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Skyrmions and Magnetic Textures

A magnetic texture is a spatially varying magnetic order parameter. Domains, domain walls, vortices, spirals, bubbles, merons, skyrmions, and three-dimensional singular structures are different ways for that order parameter to vary in space. Their form is set jointly by topology, exchange, anisotropy, dipolar fields, Dzyaloshinskii–Moriya coupling, applied fields, boundaries, disorder, and temperature.

Topology answers whether one smooth texture can be continuously deformed into another while respecting a declared order-parameter space and boundary condition. It does not by itself answer whether the texture is the equilibrium state, how large it is, how long it lives, or how much current moves it. Those are energetic and dynamical questions.

Required background. Magnetic Anisotropy supplies the exchange, anisotropy and magnetostatic energies, while Homotopy and Winding supplies the winding and topological-charge language.

Helpful background. Ferromagnetism provides the familiar order-parameter branch, while Spintronics supplies current-induced torques and electrical detection.

Magnetization textures and skyrmion charge

Section titled “Magnetization textures and skyrmion charge”

Unless stated otherwise, consider a thin magnetic layer in the oriented xyxy plane with normal +z^+\hat{\mathbf z}. A ferromagnetic texture is represented by

m(x,y)=M(x,y)Ms,∣m∣=1.\mathbf m(x,y) = \frac{\mathbf M(x,y)}{M_s}, \qquad |\mathbf m|=1.

The oriented skyrmion-density convention used here is

q(x,y)=14πm⋅(∂xm×∂ym),q(x,y) = \frac{1}{4\pi} \mathbf m\cdot \left( \partial_x\mathbf m \times \partial_y\mathbf m \right),

and the total charge is

Q=∫q(x,y) dx dy.Q = \int q(x,y)\, \mathrm dx\,\mathrm dy.

Reversing the spatial orientation, exchanging xx and yy, or reversing every spin changes the sign of QQ. A paper that quotes only “Q=1Q=1” without its orientation and core/background convention has not fully specified the texture.

Integer quantization requires more than smooth local magnetization. If

m(r)⟶m∞as∣r∣→∞,\mathbf m(\mathbf r) \longrightarrow \mathbf m_\infty \quad \text{as} \quad |\mathbf r|\to\infty,

the plane plus its point at infinity is topologically a sphere:

R2∪{∞}≃S2.\mathbb R^2\cup\{\infty\} \simeq S^2.

The texture is then a map

m:Sspace2⟶Sspin2,\mathbf m:S^2_{\mathrm{space}} \longrightarrow S^2_{\mathrm{spin}},

whose degree belongs to

π2(S2)=Z.\pi_2(S^2) = \mathbb Z.

An open edge or a nonuniform far field removes this particular quantization argument, so a finite-region integral need not be an integer. A vanishing amplitude or singularity can invalidate the smooth unit-vector map itself. Constant boundary conditions are not the only route to integer degree: a smooth periodic texture defines a map from a spatial torus to the spin sphere and also has integer charge per periodic cell.

The relevant real-space boundary differs among defects:

Texture Surrounding object in real space Typical classification Essential boundary statement
Domain wall two points on opposite sides π0(M)\pi_0(\mathcal M) the two domains lie in disconnected minima
Vortex closed loop around a core π1(M)\pi_1(\mathcal M) the order parameter remains in the allowed manifold on the loop
Skyrmion compactified two-dimensional plane π2(M)\pi_2(\mathcal M) the far field approaches one constant value

Here M\mathcal M is the actual order-parameter manifold. It need not be S2S^2. An easy-plane magnet, an antiferromagnet whose microscopic state genuinely identifies opposite Néel vectors, a noncollinear magnet, and a multiferroic can have different manifolds and different defect classifications. Homotopy and Winding supplies the general mathematical language.

Néel and Bloch skyrmion helicities with identical charge, followed by cumulative charge within a finite observation radius for a skyrmion and a meron.

Top: rotating the in-plane arrows from radial to tangential changes helicity without changing Q=−1Q=-1 for the down-core, up-background skyrmion. The arrows show the ring where mz=0m_z=0; the outer symbols denote the far field. Bottom: exact enclosed charges for the two radial profiles introduced below. A restricted image of a skyrmion can contain Q(R)=−1/2Q(R)=-1/2 even though its full-plane charge is −1-1; that alone does not make the full texture a meron.

