Abstract
We study a variational Ginzburg–Landau type model depending on a small parameter \(\varepsilon >0\) for (tangent) vector fields on a 2-dimensional Riemannian manifold S. As \(\varepsilon \rightarrow 0\), these vector fields tend to have unit length so they generate singular points, called vortices, of a (non-zero) index if the genus \({\mathfrak {g}}\) of S is different than 1. Our first main result concerns the characterization of canonical harmonic unit vector fields with prescribed singular points and indices. The novelty of this classification involves flux integrals constrained to a particular vorticity-dependent lattice in the \(2{\mathfrak {g}}\)-dimensional space of harmonic 1-forms on S if \({\mathfrak {g}}\geqq 1\). Our second main result determines the interaction energy (called renormalized energy) between vortex points as a \(\Gamma \)-limit (at the second order) as \(\varepsilon \rightarrow 0\). The renormalized energy governing the optimal location of vortices depends on the Gauss curvature of S as well as on the quantized flux. The coupling between flux quantization constraints and vorticity, and its impact on the renormalized energy, are new phenomena in the theory of Ginzburg–Landau type models. We also extend this study to two other (extrinsic) models for embedded hypersurfaces \(S\subset {{\mathbb {R}}}^3\), in particular, to a physical model for non-tangent maps to S coming from micromagnetics.
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Notes
In the sequel, a vector field on S is always tangent at S (the standard definition in differential geometry).
In the case of a surface (S, g) with genus 1 (i.e., homeomorphic with the flat torus), then \(n=0\) and \(u^*\) is smooth in S.
In fact, \(\deg (u^*; \gamma )=d_k\) for every closed simple curve \(\gamma \) around \(a_k\) and lying near \(a_k\).
We use the term “canonical harmonic unit vector field" to emphasize the parallel to the canonical harmonic map introduced in [3], but for genus \({\mathfrak {g}}>0\), specifying a canonical harmonic unit vector field requires not only the points \(a_k\) and degrees \(d_k\) but also some flux integrals, see (12) below. Thus, such a vector field can only claim to be canonical once this data is given. In addition, uniqueness holds only up to a global rotation (see Theorem 2.1).
In fact, by changing the choice of curves and the basis in \(Harm^1(S)\), the matrix \(\alpha \) is multiplied by an invertible matrix (similar to the standard change of coordinates in vector spaces) due to the above definition of homologous curves where \(\int _{\gamma }\eta = \sum _{\ell =1}^{2{\mathfrak {g}}} c_\ell \int _{\gamma _\ell }\eta \) for every harmonic 1-form \(\eta \), see also Lemma 5.2.
See Section 5.3 for the definition of \(W^{-1,1}\).
By this we mean that \(\zeta _\ell (a;d) = \{ 2\pi n+\int _{\lambda _\ell } (d^*\psi + A) : n\in {{\mathbb {Z}}}\}\). We will consistently abuse notation in a similar way.
More precisely, according to [2], page 109, eqn (17), one may define \(G_0\) as above such that \(H := G - G_0\) can be represented in the form
$$\begin{aligned} H(x,y) = \int _S \Delta _z G_0(x,z) G_0(z,y) \,\hbox {vol}_g(z) + \hbox {smoother terms}, \end{aligned}$$(where here \(\Delta _z\) denotes the pointwise Laplacian rather than the distributional Laplacian) and in addition \(\Vert \Delta _z G_0 \Vert _{L^\infty (S)}\leqq C\).
The function \(x\mapsto H(x,x)\) is called the Robin’s mass on \({\mathbb {S}}^2\), see e.g. [40].
A thin film regime is characterized by a small aspect ratio h; the ferromagnetic samples considered here are very small because \(\ell \) has the order of nanometers as \(\eta \).
A different regime is studied in [23].
However, \(A = -j(u^*)\not \in L^2\) whenever \(u^*\) has singular points (in particular, whenever \({\mathfrak {g}}\ne 1\)), and then the space of finite-energy \(\phi \) contains functions not in \(H^1\), making it inconvenient to work with the representation (33).
