arXivDaily arXiv每日学术速递 周一至周五更新
arXiv 2201.12794cond-mat.str-el
收藏

压力下Néel skyrmion宿主GaV $_4$ S $_8$的磁性

Magnetism in the Néel skyrmion host GaV$_4$S$_8$ under pressure

T. J. Hicken, M. N. Wilson, S. J. R. Holt, R. Khassanov, M. R. Lees, R. Gupta, D. Das, G. Balakrishnan, T. Lancaster

摘要:

我们目前的磁化和μ子自旋谱测量Néel skyrmion主机下的应用流体静压高达$P=2.29$ GPa的GaV $_4$ S $_8$。我们的研究结果表明,磁相图是改变与压力,通过减少交叉温度从摆线(C)铁磁类状态与增加$P$,这样,由2.29 GPa,C状态似乎坚持到最低的测量温度。借助于微磁模拟,我们提出,这种变化背后的驱动机制是减少系统的磁各向异性,并建议这可能会导致增加稳定性的skyrmion晶格。

英文摘要:

We present magnetization and muon-spin spectroscopy measurements of Néel skyrmion-host GaV$_4$S$_8$ under the application of hydrostatic pressures up to $P=2.29$ GPa. Our results suggest that the magnetic phase diagram is altered with pressure via a reduction in the crossover temperature from the cycloidal (C) to ferromagnetic-like state with increasing $P$, such that, by 2.29 GPa, the C state appears to persist down to the lowest measured temperatures. With the aid of micromagnetic simulations, we propose that the driving mechanism behind this change is a reduction in the magnetic anisotropy of the system, and suggest that this could lead to an increase in stability of the skyrmion lattice.

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。

↑