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Relationship between orbital moment anisotropy, magnetocrystalline anisotropy, and Dzyaloshinskii-Moriya interaction in W/Co/Pt trilayers
Physical Review B ( IF 3.2 ) Pub Date : 2024-11-07 , DOI: 10.1103/physrevb.110.184401 Zhendong Chi, Yong-Chang Lau, Vanessa Li Zhang, Goro Shibata, Shoya Sakamoto, Yosuke Nonaka, Keisuke Ikeda, Yuxuan Wan, Masahiro Suzuki, Masashi Kawaguchi, Masako Suzuki-Sakamaki, Kenta Amemiya, Naomi Kawamura, Masaichiro Mizumaki, Motohiro Suzuki, Hyunsoo Yang, Masamitsu Hayashi, Atsushi Fujimori
Physical Review B ( IF 3.2 ) Pub Date : 2024-11-07 , DOI: 10.1103/physrevb.110.184401 Zhendong Chi, Yong-Chang Lau, Vanessa Li Zhang, Goro Shibata, Shoya Sakamoto, Yosuke Nonaka, Keisuke Ikeda, Yuxuan Wan, Masahiro Suzuki, Masashi Kawaguchi, Masako Suzuki-Sakamaki, Kenta Amemiya, Naomi Kawamura, Masaichiro Mizumaki, Motohiro Suzuki, Hyunsoo Yang, Masamitsu Hayashi, Atsushi Fujimori
We have studied the Co layer thickness dependences of magnetocrystalline anisotropy (MCA), Dzyaloshinskii-Moriya interaction (DMI), and orbital moment anisotropy (OMA) in W/Co/Pt trilayers, in order to clarify their correlations with each other. We find that the MCA favors magnetization along the film normal and monotonically increases with decreasing effective magnetic layer thickness (𝑡 e f f ). The magnitude of the Dzyaloshinskii-Moriya exchange constant (| 𝐷 | ) increases with decreasing 𝑡 e f f until 𝑡 e f f ∼ 1 nm, below which | 𝐷 | decreases. The MCA and | 𝐷 | scale with 1 / 𝑡 e f f for 𝑡 e f f larger than ∼ 1 nm, indicating an interfacial origin. The increase of MCA with decreasing 𝑡 e f f continues below 𝑡 e f f ∼ 1 nm, but with a slower rate. To clarify the cause of the 𝑡 e f f dependences of MCA and DMI, the OMA of Co in W/Co/Pt trilayers is studied using x-ray magnetic circular dichroism. We find nonzero OMA when 𝑡 e f f is smaller than ∼ 0 . 8 nm. The OMA increases with decreasing 𝑡 e f f more rapidly than what is expected from the MCA, indicating that factors other than OMA contribute to the MCA at small 𝑡 e f f . The 𝑡 e f f dependence of the OMA also suggests that | 𝐷 | at 𝑡 e f f smaller than ∼ 1 nm is not related to the OMA at the interface. We propose that the growth of Co on W results in a strain and/or texture that reduces the interfacial DMI, and, to some extent, MCA at small 𝑡 e f f .
中文翻译:
W/Co/Pt 三层中轨道矩各向异性、磁晶各向异性与 Dzyaloshinskii-Moriya 相互作用的关系
我们研究了磁晶各向异性 (MCA)、Dzyaloshinskii-Moriya 相互作用 (DMI) 和轨道矩各向异性 (OMA) 在 W/Co/Pt 三层中的钴层厚度依赖性,以阐明它们之间的相关性。我们发现 MCA 有利于沿薄膜法向磁化,并且随着有效磁层厚度 (teff ) 的减小而单调增加。Dzyaloshinskii-Moriya 交换常数 (|D| ) 的大小随着 teff 的减小而增加,直到 teff∼1 nm,低于该波长 |D| 时减小。MCA 和 |D| 刻度为 1/teff ,对于大于 ∼1 nm 的 teff ,表示界面起源。MCA 的增加随着 teff 的减少而继续在 teff∼ 1 nm 以下,但速率较慢。为了阐明 MCA 和 DMI 的画眉草 依赖性的原因,使用 X 射线磁圆二色性研究了 W/Co/Pt 三层中 Co 的 OMA。当 teff 小于 ∼0.8 nm 时,我们发现 OMA 不为零。OMA 随着苔麸 的减少而增加,其速度比 MCA 的预期要快,这表明 OMA 以外的因素对小苔麸 的 MCA 有贡献。OMA 的 teff 依赖性还表明,小于 ∼1 nm 的 teff 的 |D| 与界面处的 OMA 无关。 我们提出 Co 在 W 上的生长导致应变和/或质地,从而降低界面 DMI,并在一定程度上降低小苔麸 下的 MCA。
更新日期:2024-11-08
中文翻译:
W/Co/Pt 三层中轨道矩各向异性、磁晶各向异性与 Dzyaloshinskii-Moriya 相互作用的关系
我们研究了磁晶各向异性 (MCA)、Dzyaloshinskii-Moriya 相互作用 (DMI) 和轨道矩各向异性 (OMA) 在 W/Co/Pt 三层中的钴层厚度依赖性,以阐明它们之间的相关性。我们发现 MCA 有利于沿薄膜法向磁化,并且随着有效磁层厚度 (