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Typical field lines of Beltrami flows and boundary field line behaviour of Beltrami flows on simply connected, compact, smooth manifolds with boundary

Abstract

We characterise the boundary field line behaviour of Beltrami flows on compact, connected manifolds with vanishing first de Rham cohomology group. Namely we show that except for an at most nowhere dense subset of the boundary, on which the Beltrami field may vanish, all other field lines at the boundary are smoothly embedded 1-manifolds diffeomorphic to \({\mathbb {R}}\), which approach the zero set as time goes to \(\pm \, \infty\). We then drop the assumptions of compactness and vanishing de Rham cohomology and prove that for almost every point on the given manifold, the field line passing through the point is either a non-constant, periodic orbit or a non-periodic orbit which comes arbitrarily close to the starting point as time goes to \(\pm \infty\). During the course of the proof, we in particular show that the set of points at which a Beltrami field vanishes in the interior of the manifold is countably 1-rectifiable in the sense of Federer and hence in particular has a Hausdorff dimension of at most 1. As a consequence, we conclude that for every eigenfield of the curl operator, corresponding to a non-zero eigenvalue, there always exists exactly one nodal domain.

Introduction

In this paper, we deal with the field line behaviour of so-called Beltrami fields. Given an oriented, smooth Riemannian 3-manifold \(({\bar{M}},g)\) with or without boundary, we call a smooth vector field \(\varvec{X}\) on \({\bar{M}}\) a weak Beltrami field if there exists a locally bounded function \(\lambda :{\bar{M}}\rightarrow {\mathbb {R}}\) such that

$$\begin{aligned} \text {curl}(\varvec{X})=\lambda \varvec{X}\text { and }\text {div}(\varvec{X})=0. \end{aligned}$$
(1.1)

These type of vector fields appear naturally in physics. For instance, they provide stationary solutions of the equations of ideal magnetohydrodynamics for the case of constant pressure and a resting plasma [3, Chapter III], and are possible terminal magnetic field configurations for suitable initial magnetic fields. Beltrami fields, in fact, arise as local minimisers of the helicity constrained magnetic energy minimisation [2, 5, 36]. Hence, Beltrami fields are of interest in ideal magnetohydrodynamics, and in astrophysics in particular. On the other hand, we recall the usual form of the incompressible Euler equations

$$\begin{aligned} \partial _t\varvec{v}+\nabla _{\varvec{v}}\varvec{v}=-\nabla p\quad \text {and}\quad \text {div}(\varvec{v})=0, \end{aligned}$$

where \(\varvec{v}\) is the fluid velocity and p is the pressure. These equations can be written equivalently as

$$\begin{aligned} \partial _t\varvec{v}+\nabla f=\varvec{v}\times \text {curl}(\varvec{v})\quad \text {and}\quad \text {div}(\varvec{v})=0, \end{aligned}$$
(1.2)

with \(f:=\frac{g(\varvec{v},\varvec{v})}{2}+p\) being the Bernoulli function of the system. It follows that if \(\varvec{v}\) is a (time-independent) weak Beltrami field, then it is a solution of (1.2) for the pressure function \(p:=c-\frac{g(\varvec{v},\varvec{v})}{2}\) and any constant \(c\in {\mathbb {R}}\). Therefore, weak Beltrami fields may instead be interpreted as stationary solutions of the incompressible Euler equations. In fact, weak Beltrami fields are a very special kind of stationary solutions of the Euler equations. If we restrict ourselves to the case of stationary solutions of these equations, we arrive at the following PDE’s

$$\begin{aligned} \varvec{v}\times \text {curl}(\varvec{v})=\nabla f\text { and }\text {div}(\varvec{v})=0, \end{aligned}$$
(1.3)

for some function f. Assuming that all quantities involved are real analytic and that \(\varvec{v}\) and its curl are not everywhere collinear Arnold’s structure theorem [1,2,3 Chapter II Theorem 1.2, 19], provides a rather complete picture of the corresponding fluid flow. On the other hand, if \(\varvec{v}\) and its curl are everywhere collinear, which includes the case of weak Beltrami fields, the topological properties of the flow can be much more complicated. For instance, it is a consequence of Arnold’s structure theorem, see [3, Chapter II, proposition 6.2], that every no-where vanishing real analytic steady flow, which possesses a ’chaotic’ trajectory, i.e. a trajectory not contained in any two-dimensional subset, is necessarily a Beltrami field. Hence, the presence of complicated flowline topology already implies that the underlying flow must be Beltrami. Conversely there are Beltrami fields which have indeed complicated field line behaviour. The so-called ABC-flows (Arnold–Beltrami–Childress) develop for certain choices of their parameters chaotic field lines [10]. Etnyre and Ghrist showed in [15] that there exists a metric g on \(S^3\) and a Beltrami field corresponding to this metric such that this Beltrami field admits all knot and link types as its fields lines. A similar result regarding the Euclidean metric was obtained by Enciso and Peralta-Salas [11], who showed that there exists an eigenfield of the curl operator on \({\mathbb {R}}^3\) with the Euclidean metric, such that it admits all tame knots and (locally finite) links as field line configurations, see also [12]. These results have in common that one considers or constructs specific Beltrami fields with interesting topologies. But not all Beltrami fields have such complicated structures. Some of them behave just like ’typical’ steady flows to which Arnold’s structure theorem applies. For instance in [8], the authors explicitly compute all Beltrami fields on the solid ball in \({\mathbb {R}}^3\) which are tangent to its boundary. The eigenfield corresponding to the smallest positive eigenvalue indeed admits field lines which lie on invariant tori and the ball fibres into such invariant tori, after removing a lower dimensional subset from it. This is in essence the statement of the structure theorem. Contrary to the above results another question one may ask is:

Is there something we can say about the field line behaviour of all Beltrami fields (or some subclass) under certain assumptions on our manifold?

A typical question in this regards is whether or not Beltrami fields admit (non-constant) periodic orbits. Under certain assumptions, the answer is positive and a consequence of the (by now proven) Weinstein conjecture [25, 34], and the relation between Reeb vector fields and no-where vanishing, rotational Beltrami fields [14]. A rotational Beltrami field is a weak Beltrami field with smooth proportionality function \(\lambda\) which is no-where zero. Weinstein’s conjecture can then be stated as follows [14]: Every no-where vanishing, rotational Beltrami field on an oriented, closed (compact, without boundary) smooth, Riemannian 3-manifold (Mg) admits a periodic orbit. See also [13] for results concerning the existence of closed orbits of real analytic steady flows of the Euler equations on \(S^3\). Much less seems to be known about Beltrami flow behaviour on manifolds with non-empty boundary. For example [16, 17] deal with the existence of closed orbits of non-singular Beltrami fields defined on and tangent to the boundary of the solid torus.

In the present paper, we want to deal with the question posed above with a focus on manifolds with boundary. Our approaches are twofold.

First: We restrict our attention to Beltrami fields tangent to the (non-empty) boundary and analyse the field line behaviour on the boundary. The idea being that it is easier to understand dynamics on surfaces rather than in 3-space. The main observation is that the restriction of a given Beltrami field to the boundary satisfies the integrability conditions. In particular, if the boundary has a vanishing first de Rham cohomology group, the restricted vector field must be a gradient field whose dynamics are well understood. To ensure that the boundary is well-behaved, we make the assumptions of compactness and \(H^1_{dR}({\bar{M}})=\{0\}\) on the underlying manifold \({\bar{M}}\). But our results also hold true on non-compact manifolds with arbitrary de Rham cohomology groups, so as long as the boundary is well-behaved.

Second: We notice that the boundary is a two-dimensional subset and hence a null set. Thus, the typical field lines of Beltrami fields on manifolds with and without boundary should be the same. Hence, our idea is that it should be possible to characterise typical field lines. Indeed it is possible and in fact we will see that the boundary field line behaviour from the previous paragraph turns out to be atypical.

While characterising typical field lines, we will show that, given a weak Beltrami field \(\varvec{X}\), the set of points at which it vanishes on \({\bar{M}}\) has Hausdorff dimension at most 2. In addition, we will see that if we restrict ourselves to the interior of the manifold and assume that the proportionality function \(\lambda\) has bounded derivatives near the zero set, see Definition 2.1 for a precise statement, then the Hausdorff dimension is at most 1. This in particular includes the case of smooth proportionality function. The upper bound is sharp, as can be seen by considering the ABC-flows [2], with parameters \(A=-C=1\) and \(B=0\). The result regarding the Hausdorff dimension in the smooth proportionality function case is not new. In fact, it is a special case of a result by Bär concerning general elliptic operators of first order [6]. However, Bär’s result, even though more general, requires deeper technical tools, such as Malgrange’s preparation theorem, see for instance [30]. Our proof only uses the implicit function theorem and a unique continuation result by exploiting the specific structure of our equations. This provides an alternative, more elementary proof for our situation in the smooth proportionality function setting. But our result allows a more general class of proportionality functions so that, in this sense, we provide a generalisation of Bär’s results for our specific equations.

