软x射线吸收光谱在变温度下研究了W(110)上Mn单分子层的自旋螺旋态

J. Honolka, S. Krotzky, M. Menzel, T. Herden, V. Sessi, H. Ebert, J. Minár, K. Bergmann, R. Wiesendanger, O. Šipr
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引用次数: 1

摘要

利用软x射线吸收光谱研究了钨(110)晶体表面外延锰单层的非共线磁态,以补充早期的自旋极化STM实验。在8 ~ 300 K温度范围内测量了Mn - l23的x射线吸收光谱(XAS)、x射线线性二色性(XLD)和x射线磁圆二色性(XMCD)边缘光谱,并与完全相对论性从头计算结果进行了比较。我们表明,反铁磁(AFM)螺旋和摆线螺旋会产生明显不同的Mn l23边缘XLD信号,从而能够区分它们。结果表明,W(110)上Mn单分子层的磁基态是AFM摆线自旋螺旋。基于温度相关的XAS, XLD和场致XMCD光谱,我们推断W(110)上Mn单层的磁性能随温度变化,但这种变化缺乏明确的相变指示,在所研究的温度范围内高达300 K -即使在170 K左右存在交叉,XAS分支比的温度依赖性和XLD剖面。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Spin-spiral state of a Mn monolayer on W(110) studied by soft x-ray absorption spectroscopy at variable temperatures
The noncollinear magnetic state of epitaxial Mn monolayers on tungsten (110) crystal surfaces is investigated by means of soft x-ray absorption spectroscopy, to complement earlier spin-polarized STM experiments. X-ray absorption spectra (XAS), x-ray linear dichroism (XLD) and x-ray magnetic circular dichroism (XMCD) Mn L23-edge spectra were measured in the temperature range from 8 to 300 K and compared to results of fully-relativistic ab initio calculations. We show that antiferromagnetic (AFM) helical and cycloidal spirals give rise to significantly different Mn L23-edge XLD signals, enabling thus to distinguish between them. It follows from our results that the magnetic ground state of a Mn monolayer on W(110) is an AFM cycloidal spin spiral. Based on temperature-dependent XAS, XLD and field-induced XMCD spectra we deduce that magnetic properties of the Mn monolayer on W(110) vary with temperature, but this variation lacks a clear indication of a phase transition in the investigated temperature range up to 300 K - even though a crossover exists around 170 K in the temperature dependence of XAS branching ratios and in XLD profiles.
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