Inertia, diffusion and dynamics of a driven skyrmion

Inertia, diffusion and dynamics of a driven skyrmion

Christoph Schütte Institut für Theoretische Physik, Universität zu Köln, D-50937 Cologne, Germany    Junichi Iwasaki Department of Applied Physics, University of Tokyo, 7-3-1, Hongo, Bunkyo-ku, Tokyo 113-8656, Japan    Achim Rosch Institut für Theoretische Physik, Universität zu Köln, D-50937 Cologne, Germany    Naoto Nagaosa nagaosa@riken.jp Department of Applied Physics, University of Tokyo, 7-3-1, Hongo, Bunkyo-ku, Tokyo 113-8656, Japan RIKEN Center for Emergent Matter Science (CEMS), Wako, Saitama 351-0198, Japan
July 14, 2019
Abstract

Skyrmions recently discovered in chiral magnets are a promising candidate for magnetic storage devices because of their topological stability, small size (nm), and ultra-low threshold current density (A/m) to drive their motion. However, the time-dependent dynamics has hitherto been largely unexplored. Here we show, by combining the numerical solution of the Landau-Lifshitz-Gilbert equation and the analysis of a generalized Thiele’s equation, that inertial effects are almost completely absent in skyrmion dynamics driven by a time-dependent current. In contrast, the response to time-dependent magnetic forces and thermal fluctuations depends strongly on frequency and is described by a large effective mass and a (anti-) damping depending on the acceleration of the skyrmion. Thermal diffusion is strongly suppressed by the cyclotron motion and is proportional to the Gilbert damping coefficient . This indicates that the skyrmion position is stable, and its motion responds to the time-dependent current without delay or retardation even if it is fast. These findings demonstrate the advantages of skyrmions as information carriers.

pacs:
73.43.Cd,72.25.-b,72.80.-r

I Introduction

Mass is a fundamental quantity of a particle determining its mechanical inertia and therefore the speed of response to external forces. Furthermore, it controls the strength of quantum and thermal fluctuations. For a fast response one usually needs small masses and small friction coefficients which in turn lead to large fluctuations and a rapid diffusion. Therefore, usually small fluctuations and a quick reaction to external forces are not concomitant. However a “particle” is not a trivial object in modern physics, it can be a complex of energy and momentum, embedded in a fluctuating environment. Therefore, its dynamics can be different from that of a Newtonian particle. This is the case in magnets, where such a “particle” can be formed by a magnetic texture Hubert98magnetic (); Malozemoff79magnetic (). A skyrmion Skyrme61nonlinear (); Skyrme62unified () is a representative example: a swirling spin texture characterized by a topological index counting the number of times a sphere is wrapped in spin space. This topological index remains unchanged provided spin configurations vary slowly, i.e., discontinuous spin configurations are forbidden on an atomic scale due to high energy costs. Therefore, the skyrmion is topologically protected and has a long lifetime, in sharp contrast to e.g. spin wave excitations which can rapidly decay. Skyrmions have attracted recent intensive interest because of their nano-metric size and high mobility Bogdanov89thermo (); Muhlbauer09skyrmion (); Yu10real (); Heinze11spontaneous (); Seki12observation (); Fert13skyrmion (); Lin13driven (); Lin13particle (); Iwasaki13constricted (); Iwasaki2014colossal (). Especially, the current densities needed to drive their motion (A/m) are ultra small compared to those used to manipulate domain walls in ferromagnets (A/m) Jonietz10spin (); Schulz12emergent (); Yu12skyrmion (); Parkin08magnetic (); Yamanouchi04current ().

The motion of the skyrmion in a two dimensional film can be described by a modified version of Newton’s equation. For sufficiently slowly varying and not too strong forces, a symmetry analysis suggests the following form of the equations of motion,

(1)

Here we assumed translational and rotational invariance of the linearized equations of motion. The ‘gyrocoupling’ is an effective magnetic field oriented perpendicular to the plane, is the (dimensionless) Gilbert damping of a single spin, describes the friction of the skyrmion, its mass and its centre coordinate. parametrizes a peculiar type of damping proportional to the acceleration of the particle. We name this term ‘gyrodamping’, since it describes the damping of a particle on a cyclotron orbit (an orbit with ), which can be stronger ( parallel to ) or weaker (antiparallel to ) than that for linear motion. Our main goal will be to describe the influence of forces on the skyrmion arising from electric currents (), magnetic field gradients ) and thermal fluctuations ).