For a film of thickness tft_f with magnetization uniform through its thickness, a representative micromagnetic energy is

E[m]=tf∫Ωd2r [A∑i=x,y(∂im)2+fD+Ku(1−mz2)−μ0MsHzmz]+Ed[m].E[\mathbf m] = t_f\int_{\Omega}\mathrm d^2r\, \big[ A \sum_{i=x,y} (\partial_i\mathbf m)^2 + f_{\mathrm D} + K_u(1-m_z^2) - \mu_0M_sH_zm_z \big] +E_d[\mathbf m].

Here Ω\Omega is the film footprint, AA has units of joules per meter, and the local densities have units of joules per cubic meter; the factor tft_f makes their integral an energy. The local anisotropy KuK_u excludes magnetostatic shape energy. The Dzyaloshinskii–Moriya density fDf_{\mathrm D} depends on crystal and interface symmetry, while EdE_d is the full nonlocal magnetostatic energy, including the stray field outside the film. Their canonical forms and sign conventions are developed in Magnetic Anisotropy. Replacing EdE_d by its local thin-film approximation gives Keff=Ku−μ0Ms2/2K_{\mathrm{eff}}=K_u-\mu_0M_s^2/2; one must then omit the full EdE_d rather than count that shape term twice.

Under a dilation

mλ(r)=m(r/λ),\mathbf m_\lambda(\mathbf r) = \mathbf m(\mathbf r/\lambda),

at fixed film thickness, consider the finite excess energy relative to the uniform background. For a sufficiently localized profile on the whole plane, the local terms scale as

Eex(λ)∝λ0,ED(λ)∝λ,EK(λ), EH(λ)∝λ2.\begin{aligned} E_{\mathrm{ex}}(\lambda) &\propto \lambda^0, \\ E_{\mathrm D}(\lambda) &\propto \lambda, \\ E_K(\lambda), \ E_H(\lambda) &\propto \lambda^2. \end{aligned}

Dipolar energy and finite boundaries have additional geometry dependence. A finite texture radius can be selected when terms with different scaling balance. Topological charge alone supplies no length scale.

For the ideal two-dimensional O(3)O(3) sigma model, define

Eσ=J2∫d2r [(∂xm)2+(∂ym)2].E_\sigma = \frac{J}{2} \int\mathrm d^2r\, \left[ (\partial_x\mathbf m)^2 + (\partial_y\mathbf m)^2 \right].

Here JJ has units of energy; the film exchange term above corresponds to J=2AtfJ=2At_f. Completing a square gives the Belavin–Polyakov bound

Eσ≥4πJ∣Q∣.E_\sigma \ge 4\pi J|Q|.

Configurations saturating the bound have a continuous size modulus: exchange alone neither selects a preferred radius nor makes the skyrmion the thermodynamic ground state. Lattice discreteness can remove scale invariance and permit collapse, while Dzyaloshinskii–Moriya coupling, frustrated exchange, anisotropy, field, dipolar energy, confinement, or higher-order interactions can stabilize a finite size.

Three stability statements must be kept separate:

  • topological distinction means a smooth deformation is obstructed under declared boundary and fixed-length assumptions;
  • metastability means the texture is a local free-energy minimum separated by a finite barrier;
  • thermodynamic stability means it minimizes the relevant free energy against every competing phase.

A skyrmion can be topologically nontrivial and metastable, while a skyrmion lattice is stable only within a material- and geometry-dependent phase region.

An easy-axis ferromagnet has two uniform minima,

m=±z^.\mathbf m = \pm\hat{\mathbf z}.

A 180∘180^\circ wall interpolates between them. With an oriented coordinate xx, define a one-dimensional wall charge

qDW=12[mz(−∞)−mz(+∞)].q_{\mathrm{DW}} = \frac{1}{2} \left[ m_z(-\infty) - m_z(+\infty) \right].

An up-to-down wall has qDW=+1q_{\mathrm{DW}}=+1 in this convention; reversing the domains reverses the sign. This charge records the boundary interpolation and is not the two-dimensional skyrmion number QQ.

In the local thin-film approximation, with residual nonlocal stray-field energy neglected, exchange stiffness AA and positive effective easy-axis anisotropy KeffK_{\mathrm{eff}} give the ideal wall scale and energy per wall area

Δ=AKeff,σ0=4AKeff.\Delta = \sqrt{ \frac{A}{K_{\mathrm{eff}}} }, \qquad \sigma_0 = 4\sqrt{ AK_{\mathrm{eff}} }.

