I Inflation and density perturbations

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Estimating the rate of false vacuum decay in the inflationary universe through density perturbations from the big bang is considered unlikely. While cosmic bubble collisions may be detectable in the cosmic microwave background (CMB), definitive evidence of such collisions has not been found. If these collisions were detected, they could help limit the number of false vacua and inform decay rates. The relationship between the phase transition dynamics and density perturbation characteristics is contingent on whether the transition is first- or second-order. Overall, current CMB data does not provide a reliable method for estimating false vacuum decay.
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Is it possible to estimate the rate of false vacuum decay in the inflationary universe by looking at the density perturbations in the big bang universe?
 
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Ranku said:
Is it possible to estimate the rate of false vacuum decay in the inflationary universe by looking at the density perturbations in the big bang universe?
Maybe, but it's unlikely.

There is the outside possibility that cosmic bubble collisions could be visible in the CMB. Here's a blog post about a paper that looks into this possibility:
https://www.earlyuniverse.org/simulating-cosmic-bubble-collisions-in-full-general-relativity/

So far, there hasn't been a definitive detection of the ring-like structure which would signal such a collision, so there probably won't ever be. If we had gotten lucky and could detect a number of these kinds of collisions, that would place limits on the number of false vacua in our past light cone, which might be useful in determining how often they decay. But with no detection, the answer is that it's probably impossible to know from the CMB data.
 
Depends. First- or second-order transition?

If the latter, then there is a direct connection between the shape of the potential, i.e. the dynamics of the phase transition, and the characteristics of the density perturbations.
 
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