Magnetic relaxation for the MHD equations via the stable manifold method

We prove that given any sufficiently small and regular solution $B$ of the stationary Euler equations there exists an infinite dimensional family of solutions $(u,b)$ of the non-resistive magnetohydrodynamics equations (MHD) that relax to $(0, B)$.

More precisely, $(u,b) \to (0, B)$ exponentially fast as $t \to +\infty$.

This family may be viewed as lying in the stable manifold of the non-resistive MHD equations around the equilibrium state $(0, B)$.

The problem whether it actually coincides with the stable manifold remains open.

As a byproduct of our result, we provide a large class of global regular solutions of the non-resistive MHD equations.

Another consequence is that any sufficiently small and regular solution of the stationary Euler equation is (non-trivially) topologically accessible via MHD from a large class of magnetic fields according to the definition of Moffatt and, in this scenario, the topology of the magnetic lines is (entirely) preserved in the limit $t \to + \infty$.