English

Wiener densities for the Airy line ensemble

Probability 2024-08-21 v4

Abstract

The parabolic Airy line ensemble A\mathfrak A is a central limit object in the KPZ universality class and related areas. On any compact set K={1,,k}×[a,a+t]K = \{1, \dots, k\} \times [a, a + t], the law of the recentered ensemble AA(a)\mathfrak A - \mathfrak A(a) has a density XKX_K with respect to the law of kk independent Brownian motions. We show that XK(f)=exp(S(f)+o(S(f))) X_K(f) = \exp \left(-\textsf{S}(f) + o(\textsf{S}(f))\right) where S\textsf{S} is an explicit, tractable, non-negative function of ff. We use this formula to show that XKX_K is bounded above by a KK-dependent constant, give a sharp estimate on the size of the set where XK<ϵX_K < \epsilon as ϵ0\epsilon \to 0, and prove a large deviation principle for A\mathfrak A. We also give density estimates that take into account the relative positions of the Airy lines, and prove sharp two-point tail bounds that are stronger than those for Brownian motion. These estimates are a key input in the classification of geodesic networks in the directed landscape. The paper is essentially self-contained, requiring only tail bounds on the Airy point process and the Brownian Gibbs property as inputs.

Keywords

Cite

@article{arxiv.2302.00097,
  title  = {Wiener densities for the Airy line ensemble},
  author = {Duncan Dauvergne},
  journal= {arXiv preprint arXiv:2302.00097},
  year   = {2024}
}

Comments

57 pages, 4 figures

R2 v1 2026-06-28T08:28:33.108Z