Department of Physics, University of Washington, Seattle, WA 98195, USA.
Phys Chem Chem Phys. 2010 Jun 7;12(21):5503-13. doi: 10.1039/b926434e. Epub 2010 May 6.
We briefly review our implementation of the real-space Green's function (RSGF) approach for calculations of X-ray spectra, focusing on recently developed parameter free models for dominant many-body effects. Although the RSGF approach has been widely used both for near edge (XANES) and extended (EXAFS) ranges, previous implementations relied on semi-phenomenological methods, e.g., the plasmon-pole model for the self-energy, the final-state rule for screened core hole effects, and the correlated Debye model for vibrational damping. Here we describe how these approximations can be replaced by efficient ab initio models including a many-pole model of the self-energy, inelastic losses and multiple-electron excitations; a linear response approach for the core hole; and a Lanczos approach for Debye-Waller effects. We also discuss the implementation of these models and software improvements within the FEFF9 code, together with a number of examples.
我们简要回顾了我们在计算 X 射线谱中使用实空间格林函数 (RSGF) 方法的情况,重点介绍了最近开发的用于主要多体效应的无参数模型。尽管 RSGF 方法已广泛用于近边 (XANES) 和扩展 (EXAFS) 范围,但以前的实现依赖于半唯象方法,例如自能的等离子体极点模型、屏蔽芯孔效应的终态规则以及用于振动阻尼的相关德拜模型。在这里,我们描述了如何用包括自能的多极模型、非弹性损耗和多电子激发;芯孔的线性响应方法;以及德拜-沃勒效应的兰索斯方法等有效从头算模型来替代这些近似。我们还讨论了这些模型的实现以及 FEFF9 代码中的软件改进,以及一些例子。