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首页> 外文期刊>Journal of structural chemistry >X-RAY EMISSION AND ABSORPTION SPECTRA OF Cr(CO)(6): A COMPARISON OF QUANTUM-CHEMICAL AND FULL MULTIPLE SCATTERING CALCULATIONS WITH EXPERIMENT
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X-RAY EMISSION AND ABSORPTION SPECTRA OF Cr(CO)(6): A COMPARISON OF QUANTUM-CHEMICAL AND FULL MULTIPLE SCATTERING CALCULATIONS WITH EXPERIMENT

机译:Cr(CO)(6)的X射线发射和吸收光谱:量子化学和全散射分析与实验的比较

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摘要

The full multiple scattering procedure using the extended continuum approximation and the single semiempirical muffin-tin (MT) potential gave X-ray emission spectra and the CrK absorption spectrum of Cr(CO)(6), which were in good agreement with experiment. The bound states above the NIT zero become the resonance states corresponding to the poles of the Green function in the lower semi-plane of the complex plane of energy. A procedure for determining the parameters or the poles was developed. A group of poles close to the real line were isolated; their number equals the number of molecular orbitals generated by well-atomized atomic orbitals. These poles completely determine the Fine structure of the emission spectra and the first narrow peak in the absorption spectrum. Their energies were close to those of molecular orbitals found at the DFT level of theory, but were in worse agreement with the results of Hartree-Fock calculations. The Hartree Fock method gave worse agreement with the experimental emission spectra than full multiple scattering and DFT. The fine structure of the region after the first narrow peak in the absorption spectrum is also mainly determined by the contributions from the poles, but these poles are farther from the real line than the poles corresponding to molecular orbitals. Keywords: full multiple scattering method, density functional theory, Hartree-Fock method, X-ray emission spectra, X-ray absorption spectra, electronic Structure, chromium hexacarbonyl.
机译:使用扩展连续近似法和单半经验性松饼-锡(MT)势进行的全多次散射过程给出了Cr(CO)(6)的X射线发射光谱和CrK吸收光谱,与实验吻合良好。 NIT零上方的束缚状态成为与能量复平面的下半平面中的格林函数的极点相对应的共振状态。开发了确定参数或极点的程序。靠近实线的一组极点被隔离了。它们的数目等于由原子化良好的原子轨道产生的分子轨道的数目。这些极点完全确定了发射光谱的精细结构和吸收光谱中的第一个窄峰。它们的能量接近在DFT理论水平上发现的分子轨道的能量,但与Hartree-Fock计算的结果更不一致。与完全多重散射和DFT相比,Hartree Fock方法与实验发射光谱的一致性更差。吸收光谱中第一个窄峰之后的区域的精细结构也主要取决于极点的贡献,但是这些极点比对应于分子轨道的极点更远离实线。关键词:全多重散射法,密度泛函理论,Hartree-Fock方法,X射线发射光谱,X射线吸收光谱,电子结构,六羰基铬。

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