By analyzing the motion of a rigid magnetic structure for static forces, one can obtain analytic formulas for and using the approach of Thiele Thiele73steady (); Everschor11current (); Schulz12emergent (); Everschor12rotating (); Iwasaki13universal (). In Ref. [Makhfudz12inertia, ], an approximate value for the mass of a skyrmion was obtained by simulating the motion of a skyrmion in a nanodisc and by estimating contributions to the mass from internal excitations of the skyrmion.

Figure 1: When a skyrmion is driven by a time dependent external force, it becomes distorted and the spins precess resulting in a delayed response and a large effective mass. In contrast, when the skyrmion motion is driven by an electric current, the skyrmion approximately flows with the current with little distortion and precession. Therefore skyrmions respond quickly to rapid changes of the electric current.

For rapidly changing forces, needed for the manipulation of skyrmions in spintronic devices, Eq. (1) is however not sufficient. A generalized version of Eq. (1) valid for weak but also arbitrarily time-dependent forces can be written as

Here is the Fourier transform of the velocity of the skyrmion, is the (spin-) drift velocity of the conduction electrons, directly proportional to the current, describes a magnetic field gradient in frequency space. The role of the random thermal forces, , is special as their dynamics is directly linked via the fluctuation-dissipation theorem to the left-hand side of the equation, see below. The matrix describes the dynamics of the skyrmion; its small- expansion defines the terms written on the left-hand side of Eq. (1). One can expect strongly frequency-dependent dynamics for the skyrmion because the external forces in combination with the motion of the skyrmion can induce a precession of the spin and also excite spinwaves in the surrounding ferromagnet, see Fig. 1. We will, however, show that the frequency dependence of the right-hand side of the Eq. (2) is at least as important: not only the motion of the skyrmion but also the external forces excite internal modes. Depending on the frequency range, there is an effective screening or antiscreening of the forces described by the matrices and . Especially for the current-driven motion, there will be for all frequencies an almost exact cancellation of terms from and . As a result the skyrmion will follow almost instantaneously any change of the current despite its large mass.

In this paper, we study the dynamics of a driven skyrmion by solving numerically the stochastic Landau-Lifshitz-Gilbert (LLG) equation. Our strategy will be to determine the parameters of Eq. (I) such that this equation reproduces the results of the LLG equation. Section II introduces the model and outlines the numerical implementation. Three driving mechanisms are considered: section III studies the diffusive motion of the skyrmion due to thermal noise, section IV the skyrmion motion due to time-dependent magnetic field gradient and section V the current-driven dynamics. We conclude with a summary and discussion of the results in Sec. VI.

Ii Model

Our study is based on a numerical analysis of the stochastic Landau-Lifshitz-Gilbert (sLLG) equations Garcia98langevin () defined by

(3)

Here is the gyromagnetic moment and the Gilbert damping; is an effective magnetic field created by the surrounding magnetic moments and a fluctuating, stochastic field creating random torques on the magnetic moments to model the effects of thermal fluctuations, see below.

The Hamiltonian is given by

(4)

We use , , , for the strength of the Dzyaloshinskii-Moriya interaction and for all plots giving rise to a skyrmion with a radius of about lattice sites, see Appendix A. For this parameter set, the ground state is ferromagnetic, thus the single skyrmion is a topologically protected, metastable excitation. Typically we simulate spins for the analysis of diffusive and current driven motion and spins for the force-driven motion. For these parameters lattice effects are negligible, see appendix B. Typical microscopic parameters used, are (this yields ) which we use to estimate typical time scales for the skyrmion motion.

