Linear Scaling Approach for Optical Excitations Using Maximally Localized Wannier Functions

IF 4.9 3区 材料科学 Q2 MATERIALS SCIENCE, MULTIDISCIPLINARY JPhys Materials Pub Date : 2023-11-06 DOI:10.1088/2515-7639/ad06cd
Konrad Merkel, Frank Ortmann
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Abstract

Abstract We present a theoretical method for calculating optical absorption spectra based on maximally localized Wannier functions, which is suitable for large periodic systems. For this purpose, we calculate the exciton Hamiltonian, which determines the Bethe–Salpeter equation for the macroscopic polarization function and optical absorption characteristics. The Wannier functions are specific to each material and provide a minimal and therefore computationally convenient basis. Furthermore, their strong localization greatly improves the computational performance in two ways: first, the resulting Hamiltonian becomes very sparse and, second, the electron–hole interaction terms can be evaluated efficiently in real space, where large electron–hole distances are handled by a multipole expansion. For the calculation of optical spectra we employ the sparse exciton Hamiltonian in a time-domain approach, which scales linearly with system size. We demonstrate the method for bulk silicon—one of the most frequently studied benchmark systems—and envision calculating optical properties of systems with much larger and more complex unit cells, which are presently computationally prohibitive.
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利用最大局域万尼尔函数的光激发线性标度方法
提出了一种基于极大定域万尼尔函数的光学吸收光谱计算理论方法,该方法适用于大周期系统。为此,我们计算了激子哈密顿量,该哈密顿量决定了宏观偏振函数和光吸收特性的Bethe-Salpeter方程。万尼尔函数是特定于每种材料,并提供了一个最小的,因此计算方便的基础。此外,它们的强局域性在两个方面极大地提高了计算性能:第一,得到的哈密顿量变得非常稀疏;第二,电子-空穴相互作用项可以在实际空间中有效地评估,其中大的电子-空穴距离由多极展开处理。对于光学光谱的计算,我们采用时域方法中的稀疏激子哈密顿量,该方法与系统大小成线性比例。我们展示了块状硅(最常被研究的基准系统之一)的方法,并设想计算具有更大更复杂单元的系统的光学特性,这在目前的计算中是禁止的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
JPhys Materials
JPhys Materials Physics and Astronomy-Condensed Matter Physics
CiteScore
10.30
自引率
2.10%
发文量
40
审稿时长
12 weeks
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