Note that if the proportionality function \(\lambda\) is a constant, then the corresponding weak Beltrami field \(\varvec{X}\) satisfies

$$\begin{aligned} \varDelta \varvec{X}=\lambda ^2 \varvec{X} \end{aligned}$$

since \(\text {div}(\varvec{X})=0\) and where we choose \(\varDelta\) to be a positive operator, i.e. it coincides in the Euclidean case with the negative of the standard Euclidean Laplacian. In the Euclidean case, each component of \(\varvec{X}\) is therefore an eigenfunction of the Laplacian and the zero set of \(\varvec{X}\) is exactly the intersection of the zero sets of the component functions. Zero sets \({\mathcal {N}}_f\) of eigenfunctions f of the Laplacian, also called nodal sets, as well as the connected components of their complement, so-called nodal domains, have been widely studied in mathematics, see for instance [22, 28, 32, 33] and see also [21] for a survey of properties of Laplacian eigenfunctions. The classical Courant’s nodal domain theorem [9, §5, p.365] states that the k-th-Dirichlet eigenfunction of the Laplacian on a bounded domain with smooth boundary in \({\mathbb {R}}^3\) admits at most k nodal domains (it is easy to show that there must be at least two, provided \(k\ge 2\)). It is then natural to ask the same question with regard to the curl operator.

Suppose \(\varvec{X}\) is an eigenfield of the curl operator, tangent to the boundary of \({\bar{M}}\). How many connected components does the set \(\text {int}({\bar{M}})\setminus \{\varvec{X}=0\}\) have?

We will show that the answer is simple, provided the corresponding eigenvalue is non-zero: It is always one component and in fact this holds regardless of the boundary conditions we impose.

Main results

Conventions Manifolds are assumed to be Hausdorff and second countable. All manifolds in question are assumed to be oriented, connected, \(C^{\infty }\)-smooth, with (possibly empty) boundary and are assumed to be equipped with a smooth Riemannian metric, unless specified otherwise. We will shortly write: ‘Let \(({\bar{M}},g)\) be a 3-manifold’ and mean by that, that \(({\bar{M}},g)\) has all the previously listed properties and is three-dimensional. If \({\bar{M}}\) is any smooth n-dimensional manifold with or without boundary with \(H^1_{dR}({\bar{M}})=\{0\}\), i.e. vanishing first de Rham cohomology group, then we call \({\bar{M}}\) a simple manifold. The set of all smooth vector fields on a given manifold \({\bar{M}}\) is denoted by \({\mathcal {V}}({\bar{M}})\). Given a smooth vector field \(\varvec{X}\in {\mathcal {V}}({\bar{M}})\) and a point \(p\in {\bar{M}}\), we denote by \(\gamma _p\) the field line of \(\varvec{X}\) starting at p and by \(\omega (p),\alpha (p)\) the corresponding \(\omega -\) and \(\alpha\)-limit sets. Recall that \(q\in \omega (p)\) if and only if there exists a sequence \((t_n)_n\), \(t_n\rightarrow +\infty\), such that \(\gamma _p(t_n)\rightarrow q\) and \(\alpha (p)\) is defined accordingly with limits \(t_n\rightarrow -\infty\). We call a vector field \(\varvec{X}\) on \(({\bar{M}},g)\) a weak \(C^k\)-Beltrami field, if it is of class \(C^k\) and there exists a locally bounded function \(\lambda :{\bar{M}}\rightarrow {\mathbb {R}}\), such that \(\text {curl}(\varvec{X})=\lambda \varvec{X}\) and \(\text {div}(\varvec{X})=0\).

Theorem 2.1

Let \({({\bar{\rm{M}}},{\rm{g}})}\) be a compact, simple 3-manifold with non-empty boundary \(\partial {\bar{M}}\ne \emptyset\) and let further \(\varvec{X}\in {\mathcal {V}}({\bar{M}})\) be a weak Beltrami field. If \(\varvec{X}\) is tangent to the boundary and not the zero vector field, then the following holds

  1. (i)

    \(K:=\{p\in \partial {{\bar{M}}}|\varvec{X}(p)=0 \}\) is a closed and no-where dense subset of \(\partial {\bar{M}}\). Equivalently \(U:=\partial {\bar{M}}\setminus K\) is an open and dense subset of \(\partial {\bar{M}}\).

  2. (ii)

    The (globally defined) field lines \(\gamma _p\) of \(\varvec{X}\) starting at points \(p\in U\subset \partial {\bar{M}}\) satisfy the following two properties:

    1. (a)

      The images \(\gamma _p({\mathbb {R}})\subset \partial {\bar{M}}\) are smoothly embedded 1-submanifolds diffeomorphic to \({\mathbb {R}}\).

    2. (b)

      The \(\omega\)- and \(\alpha\)-limit sets of any such field line are non-empty and subsets of K. Both limit sets consist either of a single point or of infinitely many points, none of which is an isolated point in \(\partial {\bar{M}}\).

  3. (iii)

    On each connected component of \(\partial {\bar{M}}\), \(\varvec{X}\) has at least two singular points.

Corollary 2.1

(Boundary field line behaviour of Beltrami fields on simple 3-manifolds) Let \(({\bar{M}},g)\) be a compact, simple 3-manifold with non-empty boundary and suppose \(\varvec{X}\in {\mathcal {V}}({\bar{M}})\) is a weak Beltrami field, which is tangent to the boundary and has at most finitely many non-isolated zeros in \(\partial {\bar{M}}\). If we let K and U be defined as in Theorem 2.1, then for any \(p\in U\), the field line \(\gamma _p\) of \(\varvec{X}\) starting at p is a smooth embedding of \({\mathbb {R}}\) into \(\partial {\bar{M}}\) (and hence also into \({\bar{M}}\)) and there exist elements \(p_{\pm }\in K\) such that \(\lim _{t\rightarrow \pm \infty }\gamma _p(t)=p_{\pm }\).

Here we mean by (non-)isolated in \(\partial {\bar{M}}\) that we consider these notions in the subspace topology of \(\partial {\bar{M}}\). The fact that the set K has no interior points is a consequence of the following result

Lemma 2.1

(Vainshtein’s lemma for abstract manifolds) Let \(({\bar{M}},g)\) be a 3-manifold with non-empty boundary and \(\varvec{X}\) a weak \(C^1\)-Beltrami field. If there exists an open subset \(U\subseteq {\bar{M}}\), such that \(\partial {\bar{M}}\cap U\ne \emptyset\) and \(\varvec{X}|_{\partial {\bar{M}}\cap U}\equiv 0\), then \(\varvec{X}\) is the zero vector field, i.e. \(\varvec{X}\equiv 0\) on all of \({\bar{M}}\).

A proof of Lemma 2.1 for the case of bounded domains with smooth boundary in \({\mathbb {R}}^3\) can be found in [7], see also [35] for the original reference. However, their proof relies on the position vector field. Thus, it does not immediately generalise to abstract manifolds. Here we use a different approach via the double of a manifold and a unique continuation result, inspired by the proof of [31, Theorem 3.4.4]. In particular, we do not need to assume that \({\bar{M}}\) is compact.

In order to show that the boundary is well-behaved in a suitable sense, given our assumptions on \({\bar{M}}\), we will first prove the following result

Lemma 2.2

Let \(n\ge 2\) and \({\bar{M}}\) be a compact, orientable, smooth n-dimensional manifold with non-empty boundary. Then for every fixed \(0\le k \le n-2\) we have the following implication

$$\begin{aligned} H^{(n-1)-k}_{dR}({\bar{M}})=\{0\} \Rightarrow \dim \left( H^k_{dR}\left( \partial {\bar{M}}\right) \right) \le \dim \left( H^k_{dR}\left( {\bar{M}}\right) \right) . \end{aligned}$$
(2.1)

This implies the following characterisation of the boundary of compact, simple manifolds

Corollary 2.2

Let \({\bar{M}}\) be a compact, orientable, simple, smooth three-dimensional manifold with non-empty boundary. Then every connected component of \(\partial {\bar{M}}\) is diffeomorphic to \(S^2\).

