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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?
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.
PREREQUISITESAstronomers, theoretical physicists, and cosmologists interested in the implications of inflationary theory and the analysis of cosmic structures.
Maybe, but it's unlikely.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?