Following Ref. Garcia98langevin, , we assume that the field is generated from a Gaussian stochastic process with the following statistical properties

(5)

where and are cartesian components and denotes an average taken over different realizations of the fluctuating field. The Gaussian property of the process stems from the interaction of with a large number of microscopic degrees of freedom (central limit theorem) which are also responsible for the damping described by , reflecting the fluctuation-dissipation theorem. The delta-correlation in time and space in Eq. (II) expresses that the autocorrelation time and length of is much shorter than the response time and length scale of the magnetic system.

For a numerical implementation of Eq. (3) we follow Ref. Garcia98langevin, and use Heun’s scheme for the numerical integration which converges quadratically to the solution of the general system of stochastic differential equations (when interpreted in terms of the Stratonovich calculus).

For static driving forces, one can calculate the drift velocity following Thiele Thiele73steady (). Starting from the Landau-Lifshitz Gilbert equations, Eq. (3), we project onto the translational mode by multiplying Eq. (3) with and integrating over space Everschor11current (); Everschor12rotating (); He2006current ().

(6)

where is the direction of the magnetization, the local spin density, the (spin-) drift velocity of the conduction electrons proportional to the electric current, and is the change of the magnetization induced by a skyrmion in a ferromagnetic background. The ’gyrocoupling vector’ with is given by the winding number of the skyrmion, independent of microscopic details.

Iii Thermal diffusion

Random forces arising from thermal fluctuations play a decisive role in controlling the diffusion of particles and therefore also the trajectories of a skyrmion. To obtain and corresponding correlation functions we used numerical simulations based on the stochastic Landau-Lifshitz-Gilbert equation Garcia98langevin (). These micromagnetic equations describe the dynamics of coupled spins including the effects of damping and thermal fluctuations. Initially, a skyrmion spin-texture is embedded in a ferromagnetic background. By monitoring the change of the magnetization, we track the center of the skyrmion , see appendix A for details.

Our goal is to use this data to determine the matrix and the randomly fluctuating thermal forces, , which together fix the equation of motion, Eq. (I), in the presence of thermal fluctuations (). One might worry that this problem does not have a unique solution as both the left-hand and the right-hand side of Eq. (I) are not known a priori. Here one can, however, make use of the fact that Kubo’s fluctuation-dissipation theorem Kubo66fluctuation () constraints the thermal forces on the skyrmion described by in Eq. (I) by linking them directly to the dissipative contributions of . On average , but its autocorrelation is proportional to the temperature and friction coefficients. In general it is given by

(7)

For small one obtains while off-diagonal correlations arise from the gyrodamping . Using Eq. (7) and demanding furthermore that the solution of Eq. (I) reproduces the correlation function (or, equivalently, ) obtained from the micromagnetic simulations, leads to the condition Kubo66fluctuation ()

(8)

We therefore determine first in the presence of thermal fluctuations () from simulations of the stochastic LLG equation (3) the correlation functions of the velocities and use those to determine using Eq. (8). After a simple matrix inversion, this fixes the left-hand side of the equation of motion, Eq. (I), and therefore contains all information on the (frequency-dependent) effective mass, gyrocoupling, damping and gyrodamping of the skyrmion. Furthermore, the corresponding spectrum of thermal fluctuations is given by Eq. (7).

Figure 2: Time dependence of the correlation function for and different values of the Gilbert damping ( is the frequency for cyclotron motion).

Fig. 2 shows . As expected, the motion of the skyrmion is diffusive: the mean squared displacement grows for long times linearly in time , where is the diffusion constant. Usually the diffusion constant of a particle grows when the friction is lowered Kubo66fluctuation (). For the skyrmion the situation is opposite: the diffusion constant becomes small for the small friction, i.e., small Gilbert damping . This surprising observation has its origin in the gyrocoupling : in the absence of friction the skyrmion would be localized on a cyclotron orbit. From Eq. (1), we obtain

(9)

The diffusion is strongly suppressed by . As in most materials is much smaller than unity while , the skyrmion motion is characterized both by a small diffusion constant and a small friction. Such a suppressed dynamics has also been shown to be important for the dynamics of magnetic vortices clarke (). For typical parameters relevant for materials like MnSi we estimate that it takes to for a skyrmion to diffusive over an average length of one skyrmion diameter.

