How Do Quantum Fluctuations Shape Cosmic Structures?

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SUMMARY

Quantum fluctuations play a critical role in the formation and evolution of cosmic structures on large scales. Research indicates that primordial quantum diffusion generates non-Gaussian, exponential tails in the distribution of inflationary perturbations, which significantly influence the likelihood of forming collapsed structures, including primordial black holes. These effects extend to very-large-scale structures, increasing the probability of heavy clusters like “El Gordo” and large voids associated with the cosmic microwave background cold spot.

PREREQUISITES
  • Understanding of quantum fluctuations in cosmology
  • Familiarity with inflationary perturbations
  • Knowledge of primordial black holes
  • Basic concepts of cosmic microwave background radiation
NEXT STEPS
  • Research the implications of non-Gaussian distributions in cosmology
  • Explore the role of primordial quantum diffusion in structure formation
  • Study the characteristics of heavy galaxy clusters like “El Gordo”
  • Investigate the cosmic microwave background cold spot and its significance
USEFUL FOR

Astronomers, cosmologists, and researchers interested in the interplay between quantum mechanics and large-scale structure formation in the universe.

Leandro Bolonini
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TL;DR
How do quantum fluctuations affect the formation and evolution of structures in the universe on large scales?
How do quantum fluctuations affect the formation and evolution of structures in the universe on large scales?
 
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That's quite a broad question. Have you done any research on this yourself?
 
@Leandro Bolonini An example paper exploring possible relations between primordial fluctuations and large-scale structures:

https://arxiv.org/abs/2207.06317
primordial quantum diffusion unavoidably generates non-Gaussian, exponential tails in the distribution of inflationary perturbations. These exponential tails have direct consequences for the formation of collapsed structures in the universe, as has been studied in the context of primordial black holes. We show that these tails also affect the very-largescale structures, making heavy clusters like “El Gordo”, or large voids like the one associated with the cosmic microwave background cold spot, more probable
 

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