Inflation and density perturbations

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    Density Inflation
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SUMMARY

The discussion centers on the estimation of false vacuum decay rates in the inflationary universe through the analysis of density perturbations from the Big Bang. While there is a theoretical possibility that cosmic bubble collisions could be detected in the Cosmic Microwave Background (CMB), definitive evidence has yet to be found. The absence of detectable ring-like structures suggests that estimating decay rates from CMB data is unlikely. The relationship between the dynamics of phase transitions and density perturbations is emphasized, particularly in the context of first- or second-order transitions.

PREREQUISITES
  • Understanding of inflationary cosmology
  • Familiarity with Cosmic Microwave Background (CMB) analysis
  • Knowledge of phase transitions in quantum field theory
  • Basic concepts of density perturbations in cosmology
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  • Research cosmic bubble collisions and their implications for CMB observations
  • Study the dynamics of phase transitions in quantum field theory
  • Explore methods for analyzing density perturbations in cosmological models
  • Investigate the relationship between potential shapes and density perturbations
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Astronomers, theoretical physicists, and cosmologists interested in the implications of inflationary theory and the analysis of cosmic structures.

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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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