Figure 3: Dissipative tensor , mass , gyrocoupling and gyrodamping as functions of the frequency for the diffusive motion at (solid lines). They differ strongly from the “apparent” dynamical coefficients (see text) obtained for the force driven (red dashed line) and current driven motion (green dot-dashed line). We use , . The error bars reflect estimates of systematic errors arising mainly from discretization effects, see appendix B.

To analyze the dynamics on shorter time scales we show in Fig. 3 four real functions parametrizing : a frequency-dependent mass , gyrocoupling , gyrodamping and dissipation strength with

Figure 4: Dissipative strength , mass , gyrocoupling and gyrodamping as functions of the Gilbert damping for different temperatures .

For one obtains the parameters of Eq. (1). All parameters depend only weakly on temperature, and are approximately independent of , while the friction coefficients and are linear in , see Fig. 4. In the limit , takes the value , fixed by the topology of the skyrmion Thiele73steady (); Jonietz10spin ().

Both the gyrodamping and and the effective mass have huge numerical values. A simple scaling analysis of the Landau-Lifshitz-Gilbert equation reveals that both the gyrocoupling and are independent of the size of the skyrmion, while and are proportional to the area of the skyrmion, and frequencies scale with the inverse area, see appendix B. For the chosen parameters (the field dependence is discussed in the appendix B), we find and , where is the mass of a single flipped spin in a ferromagnet ( in our units) and we have estimated the number of flipped spins, , from the total magnetization of the skyrmion relative to the ferromagnetic background. As expected the mass of skyrmions grows with the area (consistent with an estimatepetrova () for obtained from the magnon spectrum of skyrmion crystals), the observation that the damping rate is independent of the size of skyrmions is counter-intuitive. The reason is that larger skyrmions have smoother magnetic configurations, which give rise to less damping. For realistic system parameters (which yields a paramagnetic transition temperature K, but there are also materials, i.e. FeGe, where the skyrmion lattice phase is stabilised near room-temperature Yu12skyrmion ()) and and a skyrmion radius of one finds a typical mass scale of .

The sign of the gyrodamping is opposite to that of the gyrocoupling . This implies that describes not damping but rather antidamping: there is less friction for cyclotron motion of the skyrmion than for the linear motion. The numerical value for the antidamping turns out to be so large that . This has the profound consequence that the simplified equation of motion shown in Eq. (1) cannot be used: it would wrongly predict that some oscillations of the skyrmion are not damped, but grow exponentially in time due to the strong antidamping. This is, however, a pure artifact of ignoring the frequency dependence of , and such oscillations do not grow.

Fig. 3 shows that the dynamics of the skyrmion has a strong frequency dependence. We identify the origin of this frequency dependence with a coupling of the skyrmion coordinate to pairs of magnon excitations as discussed in Ref. Schuette14scattering, . Magnon emission sets in for where is the precession frequency of spins in the ferromagnet (in the presence of a bound state with frequency , the onset frequency is , Ref. Schuette14scattering, ). This new damping channel is most efficient when the emitted spin waves have a wavelength of the order of the skyrmion radius.

Figure 5: Effective damping, for , and .

As a test for this mechanism, we have checked that only this high-frequency damping survives for . In Fig. 5 we show the frequency dependent damping for various bare damping coefficients . For small it is proportional to as predicted by the Thiele equation. For , however, an extra dampling mechanism sets in: the skyrmion motion can be damped by the emission of pairs of spin waves. This mechanism is approximately independent of and survives in the limit. This leads necessarily to a pronounced frequency dependence of the damping and therefore to the effective mass which is related by the Kramers-Kronig relation to . Note also that the large independent mass is directly related to the independent damping mechanism for large . Also the frequency dependence of and can be traced back to the same mechanism as these quantities can be computed from and using Kramers-Kronig relations. For large frequencies, the effective mass practically vanishes and the ‘gyrocoupling’ drops by a factor of a half.

