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Cooperative Charge Pumping and Enhanced Skyrmion Mobility Adel Abbout and Aur´ elien Manchon King Abdullah University of Science and Technology (KAUST), Physical Science and Engineering Division, Thuwal 23955-6900, Saudi Arabia Joseph Weston and Xavier Waintal University Grenoble Alpes, INAC-PHELIQS, F-38000 Grenoble, France CEA, INAC-PHELIQS, F-38000 Grenoble, France The electronic pumping arising from the steady motion of ferromagnetic skyrmions is investigated by solving the time evolution of the Schr¨ odinger equation implemented on a tight-binding model with the statistical physics of the many-body problem. It is shown that the ability of steadily moving skyrmions to pump large charge currents arises from their non-trivial magnetic topology, i.e. the coexistence between spin-motive force and topological Hall effect. Based on an adiabatic scattering theory, we compute the pumped current and demonstrate that it scales with the reflection coefficient of the conduction electrons against the skyrmion. Finally, we propose that such a phenomenon can be exploited in the context of racetrack devices, where the electronic pumping enhances the collective motion of the train of skyrmions. PACS numbers: Introduction - The electrical manipulation of mag- netic textures has stimulated intense investigations lately, unraveling a wealth of dynamical phenomena that can be exploited towards memory and logic applications [1, 2]. Among the vast zoology of existing magnetic textures, skyrmions are regarded as promising candidates for high- density storage and logic applications [3]. Magnetic skyrmions are topologically nontrivial magnetic textures characterized by a quantized topological charge [4, 5]. While skymions were originally obtained in the form of stable lattices in bulk non-centrosymmetric magnets [6, 7] or at metallic interfaces [8] at low temperature, a recent breakthrough has led to the observation of individ- ual metastable magnetic skyrmions at room temperature at transition metal interfaces [912]. This achievement enables the electrical manipulation of individual bits of information and the in-depth investigation of current- driven skyrmion motion in thin nanowires. The superior- ity attributed to magnetic skyrmions compared to mag- netic domain walls is related to their topology and to the energy barrier that needs to be overcome to annihilate a skyrmion [13]. This property makes them robust against certain classes of defects (point defects, edge roughness) and weakly deformable when subjected to reasonable (field or current) drive [14]. As a result, skyrmions are expected to display high mobility and low critical driving current in weakly disordered media [15]. Although this topological protection does not apply in strongly disor- dered systems, recent experiments in polycrystalline thin films have shown that skyrmions can reach mobilities as large as 100 m/s for current densities of 5×10 7 A/cm 2 [10], comparable to domain walls. Another important characteristic of magnetic skyrmions is the presence of a spin-Berry phase resulting in an emergent electromagnetic field [16]. In- deed, the chiral configuration of the magnetic moments forming the skyrmion gets imprinted in the wavefunction of the conduction electrons such that they experience a spin-dependent effective electromagnetic field [17, 18] E s em =(s~/2e)[m · (t m × i m)]e i , (1) B s em = - ijk (s~/2e)[m · (i m × j m)]e k , (2) where m is the unit magnetization vector, ijk is Levi- Cevita symbol, e i is the i-th unit vector in cartesian co- ordinates and s = ±1 accounts for spin projection on m. When the skyrmion is static, E s em 0 and the emergent magnetic field B s em is responsible for the devia- tion of the flowing electron trajectory, resulting in topo- logical charge and spin Hall effects [13, 19], as well as topological torque [20, 21]. As a reaction, the skyrmion experiences a Magnus force that pushes it sideway, as observed experimentally [2325]. On the other hand, when the skyrmion is moving, E s em 6= 0, and it is ex- pected to pump spin and charge currents through the so-called spin-motive force, an effect experimentally re- ported in quasi-one dimensional magnetic domain walls (1D-DW) [26, 27]. In 1D-DW though, the charge pump- ing only occurs in the turbulent regime of motion, such that hE s em i = hm· (t m× i m)i6 = 0, and vanishes during steady motion (also known as the flow regime). In this Letter, we uncover the interplay between spin currents and skyrmion dynamics by directly solving the time-dependent Schr¨ odinger equation using state-of-the- art numerical tools [28, 29]. This approach enables us to describe the various pumping phenomena beyond the adiabatic limit [14]. We show that, in sharp contrast to 1D-DW, magnetic skyrmions moving steadily along nar- row nanowires pump a sizable charge current that can be detected experimentally. We propose to take advan- tage of these phenomena in a magnetic racetrack and arXiv:1804.02460v1 [cond-mat.mtrl-sci] 6 Apr 2018

