13:15 〜 13:30
▲ [17p-501-1] Tuning the magnetic properties and surface morphology of D022 Mn3-δGa film by N doping
キーワード:MnGaN, MnGa, perpendicular magnetic anisotropy
Recently, tetragonal Mn-based alloys such as L10 and D022 Mn-Ga alloys [1] have been of great concern in search of new magnetic alloy systems with low Gilbert damping, low saturation magnetization Ms, and high perpendicular magnetic anisotropy Ku for potential applications such as a next generation spin transfer torque-magnetic random access memory. In this work, we present tuning the magnetic properties and surface morphology of D022 Mn3-δGa using a small amount of N doping [2]. 50 nm thick N-doped MnGa films were prepared by RF reactive sputtering technique on an MgO(001) single crystalline substrate at 480°C substrate temperature with the varied 0-0.66% N2 flow rate percentage (η) relative to Ar 30 sccm for two Mn3Ga and Mn2.5Ga compositions. N-doped Mn-Ga films all exhibited the gradual reduction in Ms up to 33-50% with the increasing N2 flow rate as in Fig. 1 (a). In particular, N-doped Mn2.5Ga case revealed the single D022 structural phase formation with the high Ku ≈ 1 MJ/m3 between η = 0-0.66% range despite the gradual reduction in magnetization, while N-doped Mn3Ga showed coherent growth of two D022 + E21 composite phases which results in the further reduction in Ms and Ku < 1 MJ/m3, as in Fig. 1 (b). In addition, N doping in both Mn3Ga and Mn2.5Ga caused the smoothening of the surface morphology with the increasing film thickness up to 50 nm even with the use of the minimum η of 0.25%, as shown in the inset of Fig. 1, which represents the modification of the film growth mode from Volmer-Weber type of D022 Mn-Ga case at this high 480°C growth temperature. Therefore, these results suggest that a small amount of N doping is an effective way of tuning the magnetic properties of D022 Mn3-δGa films in addition to obtaining a flat surface at high growth temperature. This work was partly supported by Samsung Electronics.
References:
[1] S. Mizukami, A. Sakuma, A. Sugihara, K. Z. Suzuki, and R. Ranjbar, Scripta Mater. 118, 70 (2016).
[2] H. Lee, H. Sukegawa, J. Liu, S. Mitani, and K. Hono, Appl. Phys. Lett. 109, 152402 (2016).
References:
[1] S. Mizukami, A. Sakuma, A. Sugihara, K. Z. Suzuki, and R. Ranjbar, Scripta Mater. 118, 70 (2016).
[2] H. Lee, H. Sukegawa, J. Liu, S. Mitani, and K. Hono, Appl. Phys. Lett. 109, 152402 (2016).