Iv Force-driven motion

Next, we study the effects of an oscillating magnetic field gradient in the absence of thermal fluctuations. As the skyrmion has a large magnetic moment relative to the ferromagnetic background, the field gradient leads to a force acting on the skyrmion. In the static limit, the force is exactly given by

(10)
Figure 6: Dynamical coupling coefficients for the force driven motion (). In the static limit everything but the real part of the diagonal vanishes. however approaches the total magnetization as expected. The error bars reflect estimates of systematic errors, see appendix B.

Using determined above, we can calculate how the effective force (see Eq. I) depends on frequency. Fig. 6 shows that for one obtains the expected result , while a strong frequency dependence sets in above the magnon gap, for . This is the precession frequency of spins in the external magnetic field.

In general, both the screening of forces (parametrized by ) and the internal dynamics (described by ) determines the response of skyrmions, . Therefore it is in general not possible to extract, e.g., the mass of the skyrmion as described by from just a measurement of the response to field gradients. It is, however, instructive to ask what “apparent” mass one obtains, when the frequency dependence of is ignored. We therefore define the “apparent” dynamics by . The matrix elements of are shown in Fig. 3 as dashed lines. The apparent mass for gradient-driven motion, for example, turns out to be more than a factor of three smaller then the value obtained from the diffusive motion clearly showing the importance of screening effects on external forces. The situation is even more dramatic when skyrmions are driven by electric currents.

V Current-driven motion

Currents affect the motion of spins both via adiabatic and non-adiabatic spin torquesTatara08microscopic (). Therefore one obtains two types of forces on the spin texture even in the static limit Thiele73steady (); Everschor11current (); Schulz12emergent (); Everschor12rotating (); Iwasaki13universal ().

The effect of a time-dependent, spin-polarized current on the magnetic texture can be modelled by supplementing the right hand side of eq. (3) with a spin torque term ,

(11)

The first term is called the spin-transfer-torque term and is derived under the assumption of adiabaticity: the conduction-electrons adjust their spin orientation as they traverse the magnetic sample such that it points parallel to the local magnetic moment owing to and . This assumptions is justified as the skyrmions are rather large smooth objects (due to the weakness of spin-orbit coupling). The second so called -term describes the dissipative coupling between conduction-electrons and magnetic moments due to non-adiabatic effects. Both and are small dimensionless constants in typical materials. From the Thiele approach one obtains the force

(12)

For a Galilei-invariant system one obtains . In this special limit, one can easily show that an exact solution of the LLG equations in the presence of a time-dependent current, described by is given by provided, is a static solution of the LLG equation for . This implies that for , the skyrmion motion exactly follows the external current, . Using Eq. (I), this implies that for one has . Defining the apparent dynamics, as above, one obtains a frequency independent : the apparent effective mass and gyrodamping are exactly zero in this limit and the skyrmion follows the current without any retardation.

Figure 7: Dynamical coupling coefficients (symbols) for the current-driven motion (, , , , ). These curves follow almost the corresponding matrix elements of shown as dashed lines. A deviation of symbols and dashed line is only sizable for .

For , the LLG equations predict a finite apparent mass. Numerically, we find only very small apparent masses, , see dot-dashed line in upper-right panel of Fig. 3, where the case , is shown. This is anticipated from the analysis of the case: As the mass vanishes for , it will be small as long as both and are small. Indeed even for this relation holds approximately as shown in Fig. 7. The only sizable deviation is observed for for which the Thiele equation predicts while as observed numerically.

Figure 8: Mass and gyrodamping as functions of the driving frequency for the current-driven motion. Note that both and vanish for .

A better way to quantify that the skyrmion follows the current even for almost instantaneously is to calculate the apparent mass and gyrodamping for current driven motion, where only results for and have been shown. As these quantities vanish for , one can expect that they are proportional to at least for small . This is indeed approximately valid at least for small frequencies as can be seen from Fig. 8. Interestingly, one can even obtain negative values for (without violating causality). Most importantly, despite the rather large values for and used in our analysis, the apparent effective mass and gyrodamping remain small compared to the large values obtained for force-driven motion or the intrinsic dynamics. This shows that retardation effects remain tiny when skyrmions are controlled by currents.

