say in a sentence or two, and should we bother here, that
Cosmological time is the elapsed time since the Big Bang according to the clock of an observer comoving with the CMBR ...[we use the cosmological time parameter of comoving coordinates because it's convenient mathematically. There are other time measures that could also be used.] In the Wikipedia link above, cosmological time, the 'age of the universe', is the like the time of light transit along the red curve, about 13B years, not the transit time along today's orange curve distance which is about 28B years.
[4] Under OTHER NOTES
How about a few sentences like this :
"Sending a light signal from one penny [galaxy] to another will take longer than if the pennies were stationary with respect to each other because the distances between them are increasing. [DUH!] Because the actual rate of expansion is not constant over all of cosmological time, the Hubble 'constant' varies over time since the big bang, and the actual transit time between pennies is different today than it was at earlier times. The current expansion of the universe proceeds in all directions as determined by the Hubble constant today, but it is a 'constant' in all directions of space not over time.