For a non-variational approach to existence results in this setting, see for example [11].
That is, non self-intersecting.
Modifying f on a null set, if necessary, we assume that wherever this limit exists.
Recall that \(\Delta (\psi _1 \,\hbox {vol}_g)= (\Delta \psi _1) \,\hbox {vol}_g\).
The symmetry of H follows from \(H_{\ell k}=-\tau _k \cdot \bar{D}_\ell N=N\cdot (\bar{D}_\ell \tau _\beta -D_\ell \tau _\beta )\) as \(\tau _k\cdot N=0\) and \(\bar{D}_\ell \tau _\beta -D_\ell \tau _\beta =\bar{D}_\beta \tau _\ell -D_\beta \tau _\ell +\underbrace{[{\bar{\tau }}_\ell , {\bar{\tau }}_\beta ]-[\tau _\ell , \tau _\beta ]}_{=0}\) where \([\cdot , \cdot ]\) represents the commutator in \({{\mathbb {R}}}^3\) for the metric g.
Recall from Theorem 2.1 that \(u^*(a,d,\Phi )\) is unique only up to a rotation. For purposes of this definition, we assume that a representative \(u^*\) has been (arbitrarily) fixed. In the end we are only interested in \(\inf {\mathcal {I}}_\varepsilon \), and this is independent of the chosen rotation. We will therefore feel free to adjust the rotations as needed.
The footnote 21 applies here as well.
This argument proves the following continuity result (in addition to Theorem 2.1): if \(a_\varepsilon \rightarrow a\) and \(\Phi _\varepsilon \in {{\mathcal {L}}}(a_\varepsilon , d)\rightarrow \Phi \in {{\mathcal {L}}}(a,d)\), then up to rotations, \(u_\varepsilon ^*(a_\varepsilon , d, \Phi _\varepsilon ) \rightarrow u^*(a, d, \Phi )\) almost everywhere and in \(L^p\) for all \(p<\infty \).
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Acknowledgements
R.I. acknowledges partial support by the ANR project ANR-14-CE25-0009-01. The work of R.J. was partially supported by the Natural Sciences and Engineering Research Council of Canada under operating Grant 261955.
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Appendix A. Ball Construction. Proof of Proposition 8.2
Appendix A. Ball Construction. Proof of Proposition 8.2
In this section we present the vortex ball construction leading to Proposition 8.2. We start with several lemmas in which we verify, largely by adapting classical proofs to our setting, that basic ingredients needed for the vortex ball argument on the Euclidean plane remain available in the present setting. Once these ingredients are available, we follow classical arguments. Since the arguments are rather standard, our exposition is terse in places.
We first fix positive constants \(c_1(S), r_0(S)\) such that \(\partial B_r(x)\) is a homeomorphic to a circle for every \(x\in S\), and \(0<r<r_0\) (thus, \(r_0\) is at most the injectivity radius of S) and we recall (121). In several places later in our argument, we will impose additional smallness conditions on \(r_0\).
In view of Lemma 5.1, in proving lower energy bounds we may restrict our attention to smooth vector fields.
Lemma A.1
Given \(u\in {{\mathcal {X}}}(S)\), let \(\rho := |u|_g\). Assume that \(\varepsilon<r<r_0(S)\). Then there exist positive constants \(c_2,c_3, c_4\) such that the following hold. First,
where \(|{d}\rho |_g^2(x) := ({d}\rho (\tau _1))^2 + ({d}\rho (\tau _2))^2\) for any orthonormal basis \(\{ \tau _1,\tau _2 \}\) of \(T_xS\). Second,
where
is a nonincreasing function, and we use the convention that for \(r>0\), \(\lambda _\varepsilon (r/0) = \lambda _\varepsilon (+\infty ) = 0 \).
