On Global Dynamics of Three Dimensional Magnetohydrodynamics: Nonlinear Stability of Alfvén Waves

Magnetohydrodynamics (MHD) studies the dynamics of magnetic fields in electrically conducting fluids. In addition to the sound wave and electromagnetic wave behaviors, magneto-fluids also exhibit an interesting phenomenon: They can produce the Alfven waves, which were first described in a physics paper by Hannes Alfven in 1942. Subsequently, Alfven was awarded the Nobel prize for his fundamental work on MHD with fruitful applications in plasma physics, in particular the discovery of Alfven waves. This work studies (and constructs) global solutions for the three dimensional incompressible MHD systems (with or without viscosity) in strong magnetic backgrounds. We present a complete and self-contained mathematical proof of the global nonlinear stability of Alfven waves. Specifically, our results are as follows: We obtain asymptotics for global solutions of the ideal system (i.e.,viscosity \(\mu =0\)) along characteristics; in particular, we have a scattering theory for the system. We construct the global solutions (for small viscosity \(\mu \)) and we show that as \(\mu \rightarrow 0\), the viscous solutions converge in the classical sense to the zero-viscosity solution. Furthermore, we have estimates on the rate of the convergence in terms of \(\mu \). We explain a linear-driving decay mechanism for viscous Alfven waves with arbitrarily small diffusion. More precisely, for a given solution, we exhibit a time \(T_{n_0}\) (depending on the profile of the datum rather than its energy norm) so that at time \(T_{n_0}\) the \(H^2\)-norm of the solution is small compared to \(\mu \) (therefore the standard perturbation approach can be applied to obtain the convergence to the steady state afterwards). The results and proofs have the following main features and innovations: We do not assume any symmetry condition on initial data. The size of initial data (and the a priori estimates) does not depend on viscosity \(\mu \). The entire proof is built upon the basic energy identity. The Alfven waves do not decay in time: the stable mechanism is the separation (geometrically in space) of left- and right-traveling Alfven waves. The analysis of the nonlinear terms are analogous to the null conditions for non-linear wave equations. We use the (hyperbolic) energy method. In particular, in addition to the use of usual energies, the proof relies heavily on the energy flux through characteristic hypersurfaces. The viscous terms are the most difficult terms since they are not compatible with the hyperbolic approach. We obtain a new class of space-time weighted energy estimates for (weighted) viscous terms. The design of weights is one of the main innovations and it unifies the hyperbolic energy method and the parabolic estimates. The approach is ‘quasi-linear’ in nature rather than a linear perturbation approach: the choices of the coordinate systems, characteristic hypersurfaces, weights and multiplier vector fields depend on the solution itself. Our approach is inspired by Christodoulou–Klainerman’s proof of the nonlinear stability of Minkowski space-time in general relativity.