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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.

Topological Invariants in Higher-Dimensional Magnetohydrodynamics

TL;DR

The paper extends topological invariants of ideal MHD to higher dimensions by formulating the equations with differential forms on -dimensional manifolds and applying the Hodge–Morrey decomposition. It proves that in odd dimensions there exist generalized cross and magnetic helicities, while in even dimensions there is a whole family of enstrophy-like invariants for arbitrary . Additionally, for symmetric solutions in any dimension, a generalized mean-square magnetic potential invariant (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 , and families of invariants given by integrals of arbitrary functions of the scalar density of the magnetic field -form , where denotes its -fold wedge product and the fluid-density top form, in all even spatial dimensions . 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.

Paper Structure

This paper contains 21 sections, 16 theorems, 87 equations, 3 tables.

Key Result

Theorem 1.2

Let $\Omega$ be a compact and orientable $n$-dimensional Riemannian manifold with smooth boundary for $n\geq 2$ with trivial first and second cohomology groups. Then, smooth solutions $(\nu,u,B,h)$ to the ideal MHD equations eq: IMHD satisfying the boundary conditons $\boldsymbol{u}\cdot \boldsymbol where $A$ is a $1$-form satisfying $B=dA$. (ii) For $n=2m$, for arbitrary functions $f$.

Theorems & Definitions (44)

  • Theorem 1.2: Invariants in odd and even dimensions
  • Remark 1.3
  • Theorem 1.4: Generalized mean-square magnetic potential
  • Definition 2.1: Ideal MHD
  • Remark 2.2: The Lie--advection equation
  • Remark 2.3: The momentum balance
  • Remark 2.4: The Ampère's law
  • Remark 2.5: The closure condition
  • Remark 2.6: Relativistic MHD
  • Lemma 2.7: Hodge--Morrey decomposition
  • ...and 34 more