在元素Ni和Ni85Co15薄膜中的旋转动力学,在M2,3边缘周围由高波生成的光子探测
Juliette Dubois, Emmanuelle Jal1, Carlos Rodriguez Cortez2
1Sorbonne Université, CNRS, Laboratoire de Chimie Physique-Matière et Rayonnement, LCPMR, F-75005 Paris, France.
Structural dynamics (Melville, N.Y.)
|September 18, 2025
概括
与纯相比,-合金中的超快旋转动力学表现出明显的反应. 的存在影响了磁性散射时间尺度,揭示了这些3D金属对激光激发的反应方式的差异.
科学领域:
- 材料科学 材料科学 材料科学
- 凝聚物质物理学 凝聚物质物理学
- 超快的磁力 超快的磁力
背景情况:
- 磁性材料中的超快旋转动力学对于理解磁现象至关重要.
- -合金表现出复杂的磁性属性,受其组成的影响.
- 弱条纹域是某些磁性薄膜中的一个关键特征.
研究的目的:
- 为了比较激光激发的Ni85Co15合金和纯Ni薄膜的超快旋转动力学.
- 为了研究对的磁反应的影响.
- 用特定元素的X射线共振磁性散射探测动力学.
主要方法:
- 利用X射线共振磁性散射 (XRMS) 来探测磁力学动力学.
- 使用通过高波生成 (HHG) 产生的极端紫外线 (EUV) 脉冲.
- 同时探测到四个能量在 (Co) 和 (Ni) M2,3边缘周围的样品.
主要成果:
- 观察到激光诱导的磁性散射峰值强度在 femtosecond (fs) 时间尺度上显著减少.
- 证明这种减少是波长依赖的,显示不同的火幅度和时间尺度.
- 测量了合金中Ni和Co边缘之间分散强度动态的~17 fs延迟,在纯中不存在.
结论:
- 在合金中观察到的延迟凸显了Ni和Co的独特的超快磁反应.
- 的存在显著影响了Ni-Co合金中的旋转动态.
- 这些发现为3D过渡金属的特定元素超快磁性行为提供了洞察力.
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