Vi Conclusions

In conclusion, we have shown that skyrmions in chiral magnets are characterised by a number of unique dynamical properties which are not easily found in other systems. First, their damping is small despite the fact that skyrmions are large composite objects. Second, despite the small damping, the diffusion constant remains small. Third, despite a huge inertial mass, skyrmions react almost instantaneously to external currents. The combination of these three features can become the basis for a very precise control of skyrmions by time-dependent currents.

Our analysis of the skyrmion motion is based on a two-dimensional model where only a single magnetic layer was considered. All qualitative results can, however, easily be generalized to a film with layers. In this case, all terms in Eq. (1) get approximately multiplied by a factor with the exception of the last term, the random force, which is enhanced only by a factor . As a consequence, the diffusive motion is further suppressed by a factor while the current- and force-driven motion are approximately unaffected.

An unexpected feature of the skyrmion motion is the antidamping arising from the gyrodamping. The presence of antidamping is closely related to another important property of the system: both the dynamics of the skyrmion and the effective forces acting on the skyrmion are strongly frequency dependent.

In general, in any device based on skyrmions a combination of effects will play a role. Thermal fluctuations are always present in room-temperature devices, the shape of the device will exert forces Iwasaki13constricted (); Iwasaki2014colossal () and, finally, we have identified the current as the ideal driving mechanism. In the linear regime, the corresponding forces are additive. The study of non-linear effects and the interaction of several skyrmions will be important for the design of logical elements based on skyrmions and this is left for future works. As in our study, we expect that dynamical screening will be important in this regime.

Acknowledgements.
The authors are greatful for insightful discussions with K. Everschor and Markus Garst. Part of this work was funded through the Institutional Strategy of the University of Cologne within the German Excellence Initiative” and the BCGS. C.S. thanks the University of Tokyo for hospitality during his research internship where part of this work has been performed. N.N. was supported by Grant-in-Aids for Scientific Research (No. 24224009) from the Ministry of Education, Culture, Sports, Science and Technology (MEXT) of Japan, and by the Strategic International Cooperative Program (Joint Research Type) from Japan Science and Technology Agency. J.I. is supported by Grant-in-Aids for JSPS Fellows (No. 2610547).

Appendix A Definition of the Skyrmion’s centre coordinate

In order to calculate the Green’s function, Eq. (3), one needs to calculate the velocity-velocity correlation function. Therefore it is necessary to track the skyrmion position throughout the simulation. Mostly two methods have been used so far for thisMakhfudz12inertia (): (i) tracking the centre of the topological charge and (ii) tracking the core of the Skyrmion (reversal of magnetization).

Figure 9: Skyrmion density based on the normalized -component of the magnetization.

The topological charge density

(13)

integrates to the number of Skyrmions in the system. Therefore for our case of a single Skyrmion in the ferromagnetic background this quantity is normalized to . The center of topological charge can therefore be defined as

(14)

For the case of finite temperature this method can, however, not be used directly. Thermal fluctuations in the ferromagnetic background far away from the skyrmion lead to a large noise to this quantity which diverges in the thermodynamic limit. A similar problem arises when tracking the center using the magnetization of the skyrmion.

One therefore needs a method which focuses only on the region close to the skyrmion center. To locate the skyrmion, we use the -component of the magnetization but take into account only points where (the magnetization of the ferromagnetic background at is ). We therefore use

(15)

where is the theta function. A first estimate, , for the radius is obtained from

(16)

by integrating over the full sample volume . is noisy due to the problems mentioned above but for the system sizes simulated one nevertheless obtains a good first estimate for the skyrmion position. This estimate is refined by using in a second step for the integration area only where is choosen to be larger than the radius of the skyrmion core (we use , where is the number of spins with ). Thus we obtain a reliable estimate, , not affected by spin fluctuations far away from the skyrmion. From the resulting , one can obtain the velocity-velocity correlation function .

