A particular type of dyadic model for the magnetohydrodynamics (MHD) with dominating forward energy cascade is studied. The model includes intermittency dimension δ in the nonlinear scales. It is shown that when δ is small, positive solution with large initial data for either the dyadic MHD or the dyadic Hall MHD model develops blow-up in finite time. Moreover, for a class of positive initial data with large velocity components and small magnetic field components, we prove that there exists a positive solution that blows up at a finite time.
Funding
Mathematical Analysis of Magnetohydrodynamic Flows with Hall Effect | Funder: National Science Foundation | Grant ID: DMS-2009422
Mathematical aspects of the magneto-hydrodynamics with Hall effect | Funder: National Science Foundation | Grant ID: DMS-1815069
Von Neumann Fellowship | Funder: Institute for Advanced Study
History
Citation
Dai, M. (2022). Blow-up of dyadic MHD models with forward energy cascade. International Mathematics Research Notices. https://doi.org/10.1093/imrn/rnac337