Finite Time Singularities to the 3D Incompressible Euler Equations for Solutions in\(\:C^{\infty}(\mathbb{R}^3 \setminus \{0\})\cap C^{1,\alpha}\cap L^2\)
{"title":"Finite Time Singularities to the 3D Incompressible Euler Equations for Solutions in\\(\\:C^{\\infty}(\\mathbb{R}^3 \\setminus \\{0\\})\\cap C^{1,\\alpha}\\cap L^2\\)","authors":"Diego Córdoba, Luis Martinez-Zoroa, Fan Zheng","doi":"10.1007/s40818-025-00214-2","DOIUrl":null,"url":null,"abstract":"<div><p>We introduce a novel mechanism that reveals finite time singularities within the 1D De Gregorio model and the 3D incompressible Euler equations. Remarkably, we do not construct our blow up using self-similar coordinates, but build it from infinitely many regions with vorticity, separated by vortex-free regions in between. It yields solutions of the 3D incompressible Euler equations in <span>\\(\\mathbb{R}^3\\times [-T,0]\\)</span> such that the velocity is in the space <span>\\(C^{\\infty}(\\mathbb{R}^3 \\setminus \\{0\\})\\cap C^{1,\\alpha}\\cap L^2\\)</span> where <span>\\(0 < \\alpha \\ll 1\\)</span> for times <span>\\(t\\in (-T,0)\\)</span> and is not <span>\\(C^1\\)</span> at time 0.</p></div>","PeriodicalId":36382,"journal":{"name":"Annals of Pde","volume":"11 2","pages":""},"PeriodicalIF":2.6000,"publicationDate":"2025-07-07","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1007/s40818-025-00214-2.pdf","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Annals of Pde","FirstCategoryId":"100","ListUrlMain":"https://link.springer.com/article/10.1007/s40818-025-00214-2","RegionNum":1,"RegionCategory":"数学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"MATHEMATICS","Score":null,"Total":0}
引用次数: 0
Abstract
We introduce a novel mechanism that reveals finite time singularities within the 1D De Gregorio model and the 3D incompressible Euler equations. Remarkably, we do not construct our blow up using self-similar coordinates, but build it from infinitely many regions with vorticity, separated by vortex-free regions in between. It yields solutions of the 3D incompressible Euler equations in \(\mathbb{R}^3\times [-T,0]\) such that the velocity is in the space \(C^{\infty}(\mathbb{R}^3 \setminus \{0\})\cap C^{1,\alpha}\cap L^2\) where \(0 < \alpha \ll 1\) for times \(t\in (-T,0)\) and is not \(C^1\) at time 0.