The corresponding energy per length of wall in the film plane is tfσ0t_f\sigma_0. Those results, including the full minimizing profile and width-convention warning, are derived at From anisotropy to magnetic textures.

A Bloch wall rotates through an in-plane direction parallel to the wall, whereas a Néel wall rotates through the wall normal. Magnetostatics, thickness, crystal symmetry, and interfaces decide which costs less. Dzyaloshinskii–Moriya coupling can select both wall type and handedness, but inferring DD from a wall requires the other energy terms and boundary conditions too.

Two collective coordinates often describe a nearly rigid wall:

X(t),Φ(t),X(t), \qquad \Phi(t),

where XX is wall position and Φ\Phi its internal rotation angle. Field or current can couple translation to internal precession. Above a material- and geometry-dependent Walker scale, Φ\Phi no longer remains stationary and the simple steady-velocity picture fails. Pinning, wall tilting, deformation, and nucleation frequently matter before that ideal threshold.

Walls can terminate at a sample boundary, meet other walls, or change character through a three-dimensional singularity such as a Bloch point. Their dynamics therefore depends on both local texture and global domain geometry.

In a thin disk, magnetostatic energy often favors in-plane flux closure. Far from a small core, write

m∥=(cos⁡Φ,sin⁡Φ),\mathbf m_\parallel = \left( \cos\Phi, \sin\Phi \right),

with

Φ(φ)=nφ+γ.\Phi(\varphi) = n\varphi+\gamma.

The integer

n=12π∮∇Φ⋅dℓn = \frac{1}{2\pi} \oint \boldsymbol{\nabla}\Phi\cdot \mathrm d\boldsymbol{\ell}

is the vorticity. The phase γ\gamma sets circulation or helicity. Near the center, the magnetization turns out of plane to avoid an exchange singularity. Its polarity is

p=mz(0)=±1.p = m_z(0) = \pm1.

For the axisymmetric profile

m=(sin⁡θ(r)cos⁡[nφ+γ]sin⁡θ(r)sin⁡[nφ+γ]cos⁡θ(r)),\mathbf m= \begin{pmatrix} \sin\theta(r)\cos[n\varphi+\gamma]\\ \sin\theta(r)\sin[n\varphi+\gamma]\\ \cos\theta(r) \end{pmatrix},

the skyrmion charge inside a circular region is

Q=n2[cos⁡θ(0)−cos⁡θ(∞)].Q = \frac{n}{2} \left[ \cos\theta(0) - \cos\theta(\infty) \right].

A magnetic vortex with in-plane far field has

cos⁡θ(∞)=0,\cos\theta(\infty)=0,

so

Qvortex=np2.Q_{\mathrm{vortex}} = \frac{np}{2}.

It covers half the spin sphere and is therefore called a meron. The half-integer is compatible with topology because the far-field magnetization is not one constant point on S2S^2; it winds around the equator.

Vorticity, polarity, and circulation are distinct labels. Reversing the core changes pp and QQ without changing the in-plane winding. Reversing circulation can change γ\gamma without changing nn or QQ. A vortex can annihilate with an antivortex, leave through an edge, or reverse polarity through a short-lived singular core.

The same gyroforce that appears for skyrmions produces gyrotropic vortex-core motion. Confinement supplies a restoring force, yielding a low-frequency orbit whose sense depends on core polarity under standard conventions.

For the axisymmetric ansatz above, choose a down core and up background:

θ(0)=π,θ(∞)=0.\theta(0)=\pi, \qquad \theta(\infty)=0.

Then

Q=−n.Q=-n.

With n=+1n=+1, this page therefore calls the texture Q=−1Q=-1. Other sign conventions are common.

For n=+1n=+1, helicities γ=0,π\gamma=0,\pi give Néel-type radial rotation, while γ=π/2,3π/2\gamma=\pi/2,3\pi/2 give Bloch-type tangential rotation.

Topological charge does not determine helicity. Two textures can have the same QQ and different in-plane winding patterns, energies, and responses.

