Nonlinear instability for the 3D MHD equations around the Taylor-Couette flow

Fuente: arXiv
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Auteurs principaux: Navarro-Fernández, Víctor, Villringer, David
Format: Preprint
Publié: 2025
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author Navarro-Fernández, Víctor
Villringer, David
author_facet Navarro-Fernández, Víctor
Villringer, David
contents We study the 3D magnetohydrodynamics (MHD) equations in an annular cylinder, perturbed around the explicit steady state given by the 3D Taylor-Couette velocity field and zero magnetic field. Combining a recent linear instability result for the magnetic field with the framework of Friedlander, Pavlović and Shvydkoy [Comm. Math. Phys. 264 (2006), no. 2, 335-347], we prove nonlinear instability of the solution around this steady state in $L^p$, for any $p>1$. In particular, our results are, to the best of our knowledge, the first rigorous instability results for 3D MHD without forcing, in which the instability is produced as a result of the (exponential) growth of the magnetic field. Furthermore, we offer a mathematical proof of the physically conjectured transfer of energy from the velocity field to the magnetic field in the MHD system.
format Preprint
id arxiv_https___arxiv_org_abs_2510_12707
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Nonlinear instability for the 3D MHD equations around the Taylor-Couette flow
Navarro-Fernández, Víctor
Villringer, David
Analysis of PDEs
We study the 3D magnetohydrodynamics (MHD) equations in an annular cylinder, perturbed around the explicit steady state given by the 3D Taylor-Couette velocity field and zero magnetic field. Combining a recent linear instability result for the magnetic field with the framework of Friedlander, Pavlović and Shvydkoy [Comm. Math. Phys. 264 (2006), no. 2, 335-347], we prove nonlinear instability of the solution around this steady state in $L^p$, for any $p>1$. In particular, our results are, to the best of our knowledge, the first rigorous instability results for 3D MHD without forcing, in which the instability is produced as a result of the (exponential) growth of the magnetic field. Furthermore, we offer a mathematical proof of the physically conjectured transfer of energy from the velocity field to the magnetic field in the MHD system.
title Nonlinear instability for the 3D MHD equations around the Taylor-Couette flow
topic Analysis of PDEs
url https://arxiv.org/abs/2510.12707