Thickness-dependent magnetic properties and strain-induced orbital magnetic moment in SrRuO3 thin films

被引:47
|
作者
Ishigami, K. [1 ]
Yoshimatsu, K. [2 ]
Toyota, D. [2 ]
Takizawa, M. [1 ]
Yoshida, T. [1 ]
Shibata, G. [1 ]
Harano, T. [1 ]
Takahashi, Y. [1 ]
Kadono, T. [1 ]
Verma, V. K. [1 ]
Singh, V. R. [1 ]
Takeda, Y. [3 ]
Okane, T. [3 ]
Saitoh, Y. [3 ]
Yamagami, H. [3 ]
Koide, T. [4 ]
Oshima, M. [2 ]
Kumigashira, H. [2 ,4 ]
Fujimori, A. [1 ,3 ,5 ]
机构
[1] Univ Tokyo, Dept Phys, Bunkyo Ku, Tokyo 1130033, Japan
[2] Univ Tokyo, Dept Appl Chem, Bunkyo Ku, Tokyo 1138656, Japan
[3] Japan Atom Energy Agcy, Quantum Beam Sci Directorate, Sayo, Hyogo 6795148, Japan
[4] High Energy Accelerator Res Org, IMSS, Photon Factory, Tsukuba, Ibaraki 3050801, Japan
[5] Univ Tokyo, Dept Complex Sci & Engn, Kashiwa, Chiba 2770882, Japan
关键词
RAY CIRCULAR-DICHROISM; ELECTRONIC-STRUCTURE; ANISOTROPY;
D O I
10.1103/PhysRevB.92.064402
中图分类号
T [工业技术];
学科分类号
08 ;
摘要
Thin films of the ferromagnetic metal SrRuO3 (SRO) show a varying easy magnetization axis depending on the epitaxial strain, and undergo a metal-to-insulator transition with decreasing film thickness. We have investigated the magnetic properties of SRO thin films with varying thicknesses fabricated on SrTiO3(001) substrates by soft x-ray magnetic circular dichroism at the Ru M-2,M-3 edge. Results have shown that, with decreasing film thickness, the film changes from ferromagnetic to nonmagnetic at around 3 monolayer thickness, consistent with previous magnetization and magneto-optical Kerr effect measurements. The orbital magnetic moment perpendicular to the film was found to be similar to 0.1 mu(B)/Ru, and remained nearly unchanged with decreasing film thickness while the spin magnetic moment decreases. A mechanism for the formation of the orbital magnetic moment is discussed based on the electronic structure of the compressively strained SRO film.
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页数:5
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