Energy solutions of KPZ are unique
By Massimiliano Gubinelli, Nicolas Perkowski. 2015
144 citations recorded by the source corpus.
The Kardar-Parisi-Zhang (KPZ) equation is conjectured to universally describe the fluctuations of weakly asymmetric interface growth. Here we provide the first intrinsic well-posedness result for the KPZ equation on the real line by showing that its energy solutions (as introduced by Gon\c{c}alves and Jara and later refined by Gubinelli and Jara) are unique. Together with various convergence results already present in the literature, this establishes the weak KPZ universality conjecture for a wide class of models. A remarkable consequence is that the energy solution to the KPZ equation is not equal to the Cole-Hopf solution, but it involves an additional drift $t/12$.
Subfields: Condensed Matter Physics, Mathematical Physics, Statistics and Probability
View Paper: https://www.semanticscholar.org/paper/a564d9bc74c29d9453997cf5f50b2fea12b1fac7
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Condensed Matter Physics
In Mathematical Physics
- Hendrik Weber
- Jean-Christophe Mourrat
- Massimiliano Gubinelli
- Martin Hairer
- Felix Otto
- Samy Tindel
- Antoine Gloria
- Peter K. Friz
In Statistics and Probability
- Hendrik Weber
- Jean-Christophe Mourrat
- Massimiliano Gubinelli
- Felix Otto
- Antoine Gloria
- Stefan Neukamm
Citations in the corpus
- The Dynamic $${\Phi^4_3}$$Φ34 Model Comes Down from Infinity (2016, methodology): “Related results were obtained for the KPZ equation, first in [2] via a Cole–Hopf transformation, and then, following [22], in a series of works including [11,17,19,20,27,29].”
- Lectures on singular stochastic PDEs (2015, methodology): “were able to prove that energy solutions for the stationary stochastic Burgers equation are unique. This topic will not be touched upon here. The interested reader can find the details in the preprint [GP15b]. 2.1 Distributions We will need to use distributions defined on the d-dimensional torus Td wh”