1. Contributions of Co and Fe orbitals to perpendicular magnetic anisotropy of MgO/CoFeB bilayers with Ta, W, IrMn, and Ti underlayers
- Author
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Kab-Jin Kim, Seung-heon Chris Baek, Mio Ishibashi, Kihiro T. Yamada, Takahiro Moriyama, Yoshinori Kotani, Sanghoon Kim, Teruo Ono, Byong-Guk Park, Takaya Okuno, Takuya Taniguchi, and Tetsuya Nakamura
- Subjects
010302 applied physics ,Circular dichroism ,Materials science ,Condensed matter physics ,Perpendicular magnetic anisotropy ,Magnetic circular dichroism ,General Engineering ,Dead layer ,General Physics and Astronomy ,02 engineering and technology ,021001 nanoscience & nanotechnology ,01 natural sciences ,Condensed Matter::Materials Science ,Atomic orbital ,0103 physical sciences ,Moment (physics) ,Perpendicular ,Spin transfer ,Astrophysics::Earth and Planetary Astrophysics ,0210 nano-technology - Abstract
We study the perpendicular magnetic anisotropy (PMA) of the CoFeB/MgO bilayers in contact with W, Ta, IrMn, and Ti, which have been suggested for use as the spin–orbit-torque-related underlayers. The saturation magnetization of CoFeB depends on the underlayer material used owing to the formation of a dead layer that affects the PMA strength of each film. The X-ray magnetic circular dichroism measurement reveals that interfacial intermixing suppresses only the perpendicular orbital moment of Fe, whereas it simultaneously suppresses both the perpendicular and in-plane orbital moments of Co.
- Published
- 2017
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