Proof
At \(y\in \partial B_r(x)\), let \(\tau \in T_yS\) denote the unit tangent to \(\partial B_r(x)\), oriented in the standard way, and let \({}'\) denote differentiation with respect to \(\tau \). Further define \(\zeta := (1 - \rho )^2\). Then by (1)
Then (123) follows from a (suitably scaled) Sobolev embedding \(W^{1,1}\hookrightarrow L^\infty \) on \(\partial B_r(x)\), taking into account the fact that \({{\mathcal {H}}}^1(\partial B_r(x)) \geqq \varepsilon \).
Next, if \(\rho \geqq \frac{1}{2}\) on \(\partial B_r(x)\), then we can define \(v = u/\rho \) and \(d:= \deg (u; \partial B_r(x))\) . Since \(|v|_g=1\), we have \(|Dv|_g = |j(v)|_g\), and thus
Since S is compact and smooth, it follows from this and (121) that
Finally, if we write \(s :=\min _{\partial B_r(x)} (\rho \wedge 1) >0\), then \(|Du|_g^2 = |{d}\rho |{_g}^2 + \rho ^2|Dv|{_g}^2 \geqq |{d}\rho |_g^2 + s^2 |Dv|_g^2\). Then one may deduce (124) from (123) and (126), after first taking \(r_0\) small enough so that \(c_3r_0^2 \leqq 1/2\), which yields \(|d|(1-c_3r^2)\geqq 1-c_3\frac{r^2}{d^2}\) for every \(|d|\geqq 1\). Then (124) follows directly in the case \(\rho \geqq \frac{1}{2}\) on \(\partial B_r(x)\), if \(d\ne 0\), whereas if \(d=0\) it is immediate. If \(\min _{\partial B_r(x)}\rho < \frac{1}{2}\), then \( \Vert 1-\rho \Vert _{L^\infty } > \frac{1}{2}\), and thus
for any d. (If \(\rho =0\) somewhere on \(\partial B_r(x)\), then the definition \(v = u/\rho \) may not make sense, but the proof of (124) relies only on (123) and makes no mention of v.) \(\square \)
We also need:
Lemma A.2
Assume that u is a smooth vector field on S and that for some \(0<r<r_0(S)\) and \(x\in S\),
Then if \(r_0\) is sufficiently small,
Proof
First, let \(O := \{y\in B_r(x) : \rho (y)<t \}\), where t is a regular value of \(\rho (\cdot )\) such that \(\frac{1}{8}<t<\frac{1}{4}\). Then O is an open set with smooth boundary, compactly contained in \(B_r(x)\), and
where the final equality follows from Lemma 5.4 and Stokes’ Theorem, as well as the fact that \(|u|_g=t\) on \(\partial O\). Thus if \(r_0\) is sufficiently small (depending on \(\Vert \kappa \Vert _\infty \)) then
where the last inequality follows from Lemma 5.3, see (40). \(\square \)
Finally we recall
Lemma A.3
Assume that \(u_\varepsilon \) is a smooth vector field satisfying (51). Then there exists \(\varepsilon _0>0\) such that whenever \(0<\varepsilon <\varepsilon _0\), there exists a collection \(\tilde{{\mathcal {B}}}^0 = \{ {\tilde{B}}^0_j \}\) of closed pairwise disjoint balls that cover the set where \(|u_\varepsilon |_g\leqq \frac{1}{2}\), and such that
Proof
Let \(\rho := |u_\varepsilon |_g\). Then \(\frac{1}{2} |{d}\rho |_g^2 + \frac{1}{4\varepsilon ^2}F(\rho ^2) \geqq \frac{1}{\varepsilon \sqrt{2}} |{d}\rho |_g \sqrt{F(\rho ^2)} \geqq \frac{c}{\varepsilon }|1-\rho | \, |{d}\rho |_g\), by (1). Thus the coarea formula, which remains valid on a smooth manifold, implies that
