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APS -APS March Meeting 2017 - Event - Quasi-particle self-consistent GW calculation of the band structure of $eta$-Ga$_2$O$_3$

机译:APS -APS 2017年3月会议-事件-$ eta $ -Ga $ _2 $ O $ _3 $的能带结构的准粒子自洽GW计算

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$eta$-Ga$_2$O$_3$ has recently received attention as an ultra wideband gap oxide. There are still uncertainties over its basic electronic structure. Here we present QSGW calculations of the band structure implemented in the linearized muffin-tin orbital approach. The QSGW approach usually overestimates the band gap, due to the underestimated screening in the random phase approximation (RPA) used to calculate$W$. Even after taking into account a universal 0.8 correction factor for this effect, we find a gap of order 5.4 eV, significantly higher than experimental values for the absorption onset. After inclusion of a lattice polarization effect on the screening, we find a minimum direct gap at $Gamma$ of 4.9 eV. The zero-point motion correction is estimated to be another 0.2 eV, leading to a final gap of 4.7 eV in good agreement with experiment. The indirect gap is found to be about 0.1 eV smaller. Symmetry labeling the states near the VBM and CBM at $Gamma$ shows that the lowest gap at $Gamma$ is allowed for ${f E}perp{f b}$, and the first transition allowed for ${f E}parallel{f b}$ occurs 0.6 eV higher. This predicted shift of the absorption onset for different directions is larger than found in experiment. Calculated absorption curves will be presented.
机译:作为超宽带隙氧化物,$ eta-Ga $ _2 $ O $ _3 $最近受到关注。其基本电子结构仍存在不确定性。在这里,我们介绍了在线性松饼-锡轨道方法中实现的能带结构的QSGW计算。由于用于计算$ W $的随机相位近似(RPA)中的筛选不足,因此QSGW方法通常高估了带隙。即使在考虑到通用的0.8校正因数后,我们仍发现5.4 eV量级的缺口,明显高于吸收起始的实验值。在筛查中包括晶格极化效应后,我们发现在4.9 eV的最小伽玛射线直接间隙。零点运动校正估计为另外0.2 eV,最终间隙为4.7 eV,与实验吻合得很好。发现间接间隙约小0.1 eV。对称性在$ Gamma $处标记了VBM和CBM附近的状态,表明$ {f E} perp {fb} $允许$ Gamma $的最小缺口,而$ {f E} parallel {fb允许的第一个过渡} $上升0.6 eV。预测的不同方向吸收开始的位移比实验中发现的要大。将显示计算出的吸收曲线。

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