{"title":"On the Sobolev stability threshold for shear flows near Couette in 2D MHD equations","authors":"Ting Chen, Ruizhao Zi","doi":"10.1017/prm.2024.6","DOIUrl":null,"url":null,"abstract":"In this work, we study the Sobolev stability of shear flows near Couette in the 2D incompressible magnetohydrodynamics (MHD) equations with background magnetic field <jats:inline-formula> <jats:alternatives> <jats:tex-math>$(\\alpha,0 )^\\top$</jats:tex-math> <jats:inline-graphic xmlns:xlink=\"http://www.w3.org/1999/xlink\" mime-subtype=\"png\" xlink:href=\"S0308210524000064_inline1.png\" /> </jats:alternatives> </jats:inline-formula> on <jats:inline-formula> <jats:alternatives> <jats:tex-math>$\\mathbb {T}\\times \\mathbb {R}$</jats:tex-math> <jats:inline-graphic xmlns:xlink=\"http://www.w3.org/1999/xlink\" mime-subtype=\"png\" xlink:href=\"S0308210524000064_inline2.png\" /> </jats:alternatives> </jats:inline-formula>. More precisely, for sufficiently large <jats:inline-formula> <jats:alternatives> <jats:tex-math>$\\alpha$</jats:tex-math> <jats:inline-graphic xmlns:xlink=\"http://www.w3.org/1999/xlink\" mime-subtype=\"png\" xlink:href=\"S0308210524000064_inline3.png\" /> </jats:alternatives> </jats:inline-formula>, we show that when the initial datum of the shear flow satisfies <jats:inline-formula> <jats:alternatives> <jats:tex-math>$\\left \\| U(y)-y\\right \\|_{H^{N+6}}\\ll 1$</jats:tex-math> <jats:inline-graphic xmlns:xlink=\"http://www.w3.org/1999/xlink\" mime-subtype=\"png\" xlink:href=\"S0308210524000064_inline4.png\" /> </jats:alternatives> </jats:inline-formula>, with <jats:inline-formula> <jats:alternatives> <jats:tex-math>$N>1$</jats:tex-math> <jats:inline-graphic xmlns:xlink=\"http://www.w3.org/1999/xlink\" mime-subtype=\"png\" xlink:href=\"S0308210524000064_inline5.png\" /> </jats:alternatives> </jats:inline-formula>, and the initial perturbations <jats:inline-formula> <jats:alternatives> <jats:tex-math>${u}_{\\mathrm {in}}$</jats:tex-math> <jats:inline-graphic xmlns:xlink=\"http://www.w3.org/1999/xlink\" mime-subtype=\"png\" xlink:href=\"S0308210524000064_inline6.png\" /> </jats:alternatives> </jats:inline-formula> and <jats:inline-formula> <jats:alternatives> <jats:tex-math>${b}_{\\mathrm {in}}$</jats:tex-math> <jats:inline-graphic xmlns:xlink=\"http://www.w3.org/1999/xlink\" mime-subtype=\"png\" xlink:href=\"S0308210524000064_inline7.png\" /> </jats:alternatives> </jats:inline-formula> satisfy <jats:inline-formula> <jats:alternatives> <jats:tex-math>$\\left \\| ( {u}_{\\mathrm {in}},{b}_{\\mathrm {in}}) \\right \\| _{H^{N+1}}=\\epsilon \\ll \\nu ^{\\frac 56+\\tilde \\delta }$</jats:tex-math> <jats:inline-graphic xmlns:xlink=\"http://www.w3.org/1999/xlink\" mime-subtype=\"png\" xlink:href=\"S0308210524000064_inline8.png\" /> </jats:alternatives> </jats:inline-formula> for any fixed <jats:inline-formula> <jats:alternatives> <jats:tex-math>$\\tilde \\delta >0$</jats:tex-math> <jats:inline-graphic xmlns:xlink=\"http://www.w3.org/1999/xlink\" mime-subtype=\"png\" xlink:href=\"S0308210524000064_inline9.png\" /> </jats:alternatives> </jats:inline-formula>, then the solution of the 2D MHD equations remains <jats:inline-formula> <jats:alternatives> <jats:tex-math>$\\nu ^{-(\\frac {1}{3}+\\frac {\\tilde \\delta }{2})}\\epsilon$</jats:tex-math> <jats:inline-graphic xmlns:xlink=\"http://www.w3.org/1999/xlink\" mime-subtype=\"png\" xlink:href=\"S0308210524000064_inline10.png\" /> </jats:alternatives> </jats:inline-formula>-close to <jats:inline-formula> <jats:alternatives> <jats:tex-math>$( e^{\\nu t \\partial _{yy}}U(y),0)^\\top$</jats:tex-math> <jats:inline-graphic xmlns:xlink=\"http://www.w3.org/1999/xlink\" mime-subtype=\"png\" xlink:href=\"S0308210524000064_inline11.png\" /> </jats:alternatives> </jats:inline-formula> for all <jats:inline-formula> <jats:alternatives> <jats:tex-math>$t>0$</jats:tex-math> <jats:inline-graphic xmlns:xlink=\"http://www.w3.org/1999/xlink\" mime-subtype=\"png\" xlink:href=\"S0308210524000064_inline12.png\" /> </jats:alternatives> </jats:inline-formula>.","PeriodicalId":54560,"journal":{"name":"Proceedings of the Royal Society of Edinburgh Section A-Mathematics","volume":"10 1","pages":""},"PeriodicalIF":1.3000,"publicationDate":"2024-02-12","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Proceedings of the Royal Society of Edinburgh Section A-Mathematics","FirstCategoryId":"100","ListUrlMain":"https://doi.org/10.1017/prm.2024.6","RegionNum":3,"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
In this work, we study the Sobolev stability of shear flows near Couette in the 2D incompressible magnetohydrodynamics (MHD) equations with background magnetic field $(\alpha,0 )^\top$ on $\mathbb {T}\times \mathbb {R}$. More precisely, for sufficiently large $\alpha$, we show that when the initial datum of the shear flow satisfies $\left \| U(y)-y\right \|_{H^{N+6}}\ll 1$, with $N>1$, and the initial perturbations ${u}_{\mathrm {in}}$ and ${b}_{\mathrm {in}}$ satisfy $\left \| ( {u}_{\mathrm {in}},{b}_{\mathrm {in}}) \right \| _{H^{N+1}}=\epsilon \ll \nu ^{\frac 56+\tilde \delta }$ for any fixed $\tilde \delta >0$, then the solution of the 2D MHD equations remains $\nu ^{-(\frac {1}{3}+\frac {\tilde \delta }{2})}\epsilon$-close to $( e^{\nu t \partial _{yy}}U(y),0)^\top$ for all $t>0$.
期刊介绍:
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