Small-scale properties of the KPZ equation and dynamical symmetry breaking
David Hochberg (LAEFF, Centro de Astrobiologia; Madrid), Carmen, Molina-Paris (Los Alamos), Juan Perez-Mercader (LAEFF, Centro de, Astrobiologia; Madrid), Matt Visser (Washington University in St Louis)

TL;DR
This paper investigates the short-distance behavior of the KPZ equation using a functional integral approach, revealing its renormalizability properties and dynamical symmetry breaking phenomena in lower dimensions.
Contribution
It introduces a one-loop effective potential analysis for the KPZ equation, demonstrating its renormalizability in 1-3 dimensions and identifying dynamical symmetry breaking in 1 and 2 dimensions.
Findings
Effective potential is one-loop ultraviolet renormalizable in 1-3 dimensions.
Dynamical symmetry breaking occurs in 1 and 2 dimensions.
No symmetry breaking in 3 dimensions.
Abstract
A functional integral technique is used to study the ultraviolet or short distance properties of the Kardar-Parisi-Zhang (KPZ) equation with white Gaussian noise. We apply this technique to calculate the one-loop effective potential for the KPZ equation. The effective potential is (at least) one-loop ultraviolet renormalizable in 1, 2, and 3 space dimensions, but non-renormalizable in 4 or higher space dimensions. This potential is intimately related to the probability distribution function (PDF) for the spacetime averaged field. For the restricted class of field configurations considered here, the KPZ equation exhibits dynamical symmetry breaking (DSB) via an analog of the Coleman-Weinberg mechanism in 1 and 2 space dimensions, but not in 3 space dimensions.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
