2017
DOI: 10.1103/physrevx.7.041045
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Quantum Dynamics of Skyrmions in Chiral Magnets

Abstract: We study the quantum propagation of a Skyrmion in chiral magnetic insulators by generalizing the micromagnetic equations of motion to a finite-temperature path integral formalism, using field theoretic tools. Promoting the center of the Skyrmion to a dynamic quantity, the fluctuations around the Skyrmionic configuration give rise to a time-dependent damping of the Skyrmion motion. From the frequency dependence of the damping kernel, we are able to identify the Skyrmion mass, thus providing a microscopic descri… Show more

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Cited by 70 publications
(86 citation statements)
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“…We now write a general theory applicable to bosonic systems where the Bloch wave function corresponding to the band dispersion ε n,k is given by |ψ n,k = e ik·r |u n,k . We can then introduce a notation [42]…”
mentioning
confidence: 99%
“…We now write a general theory applicable to bosonic systems where the Bloch wave function corresponding to the band dispersion ε n,k is given by |ψ n,k = e ik·r |u n,k . We can then introduce a notation [42]…”
mentioning
confidence: 99%
“…We next address the stochastic dynamics of the skyrmion described by the classical fields Φ 0 and Θ 0 in contact with the bath of magnetic excitations at finite temperature driven by an external magnetic field that oscillates in time. This is achieved by first promoting the skyrmion center-of-mass to a dynamical variable R(t), then treating the magnetic excitations as quantum fluctuations around the classical field, and finally obtaining an effective functional [1,39,40,60] by integrating out the magnon degrees of freedom. At the same time, the real-time dynamics of the external field as well as the stochastic effects of the magnon bath at finite T are captured by replacing the time integration by an integration over the Keldysh contour which consists of two branches.…”
Section: Langevin Equationmentioning
confidence: 99%
“…Magnetic excitations are defined as fluctuations around the classical skyrmion solution through a consistent separation between collective (center-of-mass) and intrinsic (magnetic excitations) degrees of freedom. A description of the dynamics of one-dimensional (1D) domain walls [39] and 2D magnetic skyrmions [40] in a magnetic insulator beyond the classical framework, demonstrated that the dissipation arising from the magnetic excitations is generally non-Markovian with a damping kernel that is nonlocal in time. The quantum nature of the magnetic bath, naturally incorporated within this approach, becomes evident in the nontrivial temperature T dependence of the damping kernel which remains finite even for vanishingly small T .…”
Section: Introductionmentioning
confidence: 99%
“…The transformation matrix satisfies the paraunitary normalization relations, T † k σ 3 T k = σ 3 and T k σ 3 T † k = σ 3 , where here and henceforth σ i (i = 1, 2, 3) stands for the Pauli matrices acting in the particle-hole space. The particlehole space Hamiltonian can be regarded as a pseudo-Hermitian Hamiltonian, with the eigenequation [55] σ 3 H k |u n,k =ε n,k |u n,k ,…”
Section: Introductionmentioning
confidence: 99%