- #36
Chalnoth
Science Advisor
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My argument is vastly more basic than this, and isn't dependent upon a particular model of inflation. Point one is just based upon the general feature of inflation where any amount or sort of curvature is driven asymptotically flat due to the expansion. This doesn't mean that the universe becomes actually flat, just that the universe becomes so large that the curvature becomes unnoticeable.apeiron said:Right, so the assumption is of Linde style inflation with multiple local coolings and phase transitions into expanding universe-lets? And you are speaking of the shape of the whole?
Or this is a domain type argument. One single inflation event with multiple regions crystalising out with different local organisations around the same time?
If this is Lindean, then is natural to think of such a pre-bang realm as either flat and infinite in extent, or closed and connected? The other two options would seem to be fractal or locally hyperbolic.
Point two is just based upon another general feature of the universe where it appears that spontaneous symmetry breaking events appear to be part of our past, which would indicate that they happened differently elsewhere.