Now let us turn to the characterisation of typical field lines of weak Beltrami flows

Theorem 2.2

Let \({({\bar{\rm{M}}},{\rm{g}})}\) be a 3-manifold of finite volume and let \(\varvec{X}\in {\mathcal {V}}({\bar{M}})\) be a weak Beltrami field, which is tangent to the boundary of \({\bar{M}}\) and generates a global flow. If \(\varvec{X}\) is not the zero vector field, then the following holds

  1. (i)

    \(U_B:=\partial {\bar{M}}\setminus \{p\in \partial {\bar{M}}| \varvec{X}(p)=0 \}\) is an open and dense subset of \(\partial {\bar{M}}\).

  2. (ii)

    Let \({\mathcal {F}}:=\{p\in {\bar{M}}| p\in \omega (p)\cap \alpha (p)\text { and }\gamma _p \text { is not constant} \}\). Then \({\bar{M}}\setminus {\mathcal {F}}\) is a null set.

Corollary 2.3

(Typical field lines of weak Beltrami fields) Let \(({\bar{M}},g)\) be a 3-manifold of finite volume and \(\varvec{X}\in {\mathcal {V}}({\bar{M}})\) a weak Beltrami field, which is tangent to the boundary and generates a global flow. If \(\varvec{X}\) is not the zero vector field, then for almost every \(p\in {\bar{M}}\), the field line \(\gamma _p\) starting at p is either a non-constant periodic orbit, or \(\gamma _p\) is not periodic and there exist sequences \(t^{\pm }_n\rightarrow \pm \infty\) with \(\lim _{n\rightarrow \infty }\gamma _p(t^{\pm }_n)=p\).

Comparing Corollary 2.1 with the typical field line behaviour derived in Corollary 2.3 we see that the boundary field lines are either constant or non-periodic and whenever they are not periodic there do not exist any points on the field lines themselves which are \(\omega\) or \(\alpha\) limit points. Hence, all boundary field lines in the case of simple, compact 3-manifolds are atypical. Since the boundary is a null set, this, of course, is no contradiction.

Before stating the next result, we give a definition. Note that it immediately follows from definition of a weak Beltrami field \(\varvec{X}\) that the proportionality function \(\lambda\) is smooth away from the set of points at which \(\varvec{X}\) vanishes, i.e. \(\lambda \in C^{\infty }({\bar{M}}\setminus K)\) with \(K=\{p\in {\bar{M}}|\varvec{X}(p)=0\}\).

Definition 2.1

Let \(({\bar{M}},g)\) be a 3-manifold and \(\varvec{X}\in {\mathcal {V}}({\bar{M}})\) be a weak Beltrami field with proportionality function \(\lambda\) and let \(K:=\{p\in {\bar{M}}|\varvec{X}(p)=0\}\). We say that \(\lambda\) is \(C^{\infty }\)-bounded near K if for every \(p\in K\), there exists a chart \((\mu ,U)\) around p, such that for every multi-index \(\alpha \in {\mathbb {N}}^3_0\) we have \(\left\| \partial ^{\alpha }\left( \lambda \circ \mu ^{-1}\right) \right\| _{L^{\infty }(\mu (U\setminus K))}<\infty\), where we use the standard multi-index notation.

The defined notion is chart independent in the sense that if \((\mu ,U)\) is any chart around some \(p\in K\) with the described property and \(({\tilde{\mu }},{\tilde{U}})\) is another chart around p, then after shrinking \({\tilde{U}}\), if necessary, the \(L^{\infty }\) norms of the \({\tilde{\mu }}\) local expressions stay finite as well. Of course, whenever \(\lambda \in C^{\infty }({\bar{M}})\), then it is also \(C^{\infty }\)-bounded near K. The set \(U\setminus K\) may (a priori) be empty, which is for instance the case when \(\varvec{X}\) is the zero vector field. In that case, we set the \(L^{\infty }\)-norm to zero by convention.

The results of Theorem 2.2 rely on the following

Proposition 2.1

Let \(({\bar{M}},g)\) be a 3-manifold and \(\varvec{X}\in {\mathcal {V}}({\bar{M}})\) be a weak Beltrami field, which is not the zero vector field. Then the set \(K:=\{p\in {\bar{M}}| \varvec{X}(p)=0 \}\) is countably 2-rectifiable and hence has a Hausdorff dimension of at most 2. In particular, it is a null set. If the proportionality function \(\lambda :{\bar{M}}\rightarrow {\mathbb {R}}\) is \(C^{\infty }\)-bounded near K, then the set \(K_I:=\{p\in \text {int}({\bar{M}})| \varvec{X}(p)=0 \}\) is countably 1-rectifiable and thus has a Hausdorff dimension of at most 1.

Here we equip \(({\bar{M}},g)\) with the standard geodesic metric \(d_g\) induced by g [27, Theorem 2.55] and the Hausdorff dimension is considered with respect to this metric. We do not require in Proposition 2.1 that \(\varvec{X}\) is tangent to the boundary nor do we demand that \(({\bar{M}},g)\) has finite volume. As a consequence, we obtain

Corollary 2.4

Let (Mg) be a 3-manifold with empty boundary and let \(\varvec{X}\in {\mathcal {V}}(M)\) be a weak Beltrami field whose proportionality function is \(C^{\infty }\)-bounded near \(K:=\{p\in M| \varvec{X}(p)=0\}\). If \(\varvec{X}\) is not the zero vector field, then \(M\setminus K\) is path-connected, i.e. there is exactly one nodal domain.

The preceding corollary follows immediately from Proposition 2.1 and the following result

Proposition 2.2

Let (Mg) be a connected, smooth Riemannian n-dimensional manifold without boundary, \(n\ge 2\), and \(A\subseteq M\) be a closed subset whose Hausdorff dimension is strictly less than \((n-1)\), then \(M\setminus A\) is path-connected.

Proof of Theorem 2.1

We will first prove Lemma 2.1 and Corollary 2.2 and then explain how they imply Theorem 2.1.

Proof of Lemma 2.1: We observe that the interior of a manifold \(M:=\text {int}({\bar{M}})\) is homotopy equivalent to the manifold itself [26, Theorem 9.26], and since connectedness is a homotopy invariant we conclude that M is also connected. Now let \({\hat{M}}:= M\cup \left( \partial {\bar{M}}\cap U\right)\). Since \(\partial {\bar{M}}\cap U\) is an open subset of the boundary, we see that \({\hat{M}}\) is a manifold with non-empty boundary in its own right. Observe that \(M\subset {\hat{M}}\subseteq {\bar{M}}=\text {clos}(M)\), where \(\text {clos}(M)\) denotes the topological closure of M in \({\bar{M}}\). Since M is connected, so must be \({\hat{M}}\). Now consider the boundaryless double \(2{\hat{M}}\) of \({\hat{M}}\) [26, Theorem 9.29, Example 9.32], which is an orientable connected manifold without boundary into which \({\hat{M}}\) can be embedded such that the embedding is orientation preserving and such that \({\hat{M}}\) is a closed subset of the double. In particular, the topological boundary of \({\hat{M}}\) in \(2{\hat{M}}\) coincides with its manifold boundary. We can then equip the embedded copy of \({\hat{M}}\) with the pullback metric and extend it to a smooth metric on the whole double (the upcoming arguments are independent of the chosen extension). Then we can pushforward the vector field \(\varvec{X}\) to its embedded copy and extend it by 0 outside the copy. Observe that \(\text {div}(\varvec{X})=0\) and hence the divergence in particular vanishes at the boundary. Further \(\varvec{X}\) vanishes on the boundary of \({\hat{M}}\) and since it is a weak Beltrami field by assumption, we see that its curl also vanishes on the boundary of \({\hat{M}}\). From this, it follows that the vector field on the double which we extended by 0 defines a \(C^1\)-vector field on the double, see also [31, Theorem 3.4.4] for more details. One then readily checks that this extended vector field (after being identified with a 1-form via the Riemannian metric) satisfies the requirements of a unique continuation result [31, Theorem 3.4.3] and [4]. Since it vanishes identically on an open subset of the double (the complement of \({\hat{M}}\)), we conclude that \(\varvec{X}\) vanishes identically on all of \({\hat{M}}\) and in particular on M. Since M is dense in \({\bar{M}}\) and \(\varvec{X}\) is continuous we see that \(\varvec{X}\) vanishes identically on all of \({\bar{M}}\). \(\square\)