Cooperative Charge Pumping and Enhanced Skyrmion MobilityIn this Letter, we uncover the interplay between spin currents and skyrmion dynamics by directly solving the time-dependent

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Page 1: Cooperative Charge Pumping and Enhanced Skyrmion MobilityIn this Letter, we uncover the interplay between spin currents and skyrmion dynamics by directly solving the time-dependent

Cooperative Charge Pumping and Enhanced Skyrmion Mobility

Adel Abbout and Aurelien ManchonKing Abdullah University of Science and Technology (KAUST),

Physical Science and Engineering Division, Thuwal 23955-6900, Saudi Arabia

Joseph Weston and Xavier WaintalUniversity Grenoble Alpes, INAC-PHELIQS, F-38000 Grenoble,

France CEA, INAC-PHELIQS, F-38000 Grenoble, France

The electronic pumping arising from the steady motion of ferromagnetic skyrmions is investigatedby solving the time evolution of the Schrodinger equation implemented on a tight-binding modelwith the statistical physics of the many-body problem. It is shown that the ability of steadily movingskyrmions to pump large charge currents arises from their non-trivial magnetic topology, i.e. thecoexistence between spin-motive force and topological Hall effect. Based on an adiabatic scatteringtheory, we compute the pumped current and demonstrate that it scales with the reflection coefficientof the conduction electrons against the skyrmion. Finally, we propose that such a phenomenon canbe exploited in the context of racetrack devices, where the electronic pumping enhances the collectivemotion of the train of skyrmions.

PACS numbers:

Introduction - The electrical manipulation of mag-netic textures has stimulated intense investigations lately,unraveling a wealth of dynamical phenomena that can beexploited towards memory and logic applications [1, 2].Among the vast zoology of existing magnetic textures,skyrmions are regarded as promising candidates for high-density storage and logic applications [3]. Magneticskyrmions are topologically nontrivial magnetic texturescharacterized by a quantized topological charge [4, 5].While skymions were originally obtained in the formof stable lattices in bulk non-centrosymmetric magnets[6, 7] or at metallic interfaces [8] at low temperature, arecent breakthrough has led to the observation of individ-ual metastable magnetic skyrmions at room temperatureat transition metal interfaces [9–12]. This achievementenables the electrical manipulation of individual bits ofinformation and the in-depth investigation of current-driven skyrmion motion in thin nanowires. The superior-ity attributed to magnetic skyrmions compared to mag-netic domain walls is related to their topology and to theenergy barrier that needs to be overcome to annihilate askyrmion [13]. This property makes them robust againstcertain classes of defects (point defects, edge roughness)and weakly deformable when subjected to reasonable(field or current) drive [14]. As a result, skyrmions areexpected to display high mobility and low critical drivingcurrent in weakly disordered media [15]. Although thistopological protection does not apply in strongly disor-dered systems, recent experiments in polycrystalline thinfilms have shown that skyrmions can reach mobilities aslarge as 100 m/s for current densities of 5×107 A/cm2

[10], comparable to domain walls.

Another important characteristic of magneticskyrmions is the presence of a spin-Berry phaseresulting in an emergent electromagnetic field [16]. In-

deed, the chiral configuration of the magnetic momentsforming the skyrmion gets imprinted in the wavefunctionof the conduction electrons such that they experience aspin-dependent effective electromagnetic field [17, 18]

Esem = (s~/2e)[m · (∂tm× ∂im)]ei, (1)

