{"title":"Linear Fluctuation of Interfaces in Glauber–Kawasaki Dynamics","authors":"Tadahisa Funaki, Claudio Landim, Sunder Sethuraman","doi":"10.1007/s00220-026-05712-3","DOIUrl":null,"url":null,"abstract":"<div><p>In this article, we find a scaling limit of the space-time mass fluctuation field of Glauber + Kawasaki particle dynamics around its hydrodynamic mean curvature interface limit. Here, the Glauber rates are scaled by <span>\\(K=K_N\\)</span> (with <span>\\(K_N\\uparrow \\infty \\)</span> as <span>\\(N\\uparrow \\infty \\)</span>), the Kawasaki rates by <span>\\(N^2\\)</span> and space by 1/<i>N</i>. We start the process so that the continuum interface <span>\\(\\Gamma _t\\)</span> formed, between ‘high’ <span>\\(\\rho _+\\)</span> and ‘low’ <span>\\(\\rho _-\\)</span> density regions, is stationary that is, <span>\\(\\Gamma _t\\)</span> is ‘flat’. When the Glauber rates are balanced on <span>\\({\\mathbb {T}}^d\\)</span>, the interface <span>\\(\\Gamma _t=\\Gamma =\\{v: v_1=0\\}\\)</span> is immobile and the hydrodynamic limit is given by <span>\\(\\rho (t,v) = \\rho _+\\)</span> for <span>\\(v_1\\in (0,1/2)\\)</span> and <span>\\(\\rho (t,v)= \\rho _-\\)</span> for <span>\\(v_1\\in (-1/2,0)\\)</span> for all <span>\\(t\\ge 0\\)</span>, where <span>\\(v=(v_1,\\ldots ,v_d)\\in {\\mathbb {T}}^d\\)</span> identified with <span>\\([-1/2,1/2)^d\\)</span>. In the pre-limit setting, a boundary region of width <span>\\(O(1/\\sqrt{K_N})\\)</span> about the interface arises, where the density is more indeterminate than outside the region. Accordingly, we will scale the <span>\\(v_1\\)</span> coordinate in the fluctuation field by <span>\\(\\sqrt{K_N}\\)</span> so that the fluctuation field scaling limit will capture information ‘near’ the interface. We identify the fluctuation limit as a Gaussian field when <span>\\(K_N= O(\\sqrt{\\log (N)})\\)</span> in <span>\\(d\\le 2\\)</span>. In the one dimensional case, the field limit is given by <span>\\(\\textbf{e}(v_1) B_t\\)</span> where <span>\\(B_t\\)</span> is a Brownian motion and <span>\\(\\textbf{e}\\)</span> is the normalized derivative of a decreasing ‘standing wave’ solution <span>\\(\\phi \\)</span> of <span>\\(\\partial ^2_{v_1} \\phi - V'(\\phi )=0\\)</span> on <span>\\({\\mathbb {R}}\\)</span>, where <span>\\(V'\\)</span> is the homogenization of the Glauber rates. In two dimensions, the limit is <span>\\(\\textbf{e}(v_1)Z_t(v_2)\\)</span> where <span>\\(Z_t\\)</span> is the solution of a one dimensional stochastic heat equation. The appearance of the function <span>\\(\\textbf{e}(\\cdot )\\)</span> in the limit field indicates that the interface fluctuation retains the shape of the transition layer <span>\\(\\phi \\)</span>.\n</p></div>","PeriodicalId":522,"journal":{"name":"Communications in Mathematical Physics","volume":"407 11","pages":""},"PeriodicalIF":2.9000,"publicationDate":"2026-09-27","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1007/s00220-026-05712-3.pdf","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Communications in Mathematical Physics","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.1007/s00220-026-05712-3","RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"PHYSICS, MATHEMATICAL","Score":null,"Total":0}
引用次数: 0
Abstract
In this article, we find a scaling limit of the space-time mass fluctuation field of Glauber + Kawasaki particle dynamics around its hydrodynamic mean curvature interface limit. Here, the Glauber rates are scaled by \(K=K_N\) (with \(K_N\uparrow \infty \) as \(N\uparrow \infty \)), the Kawasaki rates by \(N^2\) and space by 1/N. We start the process so that the continuum interface \(\Gamma _t\) formed, between ‘high’ \(\rho _+\) and ‘low’ \(\rho _-\) density regions, is stationary that is, \(\Gamma _t\) is ‘flat’. When the Glauber rates are balanced on \({\mathbb {T}}^d\), the interface \(\Gamma _t=\Gamma =\{v: v_1=0\}\) is immobile and the hydrodynamic limit is given by \(\rho (t,v) = \rho _+\) for \(v_1\in (0,1/2)\) and \(\rho (t,v)= \rho _-\) for \(v_1\in (-1/2,0)\) for all \(t\ge 0\), where \(v=(v_1,\ldots ,v_d)\in {\mathbb {T}}^d\) identified with \([-1/2,1/2)^d\). In the pre-limit setting, a boundary region of width \(O(1/\sqrt{K_N})\) about the interface arises, where the density is more indeterminate than outside the region. Accordingly, we will scale the \(v_1\) coordinate in the fluctuation field by \(\sqrt{K_N}\) so that the fluctuation field scaling limit will capture information ‘near’ the interface. We identify the fluctuation limit as a Gaussian field when \(K_N= O(\sqrt{\log (N)})\) in \(d\le 2\). In the one dimensional case, the field limit is given by \(\textbf{e}(v_1) B_t\) where \(B_t\) is a Brownian motion and \(\textbf{e}\) is the normalized derivative of a decreasing ‘standing wave’ solution \(\phi \) of \(\partial ^2_{v_1} \phi - V'(\phi )=0\) on \({\mathbb {R}}\), where \(V'\) is the homogenization of the Glauber rates. In two dimensions, the limit is \(\textbf{e}(v_1)Z_t(v_2)\) where \(Z_t\) is the solution of a one dimensional stochastic heat equation. The appearance of the function \(\textbf{e}(\cdot )\) in the limit field indicates that the interface fluctuation retains the shape of the transition layer \(\phi \).
期刊介绍:
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