How does the supercritical GMC converge?
Federico Bertacco, Martin Hairer
TL;DR
The paper advances the understanding of supercritical Gaussian multiplicative chaos by providing a stable, process-level description of the convergence of GMC measures built from a star-scale invariant log-correlated field. It achieves this through a detailed local analysis of extremal points, a Brownian-motion based reduction of the shape around mesoscopic maxima, and a resampling framework that yields a canonical limiting shape independent of conditioning thresholds. The main results characterize the limiting objects as a Poissonian superposition of atoms with random weights, governed by a weight process and the (critical) GMC, and they establish a joint Laplace functional that encodes the stable convergence of measure-valued processes across scales. These findings illuminate the freezing phenomenon in the supercritical regime and connect the continuum GMC to a structured, canonical limit akin to a stationary Ornstein–Uhlenbeck-type dynamics, with implications for the uniqueness and robustness of the limiting measure.
Abstract
In the spirit of [M. Biskup & O. Louidor, Adv. Math. 330 (2018)], we study the local structure of $\star$-scale invariant fields -- a class of log-correlated Gaussian fields -- around their extremal points by characterising the law of the "shape" of the field's configuration near such points. As a consequence, we obtain a refined understanding of the freezing phenomenon in supercritical Gaussian multiplicative chaos.