Proof of Lemma 2.2: Let us first introduce the space of smooth k-forms with relative boundary conditions \(\varOmega ^k_D({\bar{M}}):=\{\omega \in \varOmega ^k({\bar{M}})|\iota ^{\#}\omega =0 \}\), where \(\varOmega ^k({\bar{M}})\) denotes the space of all smooth k-forms on \({\bar{M}}\), \(\iota :\partial {\bar{M}}\rightarrow {\bar{M}}\) denotes the inclusion map and \(\iota ^{\#}\) the pullback with respect to this map. We note that \(0=d\iota ^{\#}\omega =\iota ^{\#}d\omega\) for every \(\omega \in \varOmega ^k_D({\bar{M}})\), so that \(d:\varOmega ^k_D({\bar{M}})\rightarrow \varOmega ^{k+1}_D({\bar{M}})\) is well-defined and gives rise to the so-called relative de Rham cohomology group, denoted by \(H^k_r({\bar{M}})\), see also [31, Chapter 2.6] for a concise discussion regarding the connections of distinct notions of de Rham cohomology groups. Letting \(\text {Id}:\varOmega ^k_D({\bar{M}})\rightarrow \varOmega ^k({\bar{M}}),\text { }\omega \mapsto \omega\) and observing that each \(\alpha \in \varOmega ^k(\partial {\bar{M}})\) may be extended by means of a collar neighbourhood construction to a smooth form \({\tilde{\alpha }}\in \varOmega ^k({\bar{M}})\) with \(\iota ^{\#}{\tilde{\alpha }}=\alpha\), we see that the following gives rise to a short exact sequence

$$\begin{aligned} 0\rightarrow \varOmega ^k_D({\bar{M}})\xrightarrow {\text {Id}}\varOmega ^k({\bar{M}})\xrightarrow {\iota ^{\#}}\varOmega ^k(\partial {\bar{M}})\rightarrow 0. \end{aligned}$$

It then follows from the zigzag lemma [26, Lemma 17.40], that the upcoming is part of an exact sequence as well

$$\begin{aligned} \dots \rightarrow H^k_{dR}({\bar{M}})\xrightarrow {\iota ^{\#}}H^k_{dR}(\partial {\bar{M}})\xrightarrow {\psi } H^{k+1}_r({\bar{M}})\rightarrow \dots \end{aligned}$$
(3.1)

for a suitable linear map \(\psi\). It now follows from [31, Corollary 2.6.2 (b)] and our assumption that \(H^{k+1}_r({\bar{M}})\cong H^{(n-1)-k}_{dR}({\bar{M}})=\{0\}\). By exactness of the sequence (3.1), we must then have \(\text {Im}(\iota ^{\#})=\text {Ker}(\psi )=H^k_{dR}(\partial {\bar{M}})\), i.e. there exists an epimorphism between \(H^k_{dR}({\bar{M}})\) and \(H^k_{dR}(\partial {\bar{M}})\). \(\square\)

Proof of Corollary 2.2: Choose \(n=3\), \(k=1\) in Lemma 2.2, then \((n-1)-k=1\) and by assumption \({\bar{M}}\) is simple, i.e. \(H^1_{dR}({\bar{M}})=\{0\}\). Thus, we conclude \(\dim \left( H^1_{dR}(\partial {\bar{M}})\right) \le \dim \left( H^1_{dR}({\bar{M}})\right) =0\) or in other words \(H^1_{dR}\left( \partial {\bar{M}}\right) =\{0\}\). Observe that since \({\bar{M}}\) is compact and orientable, so is \(\partial {\bar{M}}\) and that \(\partial {\bar{M}}\) is a two-dimensional smooth manifold without boundary. Hence, any connected component S of \(\partial {\bar{M}}\) is a connected, orientable, closed, two-dimensional smooth manifold. By the classification theorem for compact surfaces [24, Chapter 9, Theorem 3.5], we know that its diffeomorphy type is entirely characterised by its Euler characteristic. The Euler characteristic of S may be computed via

$$\begin{aligned} \chi (S)=\sum _{i=0}^2(-1)^i\dim \left( H^i_{dR}(S)\right) . \end{aligned}$$

By connectedness of S, we have \(\dim \left( H^0_{dR}(S)\right) =1\). Since \(H^1_{dR}(\partial {\bar{M}})=\{0\}\), we have in particular \(\dim \left( H^1_{dR}(S)\right) =0\) and finally since S is compact, connected and orientable, \(\dim \left( H^2_{dR}(S)\right) =1\) [26, Theorem 17.31]. Hence, we have \(\chi (S)=2\) and therefore S is diffeomorphic to \(S^2\). \(\square\)

Proof of Theorem 2.1: The first statement of Theorem 2.1 is just a direct application of Lemma 2.1. The key in proving the last two statements is the following simple observation: Let \(\omega ^1_{\varvec{X}}\) denote the 1-form identified with \(\varvec{X}\) via the Riemannian metric. The fact that \(\varvec{X}\) is a weak Beltrami field translates to the language of forms as

$$\begin{aligned} \star d\omega ^1_{\varvec{X}}=\lambda \omega ^1_{\varvec{X}}\text { and }\delta \omega ^1_{\varvec{X}}=0. \end{aligned}$$
(3.2)

Since we assume \(\varvec{X}\) to be tangent to the boundary, its normal part vanishes, i.e. in particular \(n(\star d\omega ^1_{\varvec{X}})=\lambda n(\omega ^1_{\varvec{X}})=0\). Due to the duality relations \(\star t=n\star\) between the normal part n and the tangent part t [31, Proposition 1.2.6], we conclude \(t(d\omega ^1_{\varvec{X}})=0\) or equivalently \(\iota ^{\#}d\omega ^1_{\varvec{X}}=0\). Since the pullback commutes with the exterior derivative, we obtain

$$\begin{aligned} d\iota ^{\#}\omega ^1_{\varvec{X}}=0. \end{aligned}$$
(3.3)

Now observe that since \(\varvec{X}\) is tangent to the boundary, we can restrict it to the boundary and obtain a smooth vector field \(\varvec{X}_B\in {\mathcal {V}}(\partial {\bar{M}})\). If we now equip \(\partial {\bar{M}}\) with the pullback metric \(g_B:=\iota ^{\#}g\), then we have the identity

$$\begin{aligned} \iota ^{\#}\omega ^1_{\varvec{X}}=\omega ^{1,g_B}_{\varvec{X}_B}, \end{aligned}$$

where \(\omega ^{1,g_B}_{\varvec{X}_B}\) is the one form identified with \(\varvec{X}_B\) via the metric \(g_B\) on \(\partial {\bar{M}}\). Hence, we obtain from (3.3)

$$\begin{aligned} d\omega ^{1,g_B}_{\varvec{X}_B}=0. \end{aligned}$$
(3.4)

This means that \(\varvec{X}_B\) satisfies the necessary integrability conditions on \(\partial {\bar{M}}\).

Remark

Observe that up to this point we haven’t made use of the compactness and simplicity assumptions on \({\bar{M}}\).

Since we assume \({\bar{M}}\) to be compact and simple, we conclude from Corollary 2.2 and (3.4) that \(\omega ^{1,g_B}_{\varvec{X}_B}\) is exact, i.e. there exists a smooth function \(f:\partial {\bar{M}}\rightarrow {\mathbb {R}}\) such that

$$\begin{aligned} X_B=\text {grad}(f)\text { with respect to the metric }g_B. \end{aligned}$$
(3.5)

The field line behaviour of gradient flows is well-understood, see for instance [23, Part I, Chapter 1.6], so that the last two statements of Theorem 2.1 follow from the gradient structure in combination with the following elementary lemma (whose proof we omit)

Lemma 3.1

Let M be a smooth n-dimensional manifold without boundary and let \(\varvec{Y}\in {\mathcal {V}}(M)\). Given \(p\in M\), let \(\gamma _p:I\rightarrow M\) denote the maximal integral curve starting at p with \(I=(a,b)\) for suitable \(-\infty \le a<0<b\le +\infty\). Then \(\gamma _p\) is exactly one of the following four types of curves

  1. (i)

    The image \(\gamma _p(I)\) is a point. In this case \(I={\mathbb {R}}\) and \(\gamma _p\) is constant.

