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Ab initio calculation of UV-Vis absorption spectra of a single molecule chlorophyll a: Comparison study between RHF/CIS, TDDFT, and semi-empirical methods

机译:从头计算单分子的UV-Vis吸收光谱   叶绿素a:RHF / CIs,TDDFT和半经验的比较研究   方法

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摘要

Chlorophyll a is one the most abundant pigment on Earth that responsible fortrapping the light energy to perform photosynthesis in green plants. Thismolecule is a metal-complex that consists of a porphyrin ring with highsymmetry that acts as ligands with magnesium as the central ion. Chlorophyll ahas been studied for many years from different point of views for bothexperimental and theoretical interests. In this study, the restrictedHartree-Fock configuration interaction single (RHF/CIS), time-dependent densityfunctional theory (TDDFT) and some semi-empirical methods (CNDO/s and ZINDO)calculations were carried out and compared to reconstruct the UV-Vis absorptionspectra of chlorophyll a. In some extend, the calculation results based on asingle molecule calculation were succeeded to reconstruct the absorptionspectra but required to be scaling to match the experimental one. Differentcomputational methods (ab initio and semi-empirical) exhibit the differences inthe energy correction factor and the presence of transition states, however,still conserve the main spectral features. In general, the semi-empiricalmethods provide a better energy scaling factor, which means closer to theexperimental one. However, they lack of fine features or vertical transitionswith respect to the experimental spectra. The ab initio calculations resultmore complete features than the semi-empirical methods, especially the TDDFTwith high level of basis sets that provides a good accuracy in transitionenergies. The contribution of ground states and excited states orbitals in themain vertical transitions is discussed based on orbital structure. This mightgives a new perspective to explain the energy transfer phenomena in theabsorption processes that related to the function of chlorophyll a as alight-harvesting antenna.
机译:叶绿素a是地球上最丰富的色素之一,负责捕获光能以在绿色植物中进行光合作用。该分子是由具有高对称性的卟啉环组成的金属络合物,该卟啉环以镁为中心离子充当配体。为了实验和理论上的利益,从不同的角度对叶绿素进行了多年的研究。在这项研究中,进行了受限Hartree-Fock配置相互作用单(RHF / CIS),时变密度泛函理论(TDDFT)和一些半经验方法(CNDO / s和ZINDO)计算,并进行了比较以重建UV-Vis叶绿素的吸收光谱。在某种程度上,基于单分子计算的计算结果已成功重建了吸收光谱,但需要按比例缩放以匹配实验值。不同的计算方法(从头算和半经验的)显示出能量校正因子和过渡态的存在差异,但是仍然保留了主要的光谱特征。通常,半经验方法提供了更好的能量比例因子,这意味着更接近于实验方法。但是,它们相对于实验光谱缺乏精细的特征或垂直过渡。从头算的结果比半经验方法具有更完整的功能,尤其是具有高基集的TDDFT,它在过渡能量方面具有良好的准确性。基于轨道结构,讨论了基态和激发态轨道在主要垂直跃迁中的贡献。这可能为解释吸收过程中的能量转移现象提供了新的视角,这些现象与叶绿素a作为集光天线的功能有关。

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