G'day Apodman,
The picture you wrote down for a gravity well is the same as what i'm visualizing. In a 2D analogon: just a membrane that is stretched in two perpendicular directions. The gravity well is formed by the famous bowling ball Carl Sagan once used, lying on that membrane.
apodman wrote:Now my Physics is weak when you speak of expansion in terms of strain;
I will explain that. Please do not feel offended when the level of my explanation is rather basic. I might tell things you already knew.
Visualize a rubber band of 1 m long. Fix one end at a wall. Then apply sufficient force to the other end, that it will elongate to 1.1 m. Its extension is 0.1 m. The strain is the extension divided by the original length: 0.1m/1m = 0.1 [-]. Strain has no units, it is length divided by length.
Release the force and the rubber band will jump back to its original length of 1 m. Now fetch from your toolbox a motor with a gearbox. This motor will pull at the free end of the rubber band and stretch it with a velocity of 1 mm/s. When we let this motor run for 60 seconds, it will have extended the rubber band by 0.06 m, so its strain is 0.06. Since the motor has a constant speed, you can divide the strain by the time needed to create this strain: 0.06/60 s = 0.001 1/s. This is the strain rate: unit 1/s. You would have found the same answer if you would have divided the velocity of the motor by the length of the rubber band straight away: (1 mm/s) / 1m = 0.001 1/s.
Note the same type of division in the H0 Hubble constant:
70 km/s /Megaparsec = 2.5E-18 1/s.
you further wrote:but if you have a zone that is not expanding embedded in a zone that is expanding, doesn't there have to be strain at the transistion?
What you mean is a gradient in strain, a zone where there is a transition between the gravity dominated well and the "free" expansion of the space time fabric. What will follow is an oversimplification of the universe. Suppose the strain caused by the gravity well and the strain by the expansion of the space fabric both follow the rules of a linear elastic model. I know this is not true, follow my motto: "start simple, complicate later". From theorems of the theory of elasticity it is known that for a linear elastic material strains may be added up linearly.
As you might imagine, the strain caused by the gravity well is larger close to the center of the mass and it decreases if the distance to the center increases. This is a gradient in strain, and it is not easy to accomplish in a rubber band. The direction of the strain of the gravity well is opposite to the direction of the strain of the expanding space fabric. The latter is a constant.
Now suppose the strain of the gravity well can be mathematically approximated by: (this is far from the real shape, i do not know what particular shape it has)
gs(r) = -g0 /(r-rm)
where g0 is a constant depending on the mass, r is the distance between the center of the mass and a point in 'space' and rm is the radius of the mass. r > rm, otherwise it is nonsense. gs is the gravity strain. As you can see, if r gets bigger and bigger, gs(r) approaches 0. So at large distances from the mass, there is hardly any strain. Close to the mass there is a lot of influence.
The strain of the space fabric is (for simplicity sake) a constant, e.g. +fs (fabric strain).
Since we simplified space to a linear elastic material we can add up the strains.
gtotal = gs(r) + fs = -g0/ (r-rm) + fs.
Far away from the gravity well, the strain is fs, since gs approaches 0. There is a point r0, where the fabric strain is equal to minus the gravity strain:
r0 = rm + g0/fs.
At that point there is no strain. Closer than r0 to the mass the strain is negative, a gravity dominated region, further away than r0 the strain is positive, a fabric dominated region. If you look at the formula for gtotal, there is a smooth transition zone between both regions.
apodman wrote:I could learn to perform the necessary transformations on those 4x4 Cartesian tensors that carry gravity by trading a dose of time for a dose of x,y,z and plot the results, but I got a D in that course a long time ago. So it's left for someone else to visualize and me to appreciate.
That is definitively a "complicate later" excercise. My oversimplified description might help you visualize it in a much simpler way. Of coarse, the space fabric is not a linear elastic material. The gravity well is not linear, since Einstein needed non-linear tensor algebra to derive to its conclusions. So my numbers and shapes will not hold, it is more the general idea.
And you continued:
If a gravity well produces a node of unexpanded space, wouldn't something the size of a galaxy leave a trail of pinched space as it moves?
Visualize Carl Sagans bowling ball on bowling lane (made by a thin rubber membrane) speeding to the pins. As it moves, it indents the lane, but the lane jumps back when the ball has passed. And you were referring to the
peculiar velocity of the galaxy, not just velocity due to the general expansion.
Hope this help you visualize the expanding space fabric.