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INTRODUCTION: VORTEX INSTABILITY

In classical models for quasi-two-dimensional magnetic materials[1], it has been found that vortex nonlinear excitations play an active role in phase transitions, [2],[3] and are expected to be important in the spin dynamics. [4],[5],[6] The vortices are topologically stable excitations, carry effective charges, are created in particle-antiparticle pairs, and are expected to make contributions to correlation functions, especially, to central peak intensity in the dynamic structure function [5] . In particular, in models of three-component classical spins with easy-plane (XY) anisotropy, there are two types of vortices possible, [7],[8] known as ``in-plane'' and ``out-of-plane'' vortices, depending on whether the static vortex has zero or nonzero out-of-easy-plane spin components, respectively. For ferro- and antiferro-magnets, the static structure of the in-plane vortex is known exactly, while the static structure of the out-of-plane vortex is only known approximately (or numerically). Approximate results are also known for the modification of these spin structures for slowly moving vortices. [8],[9] Furthermore, the dynamics of pairs of vortices has received some study; for pairs of out-of-plane vortices, there are interesting orbital and translational relative motions with faster cyclotron-like oscillations superimposed. [9],[10],[11]

Some attempts have been made to describe these motions as found from numerical simulations by effective equations of motion for the vortex centers, [4],[12],[13] including effective masses and charges [11],[14],[15] that determine the dynamics (collective coordinates. [16]) However, these approaches have assumed that a vortex has no internal dynamics, that a moving vortex consists of a uniformly translating spin profile of fixed shape, with no internal oscillations or other intrinsic time dependence. However, it is expected that the vortex spin profile can have some kind of internal oscillation, perhaps even when it is stationary (i.e., not translating), in analogy with the internal modes of nonlinear excitations in one dimension. [17] Little is known about such dynamic modes of individual vortices. A description of their properties could be valuable in application to the collective coordinate theory [18] and in calculations of dynamic response functions. These modes can be determined, however, by evaluating through numerical diagonalization the small amplitude normal modes of oscillation of the spin field about a single vortex. The resulting spinwave spectrum may contain particular modes that are strongly associated with the presence of the vortex itself, and otherwise absent if the vortex is absent. It is likely that these modes would be localized on the vortex. In addition, the spectrum will contain other modes that are extended over the entire system, and possibly only modified slightly by the presence of the vortex. Those modes, however, will contain information about the interaction of the spinwaves with the vortex. For these reasons, we investigate numerically the spinwave modes of a system containing an individual vortex, and analyze one particular spinwave mode that is responsible for an intrinsic instability [8],[19] of the in-plane vortex towards developing large out-of-plane spin components and becoming an out-of-plane vortex as the easy-plane anisotropy is reduced.

Specifially, we consider a set of classical spin variables on a two-dimensional (2D) lattice, interacting with easy-plane anisotropic near neighbor exchange. The easy-plane anisotropy will be described by the parameter () in the following Hamiltonian:

 

The sum is over nearest neighbor pairs of spins S on a 2D lattice with sites , and the set of displacements to the nearest neighbors is .

Much of the theory for magnetic vortices in this model has been developed in continuum limits. In the present context, Costa et al. [20] and Pereira et al. [21] have considered the spinwave modes about single vortices and vortex-antivortex pairs [22] in the XY model (), using a continuum limit description of the lattice. However, a continuum description of a magnetic vortex on a lattice presents difficulties, because the spin field varies rapidly from one lattice site to the next in the core region of the vortex, violating the usual continuum assumptions. Also, the short distance cutoff (for example, in energy integrals) in the continuum theory is not well-prescribed, whereas these difficulties do not appear if one solves for the spinwave modes in the original lattice model. For these reasons, we consider vortices in this model on a lattice, where the discrete lattice effects, that are most influential in the core of the vortex, can be correctly accounted for.

It is well-established that for this model with a specified strength of easy-plane anisotropy, only one of the vortex types is numerically stable when placed on a lattice. [8],[19] Numerical simulations have led to the conclusion that static in-plane vortices are stable only when is less than a critical value . On the other hand, static out-of-plane vortices are stable only when is greater than . To say that one type is unstable means that it will evolve into the other type. The critical value was found to have a substantial lattice-dependence; is approximately 0.62, 0.70, 0.84, for triangular, square, and hexagonal lattices, respectively (for ferromagnets). This strong lattice dependence is due partly to the discreteness effects near the vortex core, for which the usual continuum limit theories are likely to be inadequate.

This instability or crossover has been found to be driven by a particular dynamic mode of the in-plane vortex, [23] whose frequency goes to zero as approaches . Preliminary numerical diagonalizations were made for the spinwave modes of a square lattice system containing one vortex, with a free boundary condition. [9],[24] A mode that became soft was found to have its amplitude concentrated near the center of the vortex, suggesting that it is a localized mode associated with the presence of the vortex, as opposed to an extended continuum spinwave mode of the entire system. More recently, an Ansatz was made for the structure of a vortex on a lattice, [23] in order to explain the lattice dependence of . In this Ansatz, it was assumed that only a small set of spins near the core of the vortex could have nonzero out-of-plane spin components, while all other spins farther out from the core were held fixed in the easy plane. The out-of-plane spin components were assumed to depend only on the radial distance from the vortex center. The analysis was used to determine very accurately the values of for the different lattices mentioned above. More importantly, it also was used to make estimates of the frequency of the dynamic mode responsible for the in-plane to out-of-plane vortex crossover. However, it is clear that a more complete analysis of the spinwave modes about a static vortex is needed, especially including an understanding of how that eigenfrequency depends on the system size.

Therefore, we have made a set of numerical diagonalizations for finite systems, to obtain the normal modes (i.e., spinwaves) in the presence of a single in-plane vortex for , and in the presence of a single out-of-plane vortex for . The calculations described here are semiclassical; the spin equations of motion have been linearized about a numerically-determined static vortex solution, using local Cartesian spin components with different local spin axes at each site. The notation for the calculation is described in the following section. Approximately circular systems on triangular, square, and hexagonal lattices were used. A set of calculations was performed for each lattice, with a range of system sizes. For each system used, the dependence of the eigenspectrum on the anisotropy was determined. This includes measuring the rms ``sizes'' of the wavefunctions associated with the modes, and comparing to the size of the finite system that was used, to decide which modes are localized and which are extended. The mode whose frequency approaches zero as approaches has occupied much of our attention. We give substantial analysis of its dependence on , the type of lattice, and the system size.



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Next: PERTURBATION ABOUT A Up: NORMAL MODES OF VORTICES Previous: NORMAL MODES OF VORTICES



Gary M Wysin
Mon Sep 11 12:02:10 CDT 1995