Bsem = −εijk(s~/2e)[m · (∂im× ∂jm)]ek, (2)

where m is the unit magnetization vector, εijk is Levi-Cevita symbol, ei is the i-th unit vector in cartesian co-ordinates and s = ±1 accounts for spin projection onm. When the skyrmion is static, Esem → 0 and theemergent magnetic field Bs

em is responsible for the devia-tion of the flowing electron trajectory, resulting in topo-logical charge and spin Hall effects [13, 19], as well astopological torque [20, 21]. As a reaction, the skyrmionexperiences a Magnus force that pushes it sideway, asobserved experimentally [23–25]. On the other hand,when the skyrmion is moving, Esem 6= 0, and it is ex-pected to pump spin and charge currents through theso-called spin-motive force, an effect experimentally re-ported in quasi-one dimensional magnetic domain walls(1D-DW) [26, 27]. In 1D-DW though, the charge pump-ing only occurs in the turbulent regime of motion, suchthat 〈Esem〉 = 〈m ·(∂tm×∂im)〉 6= 0, and vanishes duringsteady motion (also known as the flow regime).

In this Letter, we uncover the interplay between spincurrents and skyrmion dynamics by directly solving thetime-dependent Schrodinger equation using state-of-the-art numerical tools [28, 29]. This approach enables usto describe the various pumping phenomena beyond theadiabatic limit [14]. We show that, in sharp contrast to1D-DW, magnetic skyrmions moving steadily along nar-row nanowires pump a sizable charge current that canbe detected experimentally. We propose to take advan-tage of these phenomena in a magnetic racetrack and

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Page 2: Cooperative Charge Pumping and Enhanced Skyrmion MobilityIn this Letter, we uncover the interplay between spin currents and skyrmion dynamics by directly solving the time-dependent

2

demonstrate that mutual charge pumping in a train ofskyrmions results in enhanced collective mobility.

Model and method - We consider a skyrmion in a per-pendicularly magnetized waveguide driven by an exter-nal force, and having a velocity v confined along the x-axis. In other words, Magnus force is cancelled due toconfinement. Since our interest lies on the electronicpumping induced by the skyrmion motion, the physi-cal origin of the external force that drives the motionis unimportant and can be a non-adiabatic torque [3],a topological torque [21] or spin Hall effect arising froman adjacent heavy metal [10]. Finally, we also assumethat the skyrmion remains stable and rigid throughoutits motion. Slight deformations of the skyrmion in thepresence of weak disorder is not expected to modify thepresent results qualitatively.

Within these assumptions, the real-space tight-bindingHamiltonian reads

H(t) = −γ∑〈i,j〉

c†i cj −∆∑i

mi(t) ·(c†i σci

)+ Vconf, (3)

where ci = (c↑i , c↓i ) is the annihilation operator for elec-

trons with spin up and spin down on site i = (x, y) and c†iis the corresponding creation operator. ∆ is the exchangeparameter, γ is the hopping coefficient and the sum 〈i, j〉is only taken over nearest neighbors. The magnetic tex-ture is described by the set of the magnetic momentsmi(t) which takes the form of a skyrmion with a centerlinearly translating in time in the x-direction at a velocityv. Thus, the dynamical texture reads

m =(√

1− l2(t) sinφ(t),√

1− l2(t) cosφ(t), l(t)), (4)

with l(t) = − cos(πr(t)/R) and sinφ(t) =(x − (x0 +

vt))/r(t) and r(t) =

√(x− (x0 + vt)

)2+ (y − y0)2. R

is the radius of the skyrmion and (x0, y0) is the initialposition of the skyrmion. Vconf is the waveguide confiningpotential (hard walls). Equation (3) is implemented ona tight-binding model consisting of a magnetic nanowireconnected to two (left and right) semi-infinite leads. Inthe present work, no bias voltage is applied across thesystem so that the currents computed only stem fromskyrmion-induced electronic pumping.