An antiskyrmion has the opposite winding structure and typically anisotropic helicity around its perimeter. It is favored by selected anisotropic Dzyaloshinskii–Moriya tensors rather than by the isotropic bulk or ideal interfacial forms. A skyrmionium can contain nested walls with total Q=0Q=0. Magnetic bubbles can have Q=0Q=0 or nonzero QQ depending on their complete vector texture. A circular image alone does not determine the topological class.

In a bulk field-polarized background, an isolated skyrmion is commonly an excitation or metastable state; confinement can instead make a single skyrmion the equilibrium configuration of a finite sample. A skyrmion crystal is a periodic magnetic phase with one or more topological objects per magnetic unit cell. Reciprocal-space Bragg peaks establish periodic order, while real-space or polarization-sensitive information is needed to determine the vector texture and charge.

A simple n=1n=1 skyrmion profile has

mz(r)=r2−a2r2+a2,sin⁡θ(r)=2arr2+a2.m_z(r)=\frac{r^2-a^2}{r^2+a^2}, \qquad \sin\theta(r)=\frac{2ar}{r^2+a^2}.

The scale a>0a>0 is the radius where mz=0m_z=0. Integrating only to radius RR gives

Q(R)=−R2R2+a2.Q(R)=-\frac{R^2}{R^2+a^2}.

At R=aR=a the image contains only half the charge; even R=5aR=5a gives Q(R)=−25/26Q(R)=-25/26. In contrast, an up-core meron with mz(r)=e−r2/a2m_z(r)=e^{-r^2/a^2} and n=1n=1 has

Q(R)=12(1−e−R2/a2)⟶12.Q(R)=\frac12\left(1-e^{-R^2/a^2}\right) \longrightarrow\frac12.

The distinction lies in the complete far field, not whether a finite integral happens to equal a half-integer. These analytic profiles illustrate topology; they are not asserted to minimize a specific material’s full micromagnetic energy.

Different mechanisms stabilize superficially similar objects:

  • bulk Dzyaloshinskii–Moriya coupling in chiral crystals commonly favors Bloch-type twists;
  • interfacial Dzyaloshinskii–Moriya coupling in polar multilayers commonly favors Néel-type twists;
  • anisotropic Dzyaloshinskii–Moriya coupling can favor antiskyrmions;
  • dipolar energy can stabilize magnetic bubbles and flux-closure textures even without Dzyaloshinskii–Moriya coupling;
  • frustrated exchange can select finite-wavevector and multi-QQ textures in centrosymmetric magnets;
  • itinerant multi-spin or Fermi-surface-mediated interactions can stabilize short-period noncoplanar order;
  • confinement and patterned boundaries can stabilize states absent in the bulk phase diagram.

Broken inversion permits particular Dzyaloshinskii–Moriya invariants; it does not guarantee a skyrmion phase. Likewise, centrosymmetry forbids conventional pairwise Dzyaloshinskii–Moriya coupling on inversion-symmetric bonds but does not forbid all skyrmions.

Useful material families include chiral B20 magnets, polar magnets, ultrathin heavy-metal/ferromagnet multilayers, frustrated centrosymmetric magnets, ferrimagnetic films, antiferromagnets, and magnetic insulators. Their characteristic sizes span atomic to micrometre scales, and their stability windows vary greatly. “Skyrmion material” is therefore a phase-diagram statement, not merely a chemical label.

Creation, annihilation, and conditional protection

Section titled “Creation, annihilation, and conditional protection”

In a smooth fixed-length continuum on a closed surface, QQ cannot change continuously. Real magnets evade one of those assumptions through:

  • escape across a physical boundary;
  • a Bloch point or other three-dimensional singularity;
  • local suppression of ∣M∣|\mathbf M| near a high-temperature or itinerant core;
  • atomic-scale lattice evolution for which the continuum map ceases to be smooth;
  • nucleation from a defect, notch, contact, or strongly driven region.

Topology can therefore raise an activation barrier and prolong lifetime, but it does not make a texture indestructible. The barrier depends on the actual annihilation path and can be much smaller at an edge or defect than in a perfect bulk calculation.

When a conduction electron follows a nondegenerate local spin band adiabatically, its state accumulates a real-space Berry phase. Let e>0e>0, let ±\pm label eigenvalues ±1\pm1 of σ⋅m\boldsymbol\sigma\cdot\mathbf m, and represent the effective Lorentz force using the electron charge −e-e for both bands. This convention gives

Bem,z±=±ℏ2em⋅(∂xm×∂ym).B_{\mathrm{em},z}^{\pm} = \pm \frac{\hbar}{2e} \mathbf m\cdot \left( \partial_x\mathbf m \times \partial_y\mathbf m \right).