In particular we may find some \(\alpha \in [\frac{1}{2}, \frac{3}{4}]\), a regular value of \(\rho \), such that \({{\mathcal {H}}}^1(\rho ^{-1}(\alpha )) \leqq C \varepsilon \int _S e_\varepsilon ^{in}(\rho ) \,\hbox {vol}_g\). Following standard arguments, we may start with an efficient finite cover of \(\rho ^{-1}(\alpha )\) and then merge balls to find a collection of closed pairwise disjoint balls that cover \(\rho ^{-1}(\alpha )\) and whose radii sum to at most \(2{{\mathcal {H}}}^1(\rho ^{-1}(\alpha ))\). This is \(\tilde{{\mathcal {B}}}^0\). The complement of the union of these balls is connected as long as \(\varepsilon \) is small enough, so on the complement, either \(\rho > \alpha \) or \(\rho <\alpha \) everywhere. The latter case is impossible by (51) and (123), if \(\varepsilon \) is small enough, and this proves the lemma. \(\square \)
A few more definitions are needed before we prove Proposition 8.2. W.l.o.g., we may assume that \(\frac{1}{2}\) is a regular value of \(\rho =|u|_g\). First, we set
Next, for any set \(V\subset S\) such that \(\partial V \cap Z_E = \emptyset \) we define the generalized degree
Note that \(\hbox {dg}(u;\partial V) = \deg (u,\partial V)\) if \(\partial V\) is \(C^1\), say, and \(|u|_g > \frac{1}{2}\) on \(\partial V\). Finally we define
It is straightforward to check that
We record several other properties. First, since \(\Lambda _\varepsilon (\cdot )\) is the integral over \([0,\sigma ]\) of a positive nonincreasing function, it is easy to see that
Finally, consider two radii \(r_1<r_2\) such that \(\varepsilon \leqq r_j \leqq r_0\) for \(j=1,2\), and assume that \(x\in S\) is a point such that \(Z_E\) does not intersect the annulus \(B_{r_2}{\setminus } B_{r_1}(x)\). Then \(\hbox {dg}(u;\partial B_r(x)) = \hbox {dg}(u; \partial B_{r_1}(x))\) for all \(r\in (r_1,r_2)\), so one may use the coarea formula and integrate (124) from \(r_1\) to \(r_2\) to find that
Proof of Proposition 8.2
We divide the proof in several steps:
Step 1. An initial covering of \(Z_E\). We claim first that there exists a collection \({\mathcal {B}}^0 = \{ B_{l,0}\}_{k=1}^K\) of closed, pairwise disjoint balls with centers \(a_{l,0}\) and radii \(r_{l,0}\geqq \varepsilon \) for all l, such that \(Z_E\subset \cup B^0_k\), and (after possibly decreasing the constant \(c_2\) in the definition (125) of \(\lambda _\varepsilon \), in a way that depends only on the geometry of S)
We first cover \(Z_E\) with balls that satisfy (129). Indeed, for every \(x\in Z_E\), this estimate holds for \(B_r(x)\), for the smallest \(r\geqq \varepsilon \) such that \(\min _{\partial B_r(x)}\rho \geqq 1/2\). This is a result of Lemma A.2, if its \(r\leqq 2\varepsilon \), and otherwise it follows from (123) and the coarea formula. One can then choose a finite subcover. The balls obtained in this fashion may overlap. If so, they may be combined into pairwise disjoint balls that still satisfy (129), by exactly the arguments in [24], proof of Proposition 3.3, where the same result is proved in the Euclidean setting. This argument involves a slightly more careful choice of balls (so that no center is contained in any other ball) and use of the Besicovitch covering lemma. For our present purposes, we may appeal to Federer [16, Sections 2.8.9–2.8.14], for a difficult but doubtless correct version of the covering lemma that is valid on a smooth compact Riemannian manifold, and indeed in much greater generality. Adjustments to the constant \(c_2\) depend on constants appearing in this covering lemma, which are explicitly described in the above reference.