The main task in computing the different physicalobservables is to solve the time-dependent Schrodingerequation and to determine the different time-dependentpropagating wave functions ΨαE(t) coming from eachlead α at energy E. The total current flowing through across-section transverse to the waveguide direction reads

I(t) =∑α,ij

∫dE

2πfα(E)Iα,ij(E, t), (5)

where f(E) is Fermi-Dirac distribution, and Iα,ij(E, t) isthe current contribution of electrons coming from lead α

FIG. 1. (Color online) 2D map of the current lines at differ-ent times: (a) t = 4t0, (b) 50t0, (c) 100t0, and (d) 200t0.The black arrows denote the direction of the charge cur-rent, and the color shading amounts for the current gradient.The dark shaded region reveals the position of the skyrmion,where the current gradient is maximum. The parameters arev = 0.2a/t0, W = 31a, 2R = 15a and EF = −3.8γ. Initialskyrmion position is x(0) = 15a.

at energy E between sites i and j [28, 29], Iα,ij(E, t) =

2={

[Ψ†αE(t)]iHij(t)[ΨαE(t)]j}

. Here, ={...}

denotes theimaginary part. Equation (5) shows that the physicsof dynamical Hamiltonians is in general governed bythe whole Fermi sea and not just by the Fermi sur-face although, as discussed below, the restriction to lowskyrmion velocities makes the contribution of the Fermisurface dominating. The summation in Eq. (5) includesthe M propagating modes in the waveguide of width W(M = 2W

λ , λ being the electron wavelength).Skyrmion-induced electronic pumping - We now con-

sider a quasi-1D waveguide with a width W = 31a inwhich a skyrmion of diameter 2R = 15a is moving with avelocity v = 0.2a/t0, where a, t0 are the lattice and timesubdivisions respectively [30]. The exchange parameteris set to ∆ = 0.1γ. The skyrmion is set into motion byramping its velocity from zero to a steady value v over aramping time of ∼3t0. This ramping time is kept shortto minimize its impact on electronic pumping. A two-dimensional (2D) map of the charge current induced bythe skyrmion motion is plotted in Fig. 1 for various times.In the transient regime close to t = 0, current vorticesreveal the inhomogeneity of the wavefunction due to thepresence of the skyrmion [Fig. 1(a)]. At longer times, astationary regime establishes progressively Fig. 1(b)-(d).The streamlines show that the pumping is asymmetric

Page 3: Cooperative Charge Pumping and Enhanced Skyrmion MobilityIn this Letter, we uncover the interplay between spin currents and skyrmion dynamics by directly solving the time-dependent

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despite the axial symmetry of the system, unveiling thepresence of topological Hall effect.

FIG. 2. (Color online) Trace of the charge current computedat different interfaces in the waveguide. Each curve corre-sponds to the current probed at a specific interface, as indi-cated on the top sketch (dashed vertical lines). The coloredarrows indicate the time when the skyrmion center crosses aspecific interface. These interfaces are spaced by a distance of10a and the parameters are W = 51a, 2R = 15a, v = 0.2a/t0and ∆ = 0.1γ. The symbols H denote the current pumped bya 1D-DW with the same parameters. The inset is obtainedfor v = 0.05a/t0.

The total current pumped by the moving skyrmion isreported on Fig. 2 as a function of time and probedat different positions along the waveguide, as depictedin the top panel. After a sharp increase at early timesdue to the fast redistribution of the electronic densityupon the (slow) skyrmion motion, the pumped currentreaches a maximum and then decreases towards a steadyvalue. The visible small ripples in the stationary currentcome from the fact that the skyrmion’s shape changesslightly during motion because of the lattice discretiza-tion. The different magnitude recorded at different cross-section reflects the progressive onset of the steady regimefor electronic pumping. The inset of Fig. 2 shows thesame calculation for a much slower skyrmion velocity,v = 0.05a/t0. Remarkably, the onset of steady electronicpumping takes much longer to stabilize (∼1800t0 com-pared to ∼400t0 in the main panel), while the magnitudeof the pumped current is smaller (∼ 0.55×10−2e/t0 com-pared to ∼ 1.4× 10−2e/t0).