Appendix B Scaling invariance

To obtain analytic insight into the question of how parameters depend on system size and to check the numerics for lattice artifacts it is useful to perform a scaling analysis of the sLLG equations and the effective equations of motion for the skyrmion.

We investigate a scaling transformation, where the radius of the skyrmion is enlarged by a factor , .

For the scaling analysis, we use the continuum limit of Eq. (4) (setting )

The three terms scale with , and , respectively. To obtain a larger skyrmion, we therefore have to rescale and . This implies that the term in the sLLG equation scales with and therefore also the time axis has to be rescaled, , implying that all time scales are a factor of longer and all frequencies a factor smaller. Similiarly, the driving current, i.e. is reduced by a factor while the temperature remains unscaled. This implies that when is a solution for a given value of , and and the corresponding velocity-correlation function of the skyrmion, then is a solution for , , with correlation function .

Accordingly, the limit and therefore the gyrocoupling , the friction constant and the diffusion constant of the skyrmion are independent of , consistent with the analytical formulas eq. (6). In contrast, the mass of the skyrmion, , and the gyrodamping scale with . They are therefore proportional to the number of spins constituting the skyrmion consistent with our numerical findings.

Figure 10: Field dependence of the dissipative tensor , the mass , the gyrocoupling and the gyrodamping for , . The main effect is that both and shrink when the size of the skyrmion shrinks with increasing .

When one does, however, change the external magnetic field for fixed strength of the DM interaction, the internal structure of the skyrmion and therefore also change quantitatively in a way not predictable by scaling. In Fig. 10 we therefore show the -dependence of , , and . For increasing the size of the skyrmion shrinks. From our previous analysis, it is therefore not surprising that both the effective mass and the gyrodamping shrink substantially while and are less affected . Quantitatively, this change of and is however not proportional to the number of spins constituting the skyrmion.

We have tested numerically the scaling properties for and find that all features are quantitatively reproduced. Small variations on the level of a few percent do, however, occur reflecting the typical size of features arising from the discretization of the continuum theory. A conservative estimate of such systematic discretization effects for the diffusive motion is given by the error bars in Figs. 3 (all statistical errors are smaller than the thickness of the line). For the field-driven motion (Fig. 3 and Fig. 6) spatial discretization effects lead to a different source of errors. For very small field gradients and high frequencies the displacement of the skyrmion is much smaller than the lattice spacing and the response is affected by a tiny pinning of the skyrmion to the discreet lattice. For larger gradients, however, nonlinear effects set in and for small frequencies the skyrmion starts to approach the edge of the simulated area. In Fig. 3, we therefore used for the force-driven motion for and for . Error bars have been estimated from variations of the numerical values when was varied from to . For the current-driven motion errors are so tiny that they are not shown.

