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arXiv 2502.03166cond-mat.mes-hall
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热自旋波噪声作为 Dzyaloshinskii-Moriya 相互作用的探针

Thermal spin wave noise as a probe for the Dzyaloshinkii-Moriya interaction

Aurore Finco, Pawan Kumar, Van Tuong Pham, Joseba Urrestarazu-Larrañaga, Rodrigo Guedas Garcia, Maxime Rollo, Olivier Boulle, Joo-Von Kim, Vincent Jacques

AI总结:

本文提出利用扫描 NV 色心弛豫测量法探测畴壁和斯格明子中的热自旋波噪声,通过噪声幅度和分布推断 DMI 符号及斯格明子的 Néel/Bloch 性质。

摘要:

界面 Dzyaloshinskii-Moriya 相互作用(DMI)是稳定薄膜中手性磁态的关键因素。其符号和强度往往决定磁性对象的关键性质,例如它们的拓扑结构或如何用电流操控它们。目前有几种实验技术可以定量测量 DMI,这些技术基于对畴壁、自旋波或自旋轨道矩的研究。在这项工作中,我们提出了一种自旋波方法的定性变体。我们利用垂直磁化薄膜中畴壁和斯格明子内受限热自旋波产生的磁噪声,并通过扫描 NV 色心弛豫测量法进行探测。我们通过数值模拟和实验表明,DMI 的符号可以从检测到的噪声幅度中推断出来,该幅度受到自旋波色散中非互易性的影响。此外,我们还证明,围绕磁斯格明子轮廓的噪声分布揭示了它们的 Néel/Bloch 性质,从而也为稳定它们所需的 DMI 强度提供了见解。

英文摘要:

Interfacial Dzyaloshinkii-Moriya interaction (DMI) is a key ingredient in the stabilization of chiral magnetic states in thin films. Its sign and strength often determine crucial properties of magnetic objects, like their topology or how they can be manipulated with currents. A few experimental techniques are currently available to measure DMI quantitatively, based on the study of domain walls, spin waves, or spin-orbit torques. In this work, we propose a qualitative variant of spin wave methods. We rely on magnetic noise from confined thermal spin waves in domain walls and skyrmions in perpendicularly magnetized thin films, which we probe with scanning NV center relaxometry. We show both numerically and experimentally that the sign of the DMI can be inferred from the amplitude of the detected noise, which is affected by the non-reciprocity in the spin wave dispersion. Furthermore, we also demonstrate that the noise distribution around the contour of magnetic skyrmions reveals their Néel/Bloch nature, giving therefore also insight into the strength of DMI involved in their stabilization.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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