For the sake of completeness, we also computed thecurrent pumped by a 1D-DW, depicted by the flat linein Fig. 2. In 1D-DW, the current pumped by a movingtexture is directly proportional to the emergent electricfield, Esem. In the steady motion regime, ∂tm = −v∂xm,such that Esem = −v(s~/2e)[m · (∂xm× ∂ym)]y. Hence,because Esem‖y, there is no spin-motive force along the

axis of the waveguide, and the pumped current van-ishes, consistently with the experimental observations[26, 27]. In contrast, a skyrmion is a 2D object suchthat the pumped current arises from the cooperation be-tween the spin-motive force (∼ Esem) and the topologi-cal Hall effect (∼ Bs

em). Indeed, in the adiabatic limitthe semiclassical spin-dependent pumped current readsIs = −

∫dSσsHEsem×Bs

em [21], where S is the waveguidearea and σsH is the ordinary Hall conductivity for spin s.As a result, the total charge current is

I = −v(~/2e)2∫dS(σ↑H + σ↓H)[m · (∂xm× ∂ym)]2. (6)

Hence, the pumped current is proportional to theskyrmion velocity and does not vanish because of thecooperation between spin-motive force and topologicalHall effect, a unique feature of topologically non-trivialmagnetic textures.

Expression (6) only applies in the adiabatic and semi-classical limit (large number of modes). To provide amore accurate estimate of the current pumped by theskyrmion, we follow a scattering matrix approach [31].On the basis of the Redheffer product for combining scat-tering matrices [32], we express the ”frozen” scatteringS matrix as a function of the position of the skyrmion.After some algebra [33], we find S = QS0Q with the ele-ments of the diagonal matrix Q being Qαα = exp (ikαvt)if α ≤ M (rightward modes) and Qαα = exp (−ikαvt)if α > M (leftward modes). Here, kα is the momen-tum vector of mode α and S0 is the initial scatteringmatrix. With this, we get Sαβ = S0

αβ exp (±ikαβvt)with kαβ = kα ± kβ . The ± sign depends on whetherthe modes α and β are from the same lead or not[33]. At long times, when the stationary regime estab-lishes, we find the out of equilibrium Fermi distributionfoutα =

∑β |S0

αβ |2f0(E + ~kαβv), f0 being the distribu-tion at equilibrium. At this stage, the stationary cur-rent can be expressed in an energy integral form [31]and then estimated numerically. In order to obtain ananalytical expression, we restrict ourselves to the caseof slow skyrmion although our algorithm goes beyondthis restriction. Indeed, the skyrmion velocity (∼ 10-100m/s) remains much smaller than the electronic velocity(∼ 105 m/s). Therefore, if the electrons flow throughthe skyrmion before the texture moves substantially, onecan consider the scattering as adiabatic and thus the useof the frozen S matrix is justified [36]. This conditionis fulfilled when ~kαβv � EF ∀{α, β}, or equivalently2~kF v � EF , where kF and EF are the Fermi wavenum-ber and energy, respectively.

Within this adiabatic behavior, only electrons aroundthe Fermi energy are pertinent in the expression of thestationary current and all the contributions from theFermi sea cancel. At this stage, the expression of the cur-rent boils down to the calculation of the emissivity intothe contact m defined as −e

2πv

∑β

∑α∈m ={S∗αβ∂tSαβ}

Page 4: Cooperative Charge Pumping and Enhanced Skyrmion MobilityIn this Letter, we uncover the interplay between spin currents and skyrmion dynamics by directly solving the time-dependent

4

FIG. 3. (Color online) Stationary current pumped by oneskyrmion as a function of its radius as computed numerically(blue symbols) and analytically (green solid line). The greyregion is the range of the fluctuation due to lattice effects (i.e.,the ripples in Fig. 2). The velocity is v = 0.07a/t0 and theother parameters are the same as in Fig. 1.

[34, 35]. Within this approximation, the charge currentreads,

I = − eπvkR, (7)

