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A practical approach for STEM image simulation based on the FFT multislice method

机译:一种基于FFT多层方法的STEM图像仿真实用方法

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It has been demonstrated that a high-angle annular dark-field (HAADF) STEM technique gives an image resolving atomic columns. Due to the diffusion of this technique and an improvement of its resolution, a practical procedure for image simulation becomes important for a quantitative interpretation of the HAADF image. In this report a new practical scheme for a STEM image simulation is developed based on the FFT multislice algorithm. Here, a HAADF intensity due to thermal diffuse scattering (TDS) is calculated from the absorptive potential corresponding to high-angle TDS and the wave function equivalent to the propagating probe within the sample. Contrary to the commonly used Bloch wave method, a coherent bright-field intensity and a coherent HAADF intensity are also obtained straightforwardly. The HAADF image contrast calculated for GaAs is not simply proportional to Z~2 as expected from the Rutherford scattering at high-angle, and the As/Ga contrast ratio depends on the specimen thickness. This suggests that the generation of the HAADF signal is appreciably affected by the coherent dynamical scattering. The developed procedure here will have a definitive advantage over the Bloch wave approach for simulating the HAADF images expected from a defect and interface or amorphous materials, and also the HAADF image obtained by using a Cs-corrected microscope. This is because the former requires a huge super cell, while the latter needs a large objective aperture including a large number of incident beam directions.
机译:已经证明,高角度环形暗场(HAADF)STEM技术可提供图像解析原子列。由于该技术的普及及其分辨率的提高,图像模拟的实用程序对于HAADF图像的定量解释非常重要。在本报告中,基于FFT多层算法,为STEM图像仿真开发了一种新的实用方案。在此,根据与大角度TDS相对应的吸收电位和与样品内的传播探针相当的波函数,计算出由于热扩散散射(TDS)引起的HAADF强度。与常用的布洛赫波方法相反,还可以直接获得相干的明场强度和相干的HAADF强度。 GaAs计算出的HAADF图像对比度不仅仅与大角度的卢瑟福散射所期望的Z〜2成正比,而且As / Ga对比度取决于样品厚度。这表明,相干动态散射会明显影响HAADF信号的生成。此处开发的过程将比Bloch波方法具有确定的优势,该方法可用于模拟从缺陷和界面或非晶态材料获得的HAADF图像,以及通过使用Cs校正显微镜获得的HAADF图像。这是因为前者需要巨大的超级单元,而后者则需要包括大量入射光束方向的大物镜孔径。

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