Topological Invariants in Higher-Dimensional Magnetohydrodynamics
Naoki Sato, Ken Abe, Michio Yamada
TL;DR
The paper extends topological invariants of ideal MHD to higher dimensions by formulating the equations with differential forms on $n$-dimensional manifolds and applying the Hodge–Morrey decomposition. It proves that in odd dimensions $n=2m+1$ there exist generalized cross and magnetic helicities, while in even dimensions $n=2m$ there is a whole family of enstrophy-like invariants $\mathscr{W}=\ int f\left(\frac{B^m}{\nu}\right)\nu$ for arbitrary $f$. Additionally, for symmetric solutions in any dimension, a generalized mean-square magnetic potential invariant $\mathscr{P}=\int_{\Sigma} f(A_n)\sigma$ (and its Euler analogue) is shown to be conserved, underscoring the role of symmetry in higher-dimensional topology. The work also develops gauge considerations, nontrivial Betti-number extensions, and the exact-form case, linking invariants to the underlying manifold’s cohomology and the Hodge–Morrey framework. Overall, these results provide a rigorous, geometry-driven suite of invariants that constrain higher-dimensional MHD dynamics and inform MHS equilibria analyses across dimensions.
Abstract
It is well known that the three-dimensional ideal magnetohydrodynamics (MHD) equations possess three magnetic invariants: (M) magnetic helicity, (C) cross helicity, and (P) the mean-square magnetic potential, in addition to the fundamental invariants of fluid motion. In this paper we construct higher-dimensional generalizations of these invariants for ideal MHD. Specifically, we identify generalized magnetic helicity and generalized cross helicity in all odd spatial dimensions $n=2m+1$, and families of invariants given by integrals of arbitrary functions of the scalar density $B^m/ν$ of the magnetic field $2$-form $B$, where $B^m$ denotes its $m$-fold wedge product and $ν$ the fluid-density top form, in all even spatial dimensions $n=2m$. We further establish the existence of invariants for symmetric solutions in arbitrary dimensions, generalizing the mean-square magnetic potential and showing that this invariant arises from symmetry rather than from even dimensionality, in contrast to the enstrophy invariant of the two-dimensional Euler equations.