  2. (ii)

    The image \(\gamma _p(I)\) is a smoothly embedded, compact 1-submanifold diffeomorphic to \(S^1\). In this case \(I={\mathbb {R}}\) and there exists a smallest positive number \(T>0\) such that \(\gamma _p(t+T)=\gamma _p(t)\) for all \(t\in {\mathbb {R}}\). T is called the period of \(\gamma _p\).

  3. (iii)

    The image \(\gamma _p(I)\) is a smoothly embedded 1-submanifold diffeomorphic to \({\mathbb {R}}\). In this case \(\gamma _p:I\rightarrow \gamma _p(I)\) is a diffeomorphism.

  4. (iv)

    \(\gamma _p(I)\) is not a smoothly embedded 1-submanifold and not a point. In that case, there exists some \(x\in \gamma _p(I)\) and a sequence \((t_k)_k\subset I\) with \(t_k\uparrow b\) or \(t_k\downarrow a\) and \(\gamma _p(t_k)\rightarrow x\) as \(k\rightarrow \infty\).

Observe also that we assume \({\bar{M}}\) to be compact and \(\varvec{X}\) to be tangent. Hence, \(\varvec{X}\) has a globally defined flow [26, Theorem 9.34]. \(\square\)

Remark 3.1

  1. (i)

    As we have seen, the restriction of \(\varvec{X}\) to any given boundary component always satisfies the necessary integrability conditions. Thus, as long as the boundary component has a vanishing first de Rham cohomology, the restricted vector field will still turn out to be a gradient field and similar conclusions can be drawn. For instance, if we consider the complement of the open unit ball in \({\mathbb {R}}^3\) and a weak Beltrami field on this manifold tangent to its boundary. Then its restriction to the unit sphere shows exactly the same behaviour as described in Theorem 2.1.

  2. (ii)

    For the proof of Theorem 2.1, it was enough to have Lemma 2.2 at hand to conclude that \(H^1_{dR}(\partial {\bar{M}})=\{0\}\) and hence the restricted vector field is a gradient field. Nonetheless, the implication, Corollary 2.2, is worth stating.

  3. (iii)

    Corollary 2.1 is an immediate consequence of Theorem 2.1.

Proof of Theorem 2.2

The first statement of Theorem 2.2 is a direct consequence of Lemma 2.1. Either \(\partial {\bar{M}}\) is empty, in which case \(U_B\) is empty as well and then obviously satisfies the conclusion. Or \(\partial {\bar{M}}\) is not empty, in which case the conclusion follows from Lemma 2.1. Thus, we focus here on the second statement of Theorem 2.2. To this end, let us first recall some notions for the convenience of the reader.

Definition 4.1

(Null sets on manifolds) A subset \(N\subseteq {\bar{M}}\) of a smooth n-dimensional manifold \({\bar{M}}\) with or without boundary is called a null set if there exists an atlas \({\mathcal {A}}\) of \({\bar{M}}\) such that for every chart \(\mu :U\rightarrow \mu (U)\) in \({\mathcal {A}}\) the set \(\mu (U\cap N)\) is a Lebesgue null set of \({\mathbb {R}}^n\). We say that some property holds almost everywhere if there exists a null set \(N\subseteq {\bar{M}}\) such that the property holds for all \(p\in {\bar{M}}\setminus N\).

We observe that the boundary is always mapped into a \((n-1)\)-dimensional hyperplane and hence a subset \(N\subseteq {\bar{M}}\) is a null set if and only if \(N\cap \text {int}({\bar{M}})\) is a null set. Thus, for the time being, we will restrict the further discussion to manifolds without boundary. Given a topological space \((X,\tau )\) we denote by \({\mathcal {B}}(X)\) the Borel-\(\sigma\)-algebra on X, i.e. the smallest \(\sigma\)-algebra on X which contains all open sets.

Definition 4.2

(Riemannian measure) Let (Mg) be an oriented, smooth Riemannian manifold without boundary of dimension n. Then we define the Riemannian measure \(\mu\) on (Mg) via

$$\begin{aligned} \mu :{\mathcal {B}}(M)\rightarrow [0,\infty ], A\mapsto \int _{M} \chi _A \omega _g, \end{aligned}$$
(4.1)

where \(\omega _g\) is the Riemannian volume form and \(\chi _A\) denotes the characteristic function of A. We call \(A\in {\mathcal {B}}(M)\) a \(\mu\)-null set if \(\mu (A)=0\).

One easily checks that any \(\mu\)-null set is also a null set in the sense of Definition 4.1.

The proof of Theorem 2.2 is divided in two steps. In the first step, we will show by means of Poincaré recurrence that the complement of the set \({\mathcal {F}}^{\prime }:=\{p\in {\bar{M}}| p\in \omega (p)\cap \alpha (p) \}\) is a null set. In a second step, we will show that the set of points at which the vector field vanishes is a null set (which are exactly the constant orbits).

Step 1: Claim: The set \({\bar{M}}\setminus \{p\in {\bar{M}}| p\in \omega (p)\cap \alpha (p) \}\) is a null set.

Proof of claim: Let \(M:=\textit{int}({\bar{M}})\) and as pointed out before we may restrict to the set of points contained in the interior since the boundary is a null set either way. Consider the Riemannian measure \(\mu\), which turns \(\left( M,{\mathcal {B}}(M),\mu \right)\) into a finite measure space, since \(\mu (M)=\int _M\chi _M\omega _g=\int _M\omega _g=\text {vol}(M)<+\infty\) by assumption. Further let \(\phi _t:M\rightarrow M\) denote the (global) flow of X, which is well-defined since diffeomorphisms map interiors to interiors. Since Beltrami fields are divergence-free by definition the induced flow is volume preserving, i.e. \((\phi _t)^{\#}\omega _g=\omega _g\) for every \(t\in {\mathbb {R}}\). We observe that for any given \(A\in {\mathcal {B}}(M)\) and any fixed \(t\in {\mathbb {R}}\), we have the identity \(\chi _{\phi ^{-1}_{t}(A)}=\chi _A\circ \phi _t=\phi _t^{\#}\chi _A\). Making use of the fact that \(\phi _t\) is volume-preserving and in particular orientation preserving we conclude

$$\begin{aligned} \mu ((\phi _t)^{-1}(A))= & {} \int _M\chi _{\phi ^{-1}_{t}(A)}\omega _g=\int _M(\phi _t^{\#}\chi _A)\phi ^{\#}\omega _g \\= & {} \int _M\phi _t^{\#}\left( \chi _A\omega _g\right) =\int _M\chi _A\omega _g=\mu (A), \end{aligned}$$

i.e. the \(\phi _t\) are measure preserving transformations. Because manifolds are metrisable [27, Theorem 2.55], and separable (since we assume them to be second countable) we obtain from [20, Theorem 4] that for \(\mu\)-almost all points \(p\in M\) the point p is recurrent. That is, \(\mu\)-almost every point \(p\in M\) satisfies the following property: For every neighbourhood U of p there exist sequences \((t^{\pm }_k)_k\) with \(t^{\pm }_k\rightarrow \pm \infty\) and \(\phi _{t^{\pm }_k}(p)\in U\) for all \(k\in {\mathbb {N}}\). Since these sequences diverge, we may pick suitable subsequences (denoted the same way) with \(|t^{\pm }_k|\ge k\). Now given \(j\in {\mathbb {N}}\) consider for any such fixed p the open metric ball \(B_{\frac{1}{j}}(p)\) and let \(\tau ^{\pm }_j\) be defined as the j-th element of the corresponding sequence \((t^{\pm }_k)_k\) as constructed before. Then obviously \(\phi _{\tau ^{\pm }_j}(p)\) converges to p and by construction \(\pm \tau ^{\pm }_j=|\tau ^{\pm }_j|\ge j\) and hence in particular \(p\in \omega (p)\cap \alpha (p)\). Hence, the set in question is a \(\mu\)-null set and every \(\mu\)-null set is in particular a null set in the sense of Definition 4.1. This proves the claim. \(\square\)

Step 2: Claim: The set \(\{p\in {\bar{M}}| \gamma _p\text { is constant} \}\) is a null set.

Proof of claim: The claim will follow immediately once we have shown Proposition 2.1.

