wabbit
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I can't be positive but I'm pretty sure it doesn't, they describe it (and calculate it) as coming from an "ambiant" FRW metric. They mention vacuum bubbles before that, though they criticize that approach - but as I read it, what they really criticize is the patching of an external strict FRW solution to a bubble (they refer to that as Einstein–Straus and related solutions), which they show can work only at very large (galaxy cluster and above) scale. This is different from vacuum bubble+symmetry, the latter being a LTB, not FRW. But here too I can't truly follow their arguments so this is only an impression.PeterDonis said:Yes, exactly. I'm not sure their reasoning still applies in a bubble of empty space (possibly with a mass in the center of it) surrounded by spherically symmetric cosmological fluid.