Chiara Animali (Louvain U. and LPENS, Paris): Stochastic trees for stochastic inflation and primordial black hole formation
AlbaNova A5:1041 - CoPS grupprum
AlbaNova Main Building
Stochastic trees for stochastic inflation and primordial black hole formation
During inflation, quantum vacuum fluctuations are stretched beyond the Hubble radius, modifying the large-scale dynamics of the Universe. While their backreaction is negligible in the perturbative regime, it can become important in scenarios leading to primordial black hole (PBH) formation, where large density fluctuations are generated. The combination of stochastic inflation and the 𝛿N formalism provides an efficient framework to track these large fluctuations non-perturbatively. After reviewing the emergence of heavy non-Gaussian tails in the curvature perturbation distribution, I will show how large fluctuations are spatially correlated by computing real-space correlation functions within the stochastic-𝛿N approach. This can be used to characterise the spatial distribution of PBHs, revealing a universal clustering profile at their formation.
Place: CoPS room/A5:1041 and Zoom