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Vibrational and Electronic Absorption Spectroscopy of 2,3-Benzofluorene and Its Cation

机译:2,3-苯芴及其阳离子的振动和电子吸收光谱

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Benzofluorene (C_(17)H_(12)) has been studied in argon matrices via Fourier transform infrared and UV-visible absorption spectroscopy. The analysis of the infrared absorption spectra of neutral and cationic 2,3-benzofluorene was supported by density functional theory (DFT) B3LYP/6-311+G** calculations of the harmonic-mode frequencies. