Ab Initio Calculation of UV-Vis Absorption Spectra of a Single Molecule Chlorophyll a: Comparison Study between RHF/CIS, TDDFT, and Semi-Empirical Methods

V. Suendo, S. Viridi
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引用次数: 21

Abstract

Chlorophyll a is one the most abundant pigment on Earth that responsible for trapping the light energy to perform photosynthesis in green plants. This molecule is a metal-complex that consists of a porphyrin ring with high symmetry that acts as ligands with magnesium as the central ion. Chlorophyll a has been studied for many years from different point of views for both experimental and theoretical interests. In this study, the restricted Hartree-Fock configuration interaction single (RHF/CIS), time-dependent density functional theory (TDDFT) and some semi-empirical methods (CNDO/s and ZINDO) calculations were carried out and compared to reconstruct the UV-Vis absorption spectra of chlorophyll a. In some extend, the calculation results based on a single molecule calculation were succeeded to reconstruct the absorption spectra but required to be scaling to match the experimental one. Different computational methods (ab initio and semi-empirical) exhibit the differences in the energy correction factor and the presence of transition states, however, still conserve the main spectral features. In general, the semi-empirical methods provide a better energy scaling factor, which means closer to the experimental one. However, they lack of fine features or vertical transitions with respect to the experimental spectra. The ab initio calculations result more complete features than the semi-empirical methods, especially the TDDFT with high level of basis sets that provides a good accuracy in transition energies. The contribution of ground states and excited states orbitals in the main vertical transitions is discussed based on orbital structure. This might gives a new perspective to explain the energy transfer phenomena in the absorption processes that related to the function of chlorophyll a as a light-harvesting antenna.
单分子叶绿素a紫外-可见吸收光谱的从头计算:RHF/CIS、TDDFT和半经验方法的比较研究
叶绿素a是地球上最丰富的色素之一,在绿色植物中负责捕获光能进行光合作用。这种分子是一种金属复合物,由一个高度对称的卟啉环组成,以镁为中心离子作为配体。叶绿素a已经从实验和理论两方面进行了多年的研究。本研究通过限制Hartree-Fock构型相互作用单谱(RHF/CIS)、时变密度泛函数理论(TDDFT)和一些半经验方法(CNDO/s和ZINDO)计算进行对比,重建叶绿素a的紫外-可见吸收光谱。在一定程度上,基于单分子计算的计算结果成功重建了叶绿素a的吸收光谱,但需要进行缩放以匹配实验结果。不同的计算方法(从头计算和半经验计算)在能量校正因子和过渡态的存在方面表现出差异,但仍然保留了主要的光谱特征。一般来说,半经验方法提供了更好的能量标度因子,这意味着更接近实验值。然而,相对于实验光谱,它们缺乏精细的特征或垂直跃迁。与半经验方法相比,从头开始计算得到的特征更完整,特别是具有高水平基集的TDDFT在跃迁能量上提供了良好的精度。从轨道结构出发,讨论了基态轨道和激发态轨道在主要垂直跃迁中的作用。这可能为解释与叶绿素a作为光收集天线的功能有关的吸收过程中的能量转移现象提供了一个新的视角。
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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