从锥形阶段开始闪烁的 Skyrmion

Rai M. Menezes, Milorad V. Milosevic
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引用次数: 0

摘要

尽管人们已经广泛探索了天电离态和非拓扑态之间的转变,并将其作为电子器件信息传输和存储的比特操作,但这种转变的超快动力学仍然难以观察和理解。在这里,我们利用自旋动力学模拟和谐波转变态理论(HTST)深入分析了氦磁体中天电离态的成核过程。我们揭示了这些拓扑态在天离子态和锥形态相界附近特定条件下的持续闪烁(创造-不熄灭)现象。通过最小能量路径分析,我们阐明了这种闪烁行为是由手性晃子(CB)表面态的形成所促成的,而且由于它们的振荡模式不同,CB 的坍缩与薄膜中的天空离子不同。我们进一步利用 HTST 估算了作为外加磁场和温度函数的典型闪烁时间。最后,我们以基于天幕的随机数发生器为例,说明了天幕闪烁在受控概率计算中的实际应用。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Skyrmion blinking from the conical phase
While the transition between skyrmionic and non-topological states has been widely explored as a bit operation for information transport and storage in spintronic devices, the ultrafast dynamics of such transitions remains challenging to observe and understand. Here, we utilize spin-dynamics simulations and harmonic transition state theory (HTST) to provide an in-depth analysis of the nucleation of skyrmionic states in helimagnets. We reveal a persistent blinking (creation-annihilation) phenomenon of these topological states under specific conditions near the phase boundary between skyrmion and conical states. Through a minimum-energy path analysis, we elucidate that this blinking behavior is favored by the formation of chiral bobber (CB) surface states and that the collapse of CBs differs from that of skyrmions in thin films due to their different oscillation modes. We further employ HTST to estimate the typical blinking time as a function of the applied magnetic field and temperature. Finally, we illustrate the practical use of skyrmion blinking for controlled probabilistic computing, exemplified by a skyrmion-based random-number generator.
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