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近年来, 作为一种自旋电子学领域的关键材料, 具有高温本征铁磁性的稀磁半导体受到了广泛的关注. 为探索能够提高本征铁磁性居里温度(Curie temperature, T C)的方法, 本文运用第一性原理LDA+ U方法研究了应变对Mo掺杂GaSb的电子结构、磁学及光学性质的影响. 研究结果表明: –6%—2.5%应变范围下GaSb半导体材料具有稳定的力学性能, 压应变下GaSb材料的可塑性、韧性增强, 有利于GaSb半导体材料力学性能的提升; 应变对Mo替代Ga缺陷(Mo Ga)的电子结构有重要的影响, –3%至–1.2%应变范围下Mo Ga处于低自旋态(low spin state, LSS), 具有1
${\mu _{{\rm{B}}}}$ 的局域磁矩, –1.1%—2%应变范围下Mo Ga处于高自旋态(high spin state, HSS), 具有3${\mu _{{\rm{B}}}}$ 的磁矩; 不管是LSS还是HSS, Mo Ga产生局域磁矩之间的耦合都是铁磁耦合, 但铁磁耦合的强度和物理机制不同, 适当的压应变可有效提高铁磁耦合强度, 这有利于实现高 T C的GaSb基磁性半导体; Mo可极大提高GaSb半导体材料的电极化能力, 这有利于光生电子-空穴对的形成和分离, 提高掺杂体系对长波光子的光电转化效率; Mo引入的杂质能级使电子的带间跃迁对所需要吸收光子的能量变小, 掺杂体系光学吸收谱的吸收边发生了红移, 拉应变可进一步提升(Ga,Mo)Sb体系在红外光区的光学性能.In recent decades, as a kind of critical material in spintronics field, the diluted magnetic semiconductor with high temperature and intrinsic ferromagnetism has attracted extensive attention. In order to explore the approach to enhancing Curie temperature ( T C), the LDA+ Umethod of the first-principles calculation is adopted to study the effect of strain on electronic structure, magnetic and optical properties in Mo doped GaSb system. The results indicate that the structure of GaSb is stable with strain in a range of –6%—2.5%. Plasticity and toughness of GaSb increase under compressive strains, which is conducive to the improvement of the mechanical properties. The strain affects the electronic structure of Mo Gagreatly. In a range from –3% to –1.2%, Mo Gais in the low spin state (LSS) with a 1${\mu _{{\rm{B}}}}$ local magnetic moment, while in a range of –1.1%—2%, Mo Gais in high spin state (HSS) with a 3${\mu _{{\rm{B}}}}$ moment. The magnetic interactions between Mo Gaand Mo Gaare all ferromagnetic for LSS and so is the case for HSS, although they are different in coupling intensity and mechanism. In particular, appropriate compressive strains can improve the strength of ferromagnetic coupling effectively and are favorable for the preparation of the GaSb-based diluted magnetic semiconductors with high Curie temperatures and inherent ferromagnetism. Moreover, we find that Mo can greatly improve the polarization capability of GaSb and play a vital role in forming and separating the electron-hole pairs, and thus further improving the photoelectric conversion capability for long wave photons. The energy required to absorb photons for inter-band transition of electrons decreases because of the impurity levels induced by Mo, which leads the absorption edge to be red-shifted. The optical properties of (Ga,Mo)Sb in infrared region are further enhanced by the tensile strain.[1] [2] [3] [4] [5] [6] [7] [8] [9] [10] [11] [12] [13] [14] [15] [16] [17] [18] [19] [20] [21] [22] [23] [24] [25] [26] [27] [28] [29] [30] [31] [32] [33] [34] [35] [36] [37] [38] [39] [40] [41] [42] [43] [44] [45] [46] [47] [48] [49] [50] [51] [52] [53] [54] [55] [56] [57] [58] [59] [60] [61] [62] [63] [64] [65] [66] [67] [68] [69] [70] [71] -
Strain/% B/GPa G/GPa $\gamma $ B/G –6 148.21 37.67 0.38 3.93 –5 129.66 43.08 0.35 3.01 –3.7 109.93 43.85 0.32 2.51 –2 90.03 43.30 0.29 2.08 0 68.77 47.21 0.22 1.46 0.5 68.73 47.17 0.22 1.47 1 64.26 45.47 0.21 1.48 1.5 61.35 40.38 0.20 1.52 2 55.49 38.02 0.20 1.53 -
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