k is the barycenter of kα with coefficients∑β∈m |rαβ |2

and R is the total reflection of the system. This ex-pression reflects the rowing effect of the skyrmion. In-deed, the pumped current can be enhanced by increas-ing the velocity of the skyrmion (see Fig. 2), taking alarger Fermi energy (faster electrons) or considering amore reflective skyrmion. For instance, let us considera skyrmion moving with a velocity v = 0.05a/t0 in awaveguide of width W = 51a (inset of Fig. 2). As-suming a = 1 nm, t0 = 2.5 ps, we obtained v = 20m/s, k = 0.2 nm−1 and R = 1.8, and Eq. (7) gives acharge current I = 0.366 nA, which is in good agree-ment with the value computed numerically in the insetof Fig. 2, I = 0.352 nA. If we consider a thickness ofd = 0.5 nm for a magnetic thin film, we get a currentdensity jp = 1.43× 107 A/m2, which is accessible exper-imentally. This value can be considerably increased byincreasing the number of conducting modes and the re-flection coefficient. Figure 3 displays the pumped currentcomputed numerically (blue symbols) and analytically(green solid line) as a function of the skyrmion radius,showing a very good agreement between the two meth-ods. The electronic pumping reaches a maximum aroundR ∼ 12 a, which corresponds to the smallest wavelengthof the flowing electrons, estimated around λ ≈ 11 a [33].When the radius becomes larger than this wavelength,the reflection of the electrons against the skyrmion de-creases and the pumping efficiency is subsequently re-duced.

Cooperative pumping and enhanced motion - Theelectronic pumping can be enhanced by increasing the

FIG. 4. (Color online) Pumped current as a function of thenumber of skyrmions. The symbols • represent the currentcomputed numerically and the orange line is the fit with theequation for N skyrmions given in the main text. The insetdisplay the reflection coefficient as a function of the numberof skyrmions. The parameters are W = 31a. ∆ = 0.1γ,v = 0.15a/t0 and R = 7.5a, EF = −3.5γ.

number of skyrmions in the system and thereby the re-flection of flowing electrons. This effect is illustrated inFig. 4, where the pumped charge current is reportedas a function of the number of skyrmions present in thenanowire. The inset shows the analog behavior for the re-flection coefficient. This cooperative pumping is expectedto saturate at large number of skyrmions due to thebound of R. For instance, if we consider EF = −0.97γ,∆ = 0.98γ and 10 skyrmions, we obtain a current den-sity 50 times larger. A crude estimate of the cooperativepumping can be obtained in the frame of a chain of one-dimensional scatterers. Assuming that each skyrmion be-haves like a one-dimensional scatterer with an effectivereflection coefficient R, a chain of N skyrmions producesa total pumped current of IN = − e

πvkM

1+(M−R)/(NR). In

the limit of N → +∞, I∞ → − eπvkM . Figure 4 shows

a very good test of this formula and describes well thetotal current as a function of the number of skyrmions.

In a skyrmion racetrack [3], the current pumped col-lectively by the train of skyrmions exerts a spin transfertorque on each individual skyrmion, enhancing the effec-tive force exerted on each skyrmion. Consider a chainof skyrmions driven by either spin transfer or spin-orbittorque. Its steady state velocity reads v = χj0 + ηjp,where j0(p) is the injected (pumped) current density, χ isthe (either spin-orbit or spin transfer) torque efficiency,and η is the spin transfer torque efficiency. Since thepumped spin current itself depends on the velocity, jp =ξv, one obtains the renormalized velocity of the skyrmiontrain, v = χj0/(1 − ηξ). In other words, the electronicpumping enhances the collective skyrmion velocity. Thetypical skyrmion mobility is 100 m/s for a current den-sity of 1012 A/m2 [10], which gives η = 10−10 m3·s/A.Following the estimation given above, the pumping effi-ciency is about ξ = jp/v = −ekM/(πWd) ≈ −ek2F /π2.Here we assumed a large number of modes such that

Page 5: Cooperative Charge Pumping and Enhanced Skyrmion MobilityIn this Letter, we uncover the interplay between spin currents and skyrmion dynamics by directly solving the time-dependent

5

M/W ≈ kF /π and k ≈ kF . Taking kF = 10 nm−1

and a ferromagnetic thickness d = 0.5 nm, we obtainξ = 3 × 109 A/(m3·s). This provides a renormalizationof 1 − ηξ ≈ 0.68, which indicates that the mobility ofthe train of skyrmion can be substantially enhanced toalmost 50%.

Conclusion - We showed that under steady motion,magnetic skyrmions are able to pump a charge currentdue to the cooperation of the spin-motive force and topo-logical Hall effect. We propose that the cooperativeelectronic pumping arising from a train of skyrmions ina racetrack enhances the collective skyrmion mobility.Notice that each moving skyrmion also pumps a non-equilibrium spin density locally that enhances the mag-netic damping but does not affect our conclusions [21].This prediction calls for experimental verification and hasthe potential to foster the development of skyrmion race-tracks [2, 3].

