在低温和高压下,CRA的磁性结构不相称
Andreas Eich1, Andrzej Grzechnik2, Yixi Su3
1Jülich Centre for Neutron Science-2 and Peter Grünberg Institute-4 (JCNS-2/PGI-4), Forschungszentrum Jülich, 52425, Germany.
研究人员使用中子衍射研究化 (CrAs) 的磁性结构. 他们发现了一种新的螺旋磁结构,与之前提出的模型不同,为CRA提供了新的见解.
科学领域:
- 凝聚物质物理学 凝聚物质物理学
- 材料科学是一种材料科学.
- 晶体学 晶体学是指结晶学.
背景情况:
- 化 (CrAs) 呈现出复杂的磁性秩序.
- 了解其磁性结构对于预测其电子性质至关重要.
研究的目的:
- 为了阐明CRA的精确磁性结构.
- 解决以前结构模型中的差异.
主要方法:
- 在环境压力 (1.5300 K) 下的中子粉衍射.
- 在2K和0.12GPa的中子单晶衍射.
- 组理论分析和随机搜索磁矩精炼.
主要成果:
- 在267K时,CRA经历了反异构的阶段过渡.
- 磁结构与传播向量k = (0,0,kc) 不相称.
- 确定了一种新的螺旋磁结构,而不是简单的螺旋或环形,旋转旋转平面以c*方向的角度.
- 超空间组模型P21.1'(α0γ) 0s提供了最适合粉末和单晶数据的模型.
结论:
- 以前接受的CRA磁结构双螺旋模型是不正确的.
- 已经确定了一种新的,复杂的螺旋磁结构,具有一致的性.
- 这一发现促进了对CRA中的磁相转换的理解.
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