Proof of Proposition 2.1: The basic ideas of the proof are similar to those used for instance in [22]. For the terminology used throughout, we refer to [18, Definition 3.2.14]. First we give the following definition

Definition 4.3

(Order of a zero) Let \(U\subseteq {\mathbb {R}}^n\) be open and \(f:U\rightarrow {\mathbb {R}}\) be a smooth function. Let \(x\in U\) be a zero of f, i.e. \(f(x)=0\), then the order of x is defined as \(\inf \{ m \in {\mathbb {N}}| \exists \alpha \in {\mathbb {N}}^n_0: |\alpha |=m\text { and }\partial ^{\alpha }f(x)\ne 0\}\), where we use the multi-index notation. If no such m exists we say x is a zero of infinite order. We write \(\varOmega _f(x)\) for the order of a given zero x of f. If M is any given smooth, n-dimensional manifold without boundary and \(\varvec{X}\in {\mathcal {V}}(M)\), then given a zero \(p\in M\) of \(\varvec{X}\), we define the order \(\varOmega (p)\) of p as follows: Pick any chart \(\mu\) of M around p and consider the functions \(X^j:=\varvec{X}(\mu ^j)\circ \mu ^{-1}\), the local expressions of \(\varvec{X}\). Then we set \(\varOmega (p):=\min _{1\le j\le n}\varOmega _{X^j}(\mu (p))\).

The notion of order of a given zero is independent of a particular choice of chart. Now consider \(\varvec{X}\) as given in Proposition 2.1 and restrict it to the interior \(M:=\text {int}({\bar{M}})\) of \({\bar{M}}\). We consider the set \(K_I:=\{p\in M|\varvec{X}(p)=0 \}\). Since \(\varvec{X}\) is a weak Beltrami field, and in particular because we assume the proportionality function \(\lambda\) to be locally bounded, it is a consequence of [4, Theorem 1] that all zeros have finite order. Otherwise the unique continuation result in [4] implies that \(\varvec{X}\) is the zero vector field, contradicting our assumptions. Given \(n\in {\mathbb {N}}\) we denote by \(K_n\subseteq K_I\) the set of zeros in the interior of order n. Then we have

$$\begin{aligned} K_I=\sqcup _{n\in {\mathbb {N}}}K_n, \end{aligned}$$
(4.2)

where \(\sqcup\) indicates that this union is disjoint. Now fix any such \(K_n\) and fix any point \(p\in K_n\). By definition, we may pick any chart \((\mu ,W)\) around p and consider the functions \(X^j\) as in Definition 4.3. Without loss of generality let \(\mu (p)=0\). Then there is one \(X^j\) with \(\varOmega _{X^j}(0)=n\) and in particular we can find a multi-index \(|\beta |=n-1\) such that \(\nabla (\partial ^{\beta }X^j)(0)\ne 0\), where \(\nabla\) denotes the standard Euclidean gradient. Define \(h:=\partial ^{\beta }X^j\) and observe that \(\mu (K_n\cap W)\subseteq h^{-1}(0)\) by the choices we made. However \(h:\mu (W)\rightarrow {\mathbb {R}}\) satisfies, after possibly shrinking W, \(\nabla h(x)\ne 0\) for all \(x\in \mu (W)\) and therefore \(h^{-1}(0)\) defines a two-dimensional submanifold of \(\mu (W)\). Hence \(K_n\cap W\subseteq \mu ^{-1}(h^{-1}(0))\), where the latter is a 2-dimensional submanifold of W, since \(\mu\) is a diffeomorphism between W and \(\mu (W)\). In particular it is also a smoothly embedded submanifold of M. Now given \(p\in K_n\) let \(W_p\) denote the corresponding neighbourhood and \(H_p\) denote the corresponding two-dimensional hypersurface containing \(K_n\cap W_p\) as constructed just now. Observe that \(K_n= \bigcup _{p\in K_n}K_n\cap W_p\) where \(\left( K_n\cap W_p\right) _{p\in K_n}\) forms an open cover of \(K_n\). We recall that we assume \({\bar{M}}\) to be second countable and thus so is \(K_n\) as a subset. But second countable spaces are Lindelöf and hence we can find a countable subcover \(\left( K_n\cap W_j\right) _{j\in {\mathbb {N}}}\) of \(K_n\). Then overall we have the inclusion

$$\begin{aligned} K_n= \bigcup _{j\in {\mathbb {N}}}K_n\cap W_j\subseteq \bigcup _{j\in {\mathbb {N}}}H_j. \end{aligned}$$
(4.3)

If we now fix some \(H_j\), we may cover it by proper slice charts of the form \(\mu : V\rightarrow B_r(0)\subseteq {\mathbb {R}}^3\) and \(\mu \left( V\cap H_j \right) =B_r(0)\cap \{x_3=0 \}\) for suitable \(V\subseteq M\subseteq {\bar{M}}\) open, where by proper we mean that each such chart \(\mu\) extends to a chart \({\tilde{\mu }}:{\tilde{V}}\rightarrow B_{2r}(0)\) on some larger neighbourhood. It follows then from [27, Proposition 2.51, Lemma 2.53] that the maps \(\mu ^{-1}:(B_r(0),d_2)\rightarrow ({\bar{M}},d_g)\) are Lipschitz continuous, where \(d_2\) is the standard Euclidean distance and \(d_g\) denotes the induced Riemannian distance. Since we have chosen \(\mu\) as slice charts, we can now let \(\pi :{\mathbb {R}}^3\rightarrow {\mathbb {R}}^2\) denote the projection onto the first two components and define \(f:\pi (B_r(0))\rightarrow V\cap H_j\), \((x,y)\mapsto \mu ^{-1}(x,y,0)\), which is Lipschitz as a composition of Lipschitz functions. Further f is defined on some bounded domain of \({\mathbb {R}}^2\) and we have \(f\left( \pi (\mu (K_n\cap V\cap H_j)) \right) =K_n\cap V\cap H_j\) so that the sets \(K_n\cap V\cap H_j\) are all 2-rectifiable. We observe that due to (4.3) we have \(K_n=\bigcup _{j\in {\mathbb {N}}}(K_n\cap H_j)\) and that the sets V are open sets. Thus we can now argue exactly as before, that there must exist a countable open subcover of \(K_n\cap H_j\) of sets of the form \(K_n\cap V\cap H_j\) each of which is 2-rectifiable. Hence \(K_n\) are countably 2-rectifiable and by (4.2) it follows that \(K_I\) is countably 2-rectifiable. Since \(K=\{p\in {\bar{M}}| \varvec{X}(p)=0 \}= (\partial {\bar{M}}\cap K)\cup K_I\) and since one can argue similarly as before, using boundary charts, that \(\partial {\bar{M}}\cap K\) is also countably 2-rectifiable, we conclude that K is countably 2-rectifiable and hence has Hausdorff dimension of at most 2. This proves the first part of Proposition 2.1, which in particular concludes the proof of Step 2 and therefore the proof of Theorem 2.2. Then Corollary 2.3 immediately follows from Theorem 2.2.

Proof of second part of Proposition 2.1: Assume now that the proportionality function \(\lambda\) is \(C^{\infty }\)-bounded near K. We can argue identically as before up to the point where we specify the function h. In particular (4.2) still holds and we fix some \(K_n\) and \(p\in K_n\) and choose the multi-index \(|\beta |=n-1\) with \(\nabla (\partial ^{\beta }X^j)(0)\ne 0\) accordingly. Without loss of generality, we may assume \(j=1\). We define the functions \(h^i:=(\partial ^{\beta }X^i)\) on \(\mu (W)\) for \(1\le i\le 3\) and \(\varvec{h}:=(h^1,h^2,h^3)\). Since we were allowed to choose the chart \(\mu\) as we wanted, we may in particular choose it to be a normal coordinate chart centred around p (recall p is an interior point), see [27, Proposition 5.24] for properties of normal coordinates. We claim that

$$\begin{aligned} D\varvec{h}(0)\text { has rank at least two}, \end{aligned}$$
(4.4)

where \(D\varvec{h}(0)\) is the Jacobian matrix of \(\varvec{h}\) at 0. By choice the rank of this matrix is at least one, so it is enough to exclude the possibility that the rank is exactly 1. We recall that \(\varvec{X}\) is a weak Beltrami field, which implies

$$\begin{aligned} \text {div}(\varvec{X})=0\text { and }\text {curl}(\varvec{X})=\lambda \varvec{X}. \end{aligned}$$
(4.5)

The first equation reads in local coordinates

$$\begin{aligned} 0=(\det {g})^{-\frac{1}{2}}\partial _i\left( X^i\sqrt{\det {g}} \right) . \end{aligned}$$