The emergent flux through one smooth texture is

Φem±=∫Bem,z±dx dy=±heQ.\begin{aligned} \Phi_{\mathrm{em}}^\pm &= \int B_{\mathrm{em},z}^{\pm} \mathrm dx\,\mathrm dy \\ &= \pm \frac{h}{e} Q. \end{aligned}

The labels refer to physical spin, not automatically to majority and minority populations or magnetic-moment direction. With the conventions fixed, the magnitude is one ordinary flux quantum h/eh/e per unit ∣Q∣|Q| in this adiabatic continuum limit. It is an effective Berry field, not an additional Maxwell magnetic flux measured by a pickup coil.

For a time-dependent texture, the corresponding emergent electric field can be written

Eem,i±=±ℏ2em⋅(∂im×∂tm).E_{\mathrm{em},i}^{\pm} = \pm \frac{\hbar}{2e} \mathbf m\cdot \left( \partial_i\mathbf m \times \partial_t\mathbf m \right).

For rigid translation, ∂tm=−(v⋅∇)m\partial_t\mathbf m=-(\mathbf v\cdot\boldsymbol\nabla)\mathbf m, so Eem±=−v×Bem±\mathbf E_{\mathrm{em}}^\pm=-\mathbf v\times\mathbf B_{\mathrm{em}}^\pm. This provides a direct sign check and explains the spin-dependent electromotive response (Everschor-Sitte and Sitte, 2014). The adiabatic approximation requires texture and time scales slow enough to suppress transitions between the local spin bands.

On a lattice, the local precursor is scalar spin chirality,

χijk=mi⋅(mj×mk).\chi_{ijk} = \mathbf m_i\cdot \left( \mathbf m_j\times\mathbf m_k \right).

For a small triangle of nearly parallel spins, the oriented spherical area is Ωijk≃χijk/2\Omega_{ijk}\simeq\chi_{ijk}/2. Summing those areas gives the continuum Berry flux. At atomic scales, however, band structure, nonadiabaticity, multiple orbitals, and momentum-space Berry curvature can invalidate a simple emergent-field estimate.

An often used one-band estimate is

ρyxT≃PR0⟨Bem⟩,\rho_{yx}^{\mathrm T} \simeq P R_0 \langle B_{\mathrm{em}}\rangle,

For one parabolic electron band split into two adiabatic spin channels with equal mobilities and weak Hall angles, R0=−1/(ne)R_0=-1/(ne), P=(n+−n−)/nP=(n_+-n_-)/n and Bem=Bem+B_{\mathrm{em}}=B_{\mathrm{em}}^+. Unequal mobilities change the weighting of the two spin channels; PP cannot then be inferred from carrier numbers alone. The estimate is not a universal extraction formula. Multiband transport, anomalous Hall evolution, nonadiabatic scattering, inhomogeneity, and changing magnetic phases can all produce or reshape a Hall residual. A “topological Hall” hump is supporting evidence only when combined with independent texture information and a controlled background model.

Projecting the Landau–Lifshitz–Gilbert equation onto a slowly translating texture gives a Thiele-type force balance. Using the negative-precession-sign Gilbert equation and the texture torques defined in Spintronics, the force balance is

G×(v−u)+D(αv−βu)+∇RU−Fext=0.\mathbf G \times \left( \mathbf v-\mathbf u \right) + \mathsf D \left( \alpha\mathbf v - \beta\mathbf u \right) + \boldsymbol{\nabla}_{\mathbf R}U - \mathbf F_{\mathrm{ext}} = 0.

Here:

  • v=R˙\mathbf v=\dot{\mathbf R} is the velocity of the texture position R\mathbf R;
  • u\mathbf u is the signed adiabatic spin-transfer velocity in the term −(u⋅∇)m-(\mathbf u\cdot\boldsymbol\nabla)\mathbf m, not necessarily the electron drift velocity;
  • G=Gz^\mathbf G=G\hat{\mathbf z} is the gyrovector;
  • D\mathsf D is a symmetric positive-semidefinite dissipative tensor built from texture gradients, with material prefactors included so that each term is a force;
  • α≥0\alpha\ge0 is Gilbert damping and β\beta a nonadiabatic coefficient;
  • U(R)U(\mathbf R) is a static potential energy, including confinement, defects, and interactions;
  • Fext\mathbf F_{\mathrm{ext}} represents drives not already included in UU, such as an applied spin–orbit torque.

