tkav,
no problem with your question! But it comes within the scope of ordinary classical GR and Cosmology. It is not really a "beyond the Standard Model" question.
Your question is a mix of on-target conceptions, and off-target. I'd say you have a good pictorial idea of how gravitational waves---ripples in geometry---can be made by massive bodies collapsing or orbiting each other rapidly.
But in the usual cosmo models there is no "EDGE" of the universe that could reflect waves back.
The "observable universe" is merely the part that we currently have the opportunity to see because light-etc has had time to reach us. The boundary of your observable is not a physical real boundary, it just depends on your location. So it can't reflect anything.
The currently observable portion is assumed to be just a small part of the whole thing, which could indeed be infinite. If the whole U is spatially finite then it still has no "EDGE" because it is all there is, so there is no "OUTSIDE". Picture the 2D analogy of the surface of a sphere. If all existence were concentrated on that 2D surface then there would be no edge.
Secondly, could dark energy simply be an effect of the relative weakness of gravity? Meaning that the energy in the universe left over from the big bang and rapid expansion is slightly above the maximum expansive energy gravity could overcome, and the larger the universe gets gravity gets "spread so thin" the expansion accelerates?
Could Dark Energy possibly be detected or explained by studying its effect on gravity?
Dark Matter (which is different, and collects in clouds) has been detected by its gravitational lensing effects. Concentrations of DM bend lightrays and distort the background galaxies.
You could say that Dark Energy has been "detected" primarily by measuring its effect on expansion of distances. You could say that this was an "effect on gravity" because it overcomes the tendency of gravity to slow expansion down. But that kind of detection still leaves a lot of questions and one wants more of an observational handle on DE.
I would not call DE merely "an effect of the relative weakness of gravity"---relative to the initial kick-off expansion. No matter how weak, gravity would still be slowing expansion down, not speeding it up!
The simplest explanation of DE is simply that it corresponds to a constant term in the law of gravity that we did not know was there until 1998.
Since 1915, our law of gravity has been the Einstein Field Equation, and that equation has a natural place in it for a constant Lambda. But until 1998 most people thought that constant was zero. Then they found evidence that it wasn't zero.
You don't really have to think of it as an "energy". It is just as natural to think of it as a very slight intrinsic spacetime curvature. That was how Lambda originally appeared in the equation.
"Dark" makes it sound mysterious, and "Energy" is a bit misleading---we don't know for sure that it corresponds to any field or to anything we would ordinarily consider an energy.
Media tend to hype stuff up---stimulate the public's imagination. Give the illusion that stuff is known when it is just one possible conjecture. there is a lot of uncertainty in Cosmology---things that could be understood and explained in several different ways--and where people need more observations to decide between the different models. that uncertainty would bore the audience and would not play well on television. So it doesn't come through in the media.
Here's a professional article that I like about "Dark Energy". You could see if you could read parts of it. Parts at the beginning and end are not too technical, I think. Here is the summary HTML. To get the full article, click on PDF in the upper right corner of this summary page:
http://arxiv.org/abs/1002.3966
Why all these prejudices against a constant?
Eugenio Bianchi, Carlo Rovelli
(Submitted on 21 Feb 2010 (v1), last revised 11 Apr 2010 (this version, v3))
The expansion of the observed universe appears to be accelerating. A simple explanation of this phenomenon is provided by the non-vanishing of the cosmological constant in the Einstein equations. Arguments are commonly presented to the effect that this simple explanation is not viable or not sufficient, and therefore we are facing the "great mystery" of the "nature of a dark energy". We argue that these arguments are unconvincing, or ill-founded.
9 pages, 4 figures