Applying \(\partial ^{\beta }\) for the \(\beta\) chosen above to both sides of the above equation and using the Leibniz rule, we obtain

$$\begin{aligned} 0=\sum _{\alpha \le \beta }\left( {\begin{array}{c}\beta \\ \alpha \end{array}}\right) \partial ^{\beta -\alpha }\left( (\det {g})^{-\frac{1}{2}}\right) \partial ^{\alpha }\left( \partial _i\left( X^i\sqrt{\det {g}}\right) \right) . \end{aligned}$$

Now observe that for \(|\alpha |<|\beta |\) the order of the derivatives acting upon \(X^i\) in the term \(\partial ^{\alpha }\left( \partial _i\left( X^i\sqrt{\det {g}}\right) \right)\) is of order at most \(|\beta |=n-1\). Since the order of \(\varvec{X}\) at p is n, this means by definition that all these terms vanish if we evaluate them at \(\mu (p)=0\). So only the term for \(\alpha =\beta\) is non-zero and we obtain

$$\begin{aligned} 0=(\det {g})^{-\frac{1}{2}}\partial ^{\beta }\left( \partial _i\left( X^i\sqrt{\det {g}} \right) \right) =(\partial _ih^i)(0), \end{aligned}$$

where we used in the last step that the additional terms from the product rule vanishes because once more the derivatives in this term acting upon \(X^i\) are of order at most \(|\beta |\). We find

$$\begin{aligned} 0=(\partial _ih^i)(0)\Leftrightarrow \text {div}(\varvec{h})(0)=0, \end{aligned}$$
(4.6)

where the divergence is computed with respect to the Euclidean metric. The second equation from (4.5) reads in local coordinates as

$$\begin{aligned} \lambda X^k=\epsilon ^{ijk}\frac{\partial _i\left( X^lg_{lj}\right) }{\sqrt{\det {g}}}\text { for all }1\le k\le 3. \end{aligned}$$

For notational simplicity, we let \(Y^k:=\epsilon ^{ijk}\frac{\partial _i\left( X^lg_{lj}\right) }{\sqrt{\det {g}}}\). By what we have shown in the first part of the proof, the set K has a Hausdorff dimension of at most 2 and therefore does not contain any interior points. Thus, there exists a sequence \((x_m)_m\subset \mu (W\setminus K)\) converging to \(\mu (p)=0\). Observe that \(\lambda \circ \mu ^{-1}\) is smooth on \(\mu (W\setminus K)\) so that we may apply the Leibniz rule to get

$$\begin{aligned} (\partial ^{\beta }Y^k)(x_m)=\sum _{\alpha \le \beta }\left( {\begin{array}{c}\beta \\ \alpha \end{array}}\right) \left( \partial ^{\beta -\alpha }(\lambda \circ \mu ^{-1})(x_m)\right) (\partial ^{\alpha }X^k)(x_m). \end{aligned}$$

Then the triangle inequality and \(x_m\in \mu (W\setminus K)\) imply

$$\begin{aligned} |(\partial ^{\beta }Y^k)(x_m)|\le \sum _{\alpha \le \beta }\left( {\begin{array}{c}\beta \\ \alpha \end{array}}\right) \left\| \partial ^{\beta -\alpha }(\lambda \circ \mu ^{-1})\right\| _{L^{\infty }(\mu (W\setminus K))}|(\partial ^{\alpha }X^k)(x_m)|. \end{aligned}$$

Since we assume \(\lambda\) to be \(C^{\infty }\)-bounded near K, after possibly shrinking W if necessary, we see that there is some constant \(C>0\), independent of m, with

$$\begin{aligned} |(\partial ^{\beta }Y^k)(x_m)|\le C\sum _{\alpha \le \beta }|(\partial ^{\alpha }X^k)(x_m)|. \end{aligned}$$

Taking the limit on both sides and observing that \(Y^k\) as well as \(X^k\) are smooth, we find

$$\begin{aligned} |(\partial ^{\beta }Y^k)(0)|\le C\sum _{\alpha \le \beta }|(\partial ^{\alpha }X^k)(0)|=0, \end{aligned}$$

where we used the definition of \(K_n\) and \(\beta\) in the last step and that \(\alpha \le \beta\) implies \(|\alpha |\le |\beta |\). Thus \((\partial ^{\beta }Y^k)(0)=0\) for \(1\le k\le 3\). Applying the Leibniz rule to the definition of \(Y^k\) we can argue similarly as before, namely that all terms vanish except for the term of highest derivative acting on the \(X^l\). Since we are in normal coordinates we immediately get

$$\begin{aligned} 0=\epsilon ^{ijk}\delta _{lj}(\partial _i\partial ^{\beta }X^l)(0)\text { for all }1\le k\le 3. \end{aligned}$$

Writing this out explicitly and using the definition of the \(h^i\) we obtain:

$$\begin{aligned} (\partial _jh^i)(0)=(\partial _ih^j)(0)\text { for all }1\le i,j\le 3. \end{aligned}$$
(4.7)

Now assume for a contradiction, namely that \((D\varvec{h})(0)\) in (4.4) has rank 1. Without loss of generality we may therefore assume that \(\nabla h^1(0)\ne 0\) and since the rank is 1, both other rows must be linearly dependent, i.e. there exist constants \(a_1,a_2\in {\mathbb {R}}\) such that \((\nabla h^2)(0)=a_2(\nabla h^1)(0)\) and \((\nabla h^3)(0)=a_3(\nabla h^1)(0)\). For notational simplicity, we will drop the argument from now on. Then these relations together with (4.6) and (4.7) imply

$$\begin{aligned} \partial _2h^1= & {} \partial _1h^2=a_2\partial _1h^1\text {, }\partial _3h^1=\partial _1h^3=a_3\partial _1h^1, \\ \partial _1h^1= & {} -\partial _2h^2-\partial _3h^3=-a_2\partial _2h^1-a_3\partial _3h^1. \end{aligned}$$

Now multiply the latter equation by \(a_3\) and use the first two relations to conclude

$$\begin{aligned}&\partial _3h^1=a_3\partial _1h^1=-a_3a_2\partial _2h^1-a^2_3\partial _3h^1=-a^2_2(a_3\partial _1h^1)-a^2_3\partial _3h^1=(-a^2_2-a^2_3)\partial _3h^1 \\&\Leftrightarrow 0=(1+a^2_2+a^2_3)\partial _3h^1\Leftrightarrow \partial _3h^1=0. \end{aligned}$$

From this, we obtain

$$\begin{aligned} \partial _1h^1=-a_2\partial _2h^1-a_3\partial _3h^1=-a_2\partial _2h^1=-a^2_2\partial _1h^1\Leftrightarrow 0=(1+a^2_2)\partial _1h^1\Leftrightarrow \partial _1h^1=0. \end{aligned}$$

Finally the latter implies \(\partial _2h^1=a_2\partial _1h^1=0\) and so overall we find \((\nabla h^1)(0)=0\), a contradiction. Thus indeed the rank of \((D\varvec{h})(0)\) is at least two. Without loss of generality let \((\nabla h^2)(0)\) and \((\nabla h^1)(0)\) be linearly independent. Then by the implicit function theorem, we conclude that the set \(L:=\{h^1=0\}\cap \{h^2=0\}\), after possibly shrinking the domain W, is a one-dimensional submanifold of \(\mu (W)\) and we observe that \(\mu \left( K_n \cap W \right) \subseteq L\). From here on, we can argue exactly as previously that each \(K_n\) is contained in a countable union of 1-dimensional (smoothly embedded) submanifolds and therefore is countably 1-rectifiable. The relation (4.2) concludes the proof. \(\square\)

Proof of Corollary 2.4

The corollary follows immediately from Proposition 2.2. For a concise introduction to Hausdorff measures and dimensions on metric spaces see for instance [29, Chapter 6].

Proof of Proposition 2.2: The basic idea of the first step of the proof for the Euclidean case is taken from a math.stackexchange discussion.

Step 1: Claim: For every \(p\in M\), there exists an open neighbourhood U of p such that any two points \(q,{\tilde{q}}\in U \setminus A\) can be joined by a continuous path in \(U\setminus A\).