For a uniform ferromagnetic film in these conventions,

s=Mstf∣γ∣,G=4πsQ,Dij=s∫∂im⋅∂jm d2r.\begin{aligned} s&=\frac{M_s t_f}{|\gamma|},\\ G&=4\pi sQ,\\ D_{ij}&=s\int \partial_i\mathbf m\cdot\partial_j\mathbf m\,\mathrm d^2r. \end{aligned}

Here ss is the positive angular-momentum magnitude per area and ∣γ∣|\gamma| is in s−1T−1\mathrm{s^{-1}T^{-1}}. The sign of GG follows from the choice of magnetization rather than electron-spin direction and the displayed Gilbert/force conventions; other conventions reverse it together with other signs. Projection onto m×∂im\mathbf m\times\partial_i\mathbf m gives the antisymmetric integral ∫m⋅(∂xm×∂ym) d2r=4πQ\int\mathbf m\cdot(\partial_x\mathbf m\times\partial_y\mathbf m)\,\mathrm d^2r=4\pi Q.

For u=0\mathbf u=0, taking the scalar product with v\mathbf v checks the force signs:

dUdt=Fext⋅v−α v⋅Dv.\frac{\mathrm dU}{\mathrm dt} =\mathbf F_{\mathrm{ext}}\cdot\mathbf v -\alpha\,\mathbf v\cdot\mathsf D\mathbf v.

Without an external drive the potential energy cannot increase. The gyroscopic force does no work.

The gyroscopic term is transverse to motion and produces a skyrmion Hall angle in a ferromagnet. Damping produces a longitudinal drag. Pinning can impose a threshold. Smooth deformation changes D\mathsf D and the drive coupling, but at fixed QQ, MsM_s, tft_f and γ\gamma it does not change G=4πsQG=4\pi sQ. Spatially varying material weights, escape through an edge or topology change require reconsidering that statement.

In an ideal bipartite antiferromagnet, opposite sublattice gyrovectors can cancel, suppressing transverse drift. In a ferrimagnet, the gyroscopic coefficient can pass through zero near angular-momentum compensation. Neither cancellation is automatic in a real multilayer, canted state or uncompensated interface. Near compensation, inertial and internal-mode terms omitted from this first-order equation can become important.

The Thiele equation omits internal modes. Skyrmions can breathe, gyrate, deform, split, couple to magnons, and acquire effective inertia through additional coordinates. Near annihilation, collision, or strong drive, a rigid-particle interpretation can fail completely.

Directly replacing derivatives by finite differences is fragile when a wall spans only a few pixels. A geometric method triangulates the image or simulation mesh. For an oriented triangle (i,j,k)(i,j,k) of unit vectors, define

χijk=mi⋅(mj×mk),\chi_{ijk}=\mathbf m_i\cdot(\mathbf m_j\times\mathbf m_k), dijk=1+mi⋅mj+mj⋅mk+mk⋅mi.d_{ijk}={}1+\mathbf m_i\cdot\mathbf m_j +\mathbf m_j\cdot\mathbf m_k+\mathbf m_k\cdot\mathbf m_i.

Its signed solid angle is

Ωijk=2atan2⁡(χijk,dijk).\Omega_{ijk}=2\operatorname{atan2}(\chi_{ijk},d_{ijk}).

Then

Qlat=14π∑△Ωijk.Q_{\mathrm{lat}} = \frac{1}{4\pi} \sum_{\triangle} \Omega_{ijk}.

All triangles must use one orientation and the same geodesic interpolation convention (Berg and Lüscher, 1981). Antipodal pairs are ambiguous, but they are not the only exceptional configurations. If the triple product vanishes while the second argument of atan2⁡\operatorname{atan2} is nonpositive, the branch can jump. For example, three equatorial spins separated by 120∘120^\circ bound either hemisphere, despite having no antipodal pair.

Use enough spatial resolution to follow the wall, and test changes of mesh, triangulation and reconstruction. The complete vector field and its boundary treatment are essential: normalizing noisy pixels or artificially fixing an image boundary can change the inferred charge. For a nonexceptional closed or periodic triangulation, the geometric sum has integer degree; an open crop need not.