References

  • (1) Hubert, A. & Schäfer, R. Magnetic Domains: The Analysis of Magnetic Microstructures (Springer, Berlin, 1998).
  • (2) Malozemoff, A. P. & Slonczewski, J.C. Magnetic Domain Walls in Bubble Materials (Academic Press, New York, 1979).
  • (3) Skyrme, T. H. R. A Non-Linear Field Theory. Proc. Roy. Soc. London A 260, 127–138 (1961).
  • (4) Skyrme, T. H. R. A unified field theory of mesons and baryons. Nuc. Phys. 31, 556–569 (1962).
  • (5) Bogdanov, A. N. & Yablonskii, D. A. Thermodynamically stable ”vortices” in magnetically ordered crystals. The mixed state of magnets. Sov. Phys. JETP 68, 101–103 (1989).
  • (6) Mühlbauer, S. et al. Skyrmion lattice in a chiral magnet. Science 323, 915–919 (2009).
  • (7) Yu, X. Z. et al. Real-space observation of a two-dimensional skyrmion crystal. Nature 465, 901–904 (2010).
  • (8) Heinze, S. et al. Spontaneous atomic-scale magnetic skyrmion lattice in two dimensions. Nature Phys. 7, 713–718 (2011).
  • (9) Seki, S., Yu, X. Z., Ishiwata, S. & Tokura, Y. Observation of skyrmions in a multiferroic material. Science 336, 198–201 (2012).
  • (10) Fert, A., Cros, V. & Sampaio, J. Skyrmions on the track. Nature Nanotech. 8, 152–156 (2013).
  • (11) Lin, S. -Z., Reichhardt, C., Batista, C. D. & Saxena, A. Driven skyrmions and dynamical transitions in chiral magnets. Phys. Rev. Lett. 110, 207202 (2013).
  • (12) Lin, S. -Z., Reichhardt, C., Batista, C. D. & Saxena, A. Particle model for skyrmions in metallic chiral magnets: Dynamics, pinning, and creep. Phys. Rev. B 87, 214419 (2013).
  • (13) Iwasaki, J., Mochizuki, M. & Nagaosa, N. Current-induced skyrmion dynamics in constricted geometries. Nature Nanotech. 8, 742–747 (2013).
  • (14) Iwasaki, J., Koshibae, W. & Nagaosa, N. Colossal spin transfer torque effect on skyrmion along the edge. Nano letters 14 (8), 4432–4437 (2014).
  • (15) Jonietz, F. et al. Spin transfer torques in MnSi at ultralow current densities. Science 330, 1648–1651 (2010).
  • (16) Yu, X. Z. et al. Skyrmion flow near room temperature in an ultralow current density. Nat. Commun. 3, 988 (2012).
  • (17) Parkin, S. S. P., Hayashi, M. & Thomas, L. Magnetic domain-wall racetrack memory. Science 320, 190–194 (2008).
  • (18) Yamanouchi, M., Chiba, D., Matsukura, F. & Ohno, H. Current-induced domain-wall switching in a ferromagnetic semiconductor structure. Nature 428, 539–542 (2004).
  • (19) Schulz, T. et al. Emergent electrodynamics of skyrmions in a chiral magnet. Nature Phys. 8, 301–304 (2012).
  • (20) Thiele, A. A. Steady-state motion of magnetic domains. Phys. Rev. Lett. 30, 230–233 (1973).
  • (21) Everschor, K. et al. Current-induced rotational torques in the skyrmion lattice phase of chiral magnets. Phys. Rev. B 86, 054432 (2012).
  • (22) Everschor, K. et al. Rotating skyrmion lattices by spin torques and field or temperature gradients. Phys. Rev. B 86, 054432 (2012).
  • (23) He, J. et al. Current-driven vortex domain wall dynamics by micromagnetic simulations. Phys. Rev. B 73, 184408 (2006).
  • (24) Iwasaki, J., Mochizuki, M. & Nagaosa, N. Universal current-velocity relation of skyrmion motion in chiral magnets. Nat. Commun. 4, 1463 (2013).
  • (25) Makhfudz, I., Krüger, B. & Tchernyshyov, O. Inertia and chiral edge modes of a skyrmion magnetic bubble. Phys. Rev. Lett. 109, 217201 (2012).
  • (26) Kubo, R. The fluctuation-dissipation theorem. Rep. Prog. Phys. 29, 255–284 (1966).
  • (27) García-Palacios, J. L. and Lázaro, F. J. Langevin-dynamics study of the dynamical properties of small magnetic particles. Phys. Rev. B 58, 14937–14958 (1998).
  • (28) Clarke, D. J. and Tretiakov, O. A. and Chern, G.-W. and Bazaliy, Y. B. and Tchernyshyov, O., Phys. Rev. B 78, 134412 (2008).
  • (29) Petrova, O. and Tchernyshyov O., Phys. Rev. B 84, 214433 (2011).
  • (30) Tatara, G., Kohno, H., & Shibata, J. Microscopic approach to current-driven domain wall dynamics. Physics Reports 468, 213–301 (2008).
  • (31) Schütte, C. and Garst, M. Magnon-skyrmion scattering in chiral magnets. arxiv 1405.1568 (2014).
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