Step 2. Growing and merging balls. Now let \(d_{l,0} := \hbox {dg}(u;\partial B_{l,0})\). We will assume for this discussion that \(d_{l,0}\ne 0\) for some l, as the other case is both easier and less relevant for our main results. Using Lemma A.1 and associated properties of \(\Lambda _\varepsilon \), such as those in (129), we may now follow the algorithm from [24], proof of Proposition 4.1, to which one may refer for the details omitted here. We describe it briefly. First, define
We claim that for \(\sigma \in (\sigma _0, r_0(S))\), there exists a finite collection of pairwise disjoint closed balls \({\mathcal {B}}^\sigma = \{ B_{l,\sigma }\}_{l=1}^{K_\sigma }\) with centers \(a_{l,\sigma }\) and radii \(r_{l,\sigma }\), such that
where \(d_{l,\sigma } = \hbox {dg}(u;B_{l,\sigma })\). We take \({\mathcal {B}}^{\sigma _0}\) to be the collection found in Step 1 above. Given any \(\sigma _1 \geqq \sigma _0\) for which such a collection exists, we say that the minimizing balls are those for which \(r_{l,\sigma _1} = \sigma _1 |d_{l,\sigma _1}|\). Since the balls are closed and pairwise disjoint, there is some \(\delta >0\) such that for \(\sigma _1 \leqq \sigma \leqq \sigma +\delta \), we can expand the minimizing balls, while leaving the centers fixed, by enclosing them in pairwise disjoint annuli chosen so that, for every \(\sigma \), the equality \(r_{l,\sigma } = {\sigma } |d_{l,\sigma }|\) holds for all minimizing balls. We add balls to the collection of minimizing balls as \(\sigma \) increases, when necessary. This preserves (130) due to properties of \(\Lambda _\varepsilon \) summarized above, such as (128). At certain values of \(\sigma \), for example \(\sigma = \sigma _1+\delta \), the expansion process will lead to two or more balls colliding. When this occurs, one can regroup them into larger, pairwise disjoint balls in a way that preserves the properties (130). (Details of all these assertions can be found in [24].) This process can be continued as long as every minimizing ball has radius at most \(r_0(S)\), which happens as long as \(\sigma < r_0(S)\).
Step 3. Stopping the process, and covering all of Z. Recalling that \(n>T-1\) by hypothesis, we fix \(q \in (0, 1-\frac{T}{n+1})\), which implies that \(\frac{T}{1-q}< n+1\). It then follows from (130), (127), and (51) that if \(\varepsilon ^q\leqq \sigma < r_0(S)\), then
Thus there exists \(\varepsilon _0>0\) (depending on S, q, and the constant in (51)) such that if \(0<\varepsilon <\varepsilon _0\), then \(\sum |d_{l,\sigma }| < n+1\), and thus \(\sum |d_{l,\sigma }|\leqq n\).
These balls have all the desired properties (the bound (57) on the sum of the radii follows from (131)) except that they cover \(Z_E\) rather than all of Z. To rectify this, recall from Lemma A.3 that \(Z{\setminus } Z_E\) can be covered by a finite collection of balls whose radii sum to at most \(C \varepsilon {|\!\log \varepsilon |}\). We can add these balls to \({\mathcal {B}}^\sigma \), merging as necessary to obtain a pairwise disjoint collection (still denoted \({\mathcal {B}}^\sigma \)) that covers all of Z, and with the sum of the radii increased by at most \(C\varepsilon {|\!\log \varepsilon |}\). Since \(\frac{T}{1-q}<n+1\), it follows from (131) that these still satisfy \(\sum r_{l,\sigma } < \sigma (n+1)\) for \(0<\varepsilon <\varepsilon _0\). The bound on the total degrees (56) and the energy lower bound (58) for this modified collection of balls are directly inherited from the previous collection. \(\square \)
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Ignat, R., Jerrard, R.L. Renormalized Energy Between Vortices in Some Ginzburg–Landau Models on 2-Dimensional Riemannian Manifolds. Arch Rational Mech Anal 239, 1577–1666 (2021). https://doi.org/10.1007/s00205-020-01598-0
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DOI: https://doi.org/10.1007/s00205-020-01598-0