Origin of perpendicular magnetic anisotropy in CoxFe3-xO4+δ thin films studied by x-ray magnetic circular and linear dichroisms

被引:9
|
作者
Okabayashi, Jun [1 ]
Tanaka, Masaaki A. [2 ]
Morishita, Masaya [2 ]
Yanagihara, Hideto [3 ]
Mibu, Ko [2 ]
机构
[1] Univ Tokyo, Res Ctr Spectrochem, Bunkyo Ku, Tokyo 1130033, Japan
[2] Nagoya Inst Technol, Grad Sch Engn, Nagoya, Aichi 4668555, Japan
[3] Univ Tsukuba, Dept Appl Phys, Tsukuba, Ibaraki 3058573, Japan
关键词
COFE2O4; MGO;
D O I
10.1103/PhysRevB.105.134416
中图分类号
T [工业技术];
学科分类号
08 ;
摘要
We investigate the element-specific spin and orbital states and their roles in magnetic anisotropy in Co-ferrite [CoxFe3-xO4+delta (001)] thin films which exhibit perpendicular magnetic anisotropy (PMA). The origin of PMA in the low-x region (x < 1) can be mainly explained by the large perpendicular orbital magnetic moments in the Co2+ (3d(7)) states detected by x-ray magnetic circular dichroism and x-ray magnetic linear dichroism (XMLD). The XMLD for a PMA film (x = 0.2) with a square hysteresis curve shows the oblate charge distribution in the Co2+ site, which is consistent with the change in local nearest-neighbor distance in Co detected by extended x-ray absorption fine structure analysis. Our finding reveals that the microscopic origin of PMA in Co ferrite comes from the enhanced orbital magnetic moments along the out-of-plane [001] direction through in-plane charge distribution by tensile strain, which adds the material functionalities in spinel ferrite thin films from the viewpoint of strain and orbital magnetic moments.
引用
收藏
页数:8
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