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.