A. A. and A. M. acknowledge financial support fromthe King Abdullah University of Science and Technol-ogy (KAUST). We acknowledge computing time on thesupercomputers SHAHEEN at KAUST SupercomputingCentre and the team assistance. A. A. thanks A. Sali-math, P. B. Ndiaye, S. Ghosh and C. A. Akosa for usefuldiscussions.

[1] D.A. Allwood, G. Xiong, C.C. Faulkner, D. Atkinson, .Petit, and R.P. Cowburn, Science 3009, 1688 (2005).

[2] S.S.P. Parkin, M. Hayashi, L. Thomas, Science 320, 190(2008).

[3] A. Fert, V. Cros and J. Sampaio. Nat. Nanotechnol. 8,152-156 (2013).

[4] T. H. R. Skyrme, A unified field theory of mesons andbaryons. Nucl. Phys. 31, 556-569 (1962).

[5] A. Fert, N. Reyren, and V. Cros, Nat. Rev. Mater. 2,17031 (2017).

[6] S. Muhlbauer, B. Binz, F. Jonietz, C. Pfleiderer, A.

Rosch, A. Neubauer, R. Georgii, P. Boni, Science 323,915 (2009).

[7] X.Z. Yu et al., Nature 465, 901 (2010).[8] S. Heinze, et al. Nat. Phys. 7, 713-718 (2011).[9] W. Jiang et al., Science 349, 283 (2015).

[10] S. Woo, et al. Nat. Mater. 15, 501-506 (2016).[11] O. Boulle, et al. Nat. Nanotechnol. 11, 449-454 (2016).[12] C. Moreau-Luchaire, et al. Nat. Nanotechnol. 11, 444-

448 (2016).[13] N. Nagaosa and Y. Tokura, Nat. Nanotechnol. 8, 899

(2013).[14] J. Iwasaki, M. Mochizuki, and N. Nagaosa, Nat. Nan-

otechnol. 8, 742 (2013).[15] F. Jonietz et al., Science 330, 1648 (2010).[16] Y. Taguchi, Y. Oohara, H. Yoshizawa, N. Nagaosa, and

Y. Tokura, Science 291, 2573 (2001).[17] S. E. Barnes, S. Maekawa, Physical Review Letters 98,

246601 (2007).[18] G. Tatara, H. Kohno, and J. Shibata. Phys. Rep. 468,

213 (2008).

[19] P. B. Ndiaye, C. A. Akosa, and A. Manchon, Phys. Rev.B 95, 064426 (2017).

[20] A. Bisig et al., Phys.Rev. Lett. 117, 277203 (2016)[21] C. A. Akosa, P. B. Ndiaye, and A. Manchon, Phys. Rev.

B 95, 054434 (2017).[22] M. Stone, Phys. Rev. B 53,16573 (1996).[23] W. Jiang et al., Nat. Phys. 13, 162 (2017).[24] K. Litzius et al., Nat. Phys. 13, 170 (2017).[25] W. Legrand et al., Nano Letters 17, 2703 (2017).[26] S. Yang et al., Phys. Rev. Lett. 102 067201 (2009).[27] M. Hayashi, Phys. Rev. Lett. 108, 147202 (2012).[28] J. Weston and X. Waintal. Phys. Rev. B 93, 134506

(2016).[29] B. Gaury, J. Weston, M. Santin, M. Houzet, C. Groth,

X. Waintal . Phys. Rep. 534, 1 (2014).[30] J. Weston and X. Waintal. J. Comput. Electron. 15, 1148

(2016).[31] M. Moskalets and M. Buttiker.Phys. Rev. B 66, 035306.[32] R. Redheffer. J. Math. Phys., 41 (1962).[33] Supplementary Materials.[34] M. Buttiker, H. Thomas, and A. Pretre, Z. Phys. B 94,

133 (1994).[35] P. W. Brouwer. Phys. Rev. B 58, R10135(R).[36] O. E. Wohlman, A. Aharony and Y. Levinson. Phys. Rev.

B 65, 195411 (2002).