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arXiv 1107.2073cond-mat.str-el
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GW +U实空间格林函数计算X射线谱

GW+U real-space Green's function calculations of x-ray spectra

Towfiq Ahmed, J. J. Kas, J. J. Rehr

摘要:

在实空间格林函数计算的X射线光谱的哈伯德模型实现使用一个有效的自适应能量从LSDA+U方法Anisimov等人。这种自能包括一个依赖于能量的多极近似GW自能与添加剂校正由于现场库仑排斥之间的部分填充的局域电子状态。这导致了GW+U的方法,它提供了一个有效的程序来考虑局部相关效应的X射线光谱。计算了MnO、NiO和La_(2-x)Sr_xCuO_4(LSCO)的自旋和角动量投影态密度,MnO和NiO中氧原子的K边X射线谱,以及未掺杂LSCO的空电子态和O的K边谱。该方法被发现产生合理的协议与实验。

英文摘要:

The Hubbard model is implemented in real-space Green's function calculations of x-ray spectra using an effective self-energy adapted from the LSDA+U method of Anisimov et al. This self-energy consists of an energy-dependent many-pole approximation to the GW self-energy with an additive correction due to on-site Coulomb repulsion among the partially filled localized-electron states. This leads to a GW+U approach which provides an efficient procedure to account for local correlation effects on x-ray spectra. Results are presented for the spin and angular momentum projected density of states of MnO, NiO, and La_(2-x)Sr_xCuO_4 (LSCO), for the K-edge x-ray spectra of O atoms in MnO and NiO, and the unoccupied electronic states and O K-edge spectra of undoped LSCO. The method is found to yield reasonable agreement with experiment.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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