Proof of claim: Fix any \(p\in M\), then there exists some \(\epsilon (p)>0\) such that every open geodesic ball centred around p whose radius is smaller than \(\epsilon (p)\) is geodesically convex [27, Theorem 6.17]. Thus, let U be an open geodesic ball of radius smaller than \(\epsilon (p)\) and such that its closure is a closed geodesic ball, in particular its closure is contained in a coordinate chart. Then by definition of an open geodesic ball we can find a chart \(\mu :U\rightarrow B_r(0)\) for suitable \(r>0\) and \(\mu (p)=0\). Observe that \(\mu :U\rightarrow B_r(0)\) is Lipschitz if we equip U with the induced Riemannian distance function and \(\mu (U)\) with the standard Euclidean distance [27, Proposition 2.51,Lemma 2.53] and observe further that the induced Riemannian distance function on U coincides with the restriction of the Riemannian distance function of M to \(U\times U\) since U is geodesically convex. Now let \(q,{\tilde{q}}\in U\setminus A\) be any two fixed points. If \({\tilde{q}}=q\) we may join them by the constant path, which lies entirely within \(U\setminus A\). So now suppose \({\tilde{q}}\ne q\). Define \({\tilde{y}}:=\mu ({\tilde{q}})\), \(y:=\mu (q)\) and \(v:=y-{\tilde{y}}\). Since \({\tilde{q}}\ne q\) we have \(v\ne 0\) and hence it spans a one-dimensional subspace L of \({\mathbb {R}}^n\). Let H denote the Euclidean orthogonal complement of L in \({\mathbb {R}}^n\) and let \(\pi :{\mathbb {R}}^n\rightarrow H\) denote the orthogonal projection onto H. Since \(U\cap A\subseteq A\), its Hausdorff dimension is at most as large as that of A and since \(U\cap A\subseteq U\) the Hausdorff dimension of \(U\cap A\) computed with respect to the restriction of the Riemannian distance function of M to \(U\times U\) coincides with the Hausdorff dimension of \(U\cap A\) with respect to the Riemannian distance on M. In addition \(\mu\) is a Lipschitz map with respect to the Euclidean metric and the restriction of the Riemannian distance of M to \(U\times U\). Therefore, the image \(\mu (U\cap A)\subseteq {\mathbb {R}}^n\) has a Hausdorff dimension (with respect to the Euclidean distance) strictly less than \((n-1)\). Observe that \(\pi\) is a linear map between finite dimensional vector spaces and hence Lipschitz continuous. Thus, \(\pi \left( \mu (U\cap A)\right) \subseteq H\) has a Hausdorff dimension strictly less than \((n-1)\). But H is \((n-1)\)-dimensional which implies that \(\pi \left( \mu (U\cap A)\right)\) does not have any interior points and so in particular \(H\setminus \pi \left( \mu (U\cap A)\right)\) is dense in H. Further A is closed in M, thus \(U\cap A\) is closed in U and since \(\mu\) is a homeomorphism \(\mu (U\cap A)\) is closed in \(B_r(0)\). Since \(q,{\tilde{q}}\in U\setminus A\) we see that \(y,{\tilde{y}}\in B_r(0)\setminus \mu (U\cap A)\), which is open as the complement of a closed subset. Therefore, there exist open balls \(B_y\) and \(B_{{\tilde{y}}}\) around y and \({\tilde{y}}\), respectively, which are contained in \(B_r(0)\setminus \mu (U\cap A)\). Observe that \(\pi (v)=0\) and thus \(\pi (B_{{\tilde{y}}})\cap \pi (B_y)\ne \emptyset\) since \(0=\pi (v)=\pi (y)-\pi ({\tilde{y}})\) by linearity of \(\pi\) and definition of v. Since \(\pi\) is surjective and H, \({\mathbb {R}}^n\) finite dimensional, \(\pi\) is an open map. We conclude that \(\pi \left( B_{{\tilde{y}}}\right) \cap \pi (B_y)\) is a non-empty open subset of H and since \(H\setminus \pi \left( \mu (U\cap A)\right)\) is dense in H the intersection of \(\left( H\setminus \pi \left( \mu (U\cap A)\right) \right)\) and \(\pi \left( B_{{\tilde{y}}}\right) \cap \pi (B_y)\) is non-empty. Let z be any fixed element of this intersection and let \(L_z:=\pi ^{-1}(\{z\})=\{z+\lambda v|\lambda \in {\mathbb {R}}\}\). By definition of z we have \(L_z\cap \mu (U\cap A)=\emptyset\) and there exist \(x_0\in B_{{\tilde{y}}}\), \(y_0\in B_y\) with \(\pi (x_0)=z=\pi (y_0)\), i.e. \(x_0,y_0\in L_z\) or equivalently there are \(\lambda _x,\lambda _y\in {\mathbb {R}}\) with \(x_0=z+\lambda _xv\) and \(y_0=z+\lambda _yv\). Assume without loss of generality that \(\lambda _x\le \lambda _y\), then the pass \(l(t):=z+tv\) with \(\lambda _x\le t\le \lambda _y\) connects \(x_0\) and \(y_0\) and is contained in \(L_z\) which does not intersect \(\mu (U\cap A)\). In addition \(x_0\in B_{{\tilde{y}}}\subseteq B_r(0)\) and similarly \(y_0\in B_r(0)\). By convexity of \(B_r(0)\) and since l(t) defines a straight line connecting two points within \(B_r(0)\) the whole path \(l([\lambda _x,\lambda _y])\) is contained in \(B_r(0)\). Finally recall that \(y_0\in B_y\) and \(B_y\) was an open ball around y contained in \(B_r(0)\setminus \mu (U\cap A)\). Hence, we may connect \(y_0\) and y by a straight line and similarly connect \(x_0\) and \({\tilde{y}}\) by a straight line and obtain a continuous path from y to \({\tilde{y}}\) contained in \(B_r(0)\setminus \mu (U\cap A)\). Lifting this path via \(\mu ^{-1}\) gives us a path contained in \(U\setminus A\) connecting q and \({\tilde{q}}\). This proves the claim.

Step 2: Claim: Any two points \(p,q\in M\setminus A\) can be joined by a continuous path contained in \(M\setminus A\).

Proof of claim: By assumption M is connected and connected manifolds are in particular path connected. Thus, let \(\gamma :[0,1]\rightarrow M\) be a path connecting p and q. For any given \(x\in \gamma ([0,1])\) let \(U_x\) be a neighbourhood as in the first step, i.e. any two points within \(U_x\setminus A\) can be joined by a path within \(U_x\setminus A\). By compactness and connectedness of \(\gamma ([0,1])\) we can cover \(\gamma ([0,1])\) by finitely many such neighbourhoods \(U_i\), \(1\le i\le N\) such that \(p\in U_1\), \(q\in U_N\) and \(U_i\cap U_{i+1}\ne \emptyset\) for all \(i=1,\dots , N-1\), see also the proof of [26, Proposition 1.16]. Since A has a Hausdorff dimension of less than \((n-1)\) and in particular less than n, it does not contain any interior points, hence \(M\setminus A\) is dense in M. But the \(U_i\cap U_{i+1}\) are non-empty open subsets of M and thus there exist elements \(p_i\in U_i\cap U_{i+1}\cap (M\setminus A)\), \(1\le i\le N-1\). By choice of the \(U_i\), we can now connect p and \(p_1\) by a continuous path within \(U_1\setminus A\subseteq M\setminus A\). Then connect \(p_i\) with \(p_{i+1}\) by a path within \(U_{i+1}\setminus A\subseteq M\setminus A\) and finally join \(p_{N-1}\) with q within \(U_N\setminus A\subseteq M\setminus A\). Overall, we obtain a continuous path \({\tilde{\gamma }}:[0,1]\rightarrow M\setminus A\) joining p and q. \(\square\)

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Acknowledgements

I would like to thank Christof Melcher and Heiko von der Mosel for discussions. Further I want to thank Daniel Peralta-Salas for pointing out the results of Christian Bär to me. Lastly I also want to thank the anonymous referee for carefully reading my manuscript.

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Open Access funding enabled and organized by Projekt DEAL. The author was funded by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation)—Projektnummer 320021702/GRK2326—Energy, Entropy, and Dissipative Dynamics (EDDy).

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Gerner, W. Typical field lines of Beltrami flows and boundary field line behaviour of Beltrami flows on simply connected, compact, smooth manifolds with boundary. Ann Glob Anal Geom 60, 65–82 (2021). https://doi.org/10.1007/s10455-021-09768-3

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Keywords

  • Beltrami fields
  • Field line dynamics
  • Dynamical systems
  • (Magneto-)Hydrodynamics
  • Nodal sets
  • Nodal domains

Mathematics Subject Classification

  • 35Q31
  • 35Q35
  • 35Q85
  • 37C10
  • 37E35
  • 37B20
  • 53Z05
  • 58K45
  • 60B05
  • 76W05