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Magnetoelectric skyrmions in multiferroics

机译:多铁磁中的磁电天空

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摘要

Skyrmion is a topologically stable particle-like object originally proposed by field theory, which has recently been identified in chiral-lattice magnets as vortex-like swirling spin texture of typical size ranging from 5 nm to 100 nm[1,2] . In metallic system, skyrmions can be moved by electric current through the spin-transfer torque[3] . Because of its electric controllability, nanometric scale, and particle-like nature, skyrmion is now rapidly attracting attention as a promising building block for novel spintronic device like high density magnetic storage[4] . However, such current-driven approach inevitably involves joule heat loss, and the previous observation of skyrmions has been limited to specific metallic alloys with chiral B20 structure . Based on the assumption that the chiral symmetry of underlying crystal lattice and associated Dzyaloshinskii-Moriya interaction plays a crucial role for the stabilization of skyrmion spin texture, we have recently discovered the emergence of skyrmions in a chiral-lattice insulator CuOSeO by performing the Lorentz transmission electron microscopy and small angle neutron scattering[5,6] . Through the detailed dielectric and magnetic measurements, we proved that the skyrmion spin texture in insulator can magnetically induce electric polarization via the relativistic spin-orbit interaction[7] . Such a coupling between skyrmion spin texture and electric dipole strongly suggests that skyrmions in insulators can be manipulated by external electric field, which has later been confirmed by the experiments of small angle neutron scattering[8] and magnetic resonance[9] . Since this approach is free from the Joule heat loss compared to the current-driven method in the metallic system, our present finding of magnetoelectric skyrmions in insulators can be considered as a key milestone for the development of next generation of ultra-high-density magnetic storage device with extremely low energy consumption .
机译:Skyrmion是最初由场论提出的一种拓扑稳定的粒子状物体,最近已在手性晶格磁体中确定为典型大小为5 nm至100 nm的漩涡状旋涡自旋织构[1,2]。在金属系统中,天体离子可以通过自旋传递扭矩[3]被电流移动。由于其电可控性,纳米尺度和类粒子性质,作为一种新的自旋电子学器件(如高密度磁存储)的有前途的构建材料,天蝎子现在正迅速受到关注[4]。然而,这种电流驱动的方法不可避免地涉及焦耳热损失,并且先前对天rm子的观察仅限于具有手性B20结构的特定金属合金。基于以下假设:下层晶格的手性对称性和相关的Dzyaloshinskii-Moriya相互作用对于稳定天rm子自旋结构起着至关重要的作用,我们最近通过执行洛仑兹传输发现了手征格绝缘子CuOSeO中天rm子的出现。电子显微镜和小角中子散射[5,6]。通过详细的介电和磁测量,我们证明了绝缘子中的天蝎子自旋织构可以通过相对论自旋轨道相互作用而磁感应极化[7]。天体离子自旋纹理与电偶极子之间的这种耦合强烈表明,绝缘子中的天体离子可以通过外部电场来操纵,后来通过小角中子散射[8]和磁共振[9]的实验证实了这一点。与金属系统中的电流驱动方法相比,由于这种方法没有焦耳热损失,因此我们目前在绝缘子中发现的磁电天文离子可以被认为是下一代超高密度磁粉发展的关键里程碑。能耗极低的存储设备。

著录项

  • 来源
  • 会议地点 Beijing(CN)
  • 作者

    Seki S.;

  • 作者单位

    Center for Emergent Matter Sci. (CEMS), RIKEN, Wako, Japan;

  • 会议组织
  • 原文格式 PDF
  • 正文语种 eng
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