No single probe universally measures QQ.

Probe Primary sensitivity What remains model dependent
Lorentz transmission electron microscopy projected in-plane induction and deflection contrast three-dimensional magnetization, core polarity, thickness and defocus transfer
Spin-polarized scanning tunneling microscopy surface magnetic contrast with atomic resolution tip polarization, vector reconstruction, subsurface texture
XMCD photoemission or transmission microscopy element-specific magnetization projection missing vector components, depth averaging, domain overlap
MFM or scanning NV magnetometry stray field above the sample inverse reconstruction, material parameters, buried layers
Small-angle neutron or resonant x-ray scattering periodic wavevectors, orientation, selected chirality information individual-object topology and defects
Hall transport transverse electrical response ordinary/anomalous backgrounds, adiabaticity, multiband coefficients
Microwave and terahertz spectroscopy collective gyration and breathing modes mode assignment and coexistence with non-skyrmion phases

Magnetic contrast first constrains candidate textures. Multiple projections, field and temperature dependence, and a forward model of the probe then help distinguish a trivial bubble from a Néel or Bloch skyrmion. A numerical charge requires enough information to determine the vector field, including its core and boundary. Scattering, transport and mode spectra provide independent constraints on the same model.

Imaging circles plus a Hall hump is not yet a topology measurement. Conversely, imperfectly quantized QQ from finite-resolution open-boundary data does not automatically refute a skyrmion interpretation. Compare the uncertainty from missing components, reconstruction and finite field of view before assigning a topological class. Hall Measurements discusses the transport backgrounds in more detail.

For

m=(sin⁡θcos⁡[nφ+γ]sin⁡θsin⁡[nφ+γ]cos⁡θ),\mathbf m= \begin{pmatrix} \sin\theta\cos[n\varphi+\gamma]\\ \sin\theta\sin[n\varphi+\gamma]\\ \cos\theta \end{pmatrix},

derive

Q=n2[cos⁡θ(0)−cos⁡θ(∞)].Q = \frac{n}{2} \left[ \cos\theta(0) - \cos\theta(\infty) \right].

Does QQ depend on helicity γ\gamma?

Solution

In polar coordinates,

dx dy=r dr dφ,\mathrm dx\,\mathrm dy = r\,\mathrm dr\,\mathrm d\varphi,

and

m⋅(∂xm×∂ym)=1rm⋅(∂rm×∂φm).\mathbf m\cdot(\partial_x\mathbf m\times\partial_y\mathbf m) =\frac1r\mathbf m\cdot (\partial_r\mathbf m\times\partial_\varphi\mathbf m).

For the ansatz,

m⋅(∂rm×∂φm)=nθ′(r)sin⁡θ.\mathbf m\cdot \left( \partial_r\mathbf m \times \partial_\varphi\mathbf m \right) = n\theta'(r)\sin\theta.

Therefore

Q=n2∫0∞θ′sin⁡θ dr=n2[cos⁡θ(0)−cos⁡θ(∞)].\begin{aligned} Q &= \frac{n}{2} \int_0^\infty \theta'\sin\theta\, \mathrm dr \\ &= \frac{n}{2} \left[ \cos\theta(0) - \cos\theta(\infty) \right]. \end{aligned}

The constant γ\gamma drops out. Helicity changes the in-plane pattern but not the degree.

Starting from

Eσ=J2∫[(∂xm)2+(∂ym)2]d2r,E_\sigma = \frac{J}{2} \int \left[ (\partial_x\mathbf m)^2 + (\partial_y\mathbf m)^2 \right] \mathrm d^2r,

use ∣m∣=1|\mathbf m|=1 to prove

Eσ≥4πJ∣Q∣.E_\sigma \ge 4\pi J|Q|.
Solution

Because m⋅∂im=0\mathbf m\cdot\partial_i\mathbf m=0,

∣m×∂ym∣2=∣∂ym∣2.|\mathbf m\times\partial_y\mathbf m|^2 = |\partial_y\mathbf m|^2.

Positivity gives

0≤J2∫∣∂xm±m×∂ym∣2d2r.0 \le \frac{J}{2} \int \left| \partial_x\mathbf m \pm \mathbf m\times\partial_y\mathbf m \right|^2 \mathrm d^2r.

Expanding the square and using the scalar triple product yields

0≤Eσ∓4πJQ.0 \le E_\sigma \mp 4\pi JQ.

Choose the sign appropriate to the sign of QQ:

Eσ≥4πJ∣Q∣.E_\sigma \ge 4\pi J|Q|.

Saturating the bound constrains the texture to a first-order self-duality equation. The bound fixes energy within a charge sector but does not select a radius.

A rigid texture moves with constant velocity v=(vx,vy,0)\mathbf v=(v_x,v_y,0). Use the emergent-field definitions to find Eem\mathbf E_{\mathrm{em}} and check Faraday’s law for a smooth Bem,z(x−vxt,y−vyt)B_{\mathrm{em},z}(x-v_xt,y-v_yt).

Solution

Substitution of ∂tm=−vx∂xm−vy∂ym\partial_t\mathbf m=-v_x\partial_x\mathbf m-v_y\partial_y\mathbf m gives

Eem,x=−vyBem,z,Eem,y=vxBem,z.\begin{aligned} E_{\mathrm{em},x}&=-v_yB_{\mathrm{em},z},\\ E_{\mathrm{em},y}&=v_xB_{\mathrm{em},z}. \end{aligned}

Thus Eem=−v×Bem\mathbf E_{\mathrm{em}}=-\mathbf v\times\mathbf B_{\mathrm{em}}. Its curl obeys

(∇×Eem)z=v⋅∇Bem,z=−∂tBem,z.(\boldsymbol\nabla\times\mathbf E_{\mathrm{em}})_z =\mathbf v\cdot\boldsymbol\nabla B_{\mathrm{em},z} =-\partial_t B_{\mathrm{em},z}.

Both spin bands satisfy the relation, with opposite fields. Singularities where the smooth spin-band projection fails require separate treatment.

4. Hall angle from a simple Thiele balance

Section titled “4. Hall angle from a simple Thiele balance”

Set u=0\mathbf u=0, take UU constant, and apply Fext=Fx^\mathbf F_{\mathrm{ext}}=F\hat{\mathbf x}, so that

Gz^×v+αDv=Fx^,G\hat{\mathbf z}\times\mathbf v + \alpha D\mathbf v = F\hat{\mathbf x},

with scalar D>0D>0. Find vxv_x, vyv_y, and the Hall angle.

Solution

Since

z^×v=−vyx^+vxy^,\hat{\mathbf z}\times\mathbf v = - v_y\hat{\mathbf x} + v_x\hat{\mathbf y},

the component equations are

−Gvy+αDvx=F,-Gv_y+\alpha Dv_x=F,

and

Gvx+αDvy=0.Gv_x+\alpha Dv_y=0.

Solving,

vx=FαDG2+(αD)2,v_x = \frac{ F\alpha D }{ G^2+(\alpha D)^2 },

and

vy=−FGG2+(αD)2.v_y = - \frac{ FG }{ G^2+(\alpha D)^2 }.

Thus

tan⁡ΘSkH=vyvx=−GαD.\tan\Theta_{\mathrm{SkH}} = \frac{v_y}{v_x} = - \frac{G}{\alpha D}.

The sign follows the stated gyrovector and force conventions. Pinning, drive-dependent deformation, and edges can change the observed angle.

5. An ambiguous triangle without antipodal spins

Section titled “5. An ambiguous triangle without antipodal spins”

Take three unit vectors in the equatorial plane with azimuths 00, 2π/32\pi/3 and 4π/34\pi/3. Evaluate the two arguments of the solid-angle formula. What changes if all three acquire the same small positive or negative zz component before normalization?

Solution

Every pair has dot product −1/2-1/2, while the triple product vanishes. The two arguments are therefore 00 and 1−3/2=−1/21-3/2=-1/2. The triangle runs around a great circle; choosing either hemisphere gives an area of magnitude 2π2\pi.

An infinitesimal positive common zz component gives a positive triple product, selecting Ω→+2π\Omega\to+2\pi. A negative component selects Ω→−2π\Omega\to-2\pi. The jump is 4π4\pi, or one unit in the sum defining QlatQ_{\mathrm{lat}}. No pair was antipodal. Such a configuration needs a finer spatial model or an explicit interpolation choice; rounding the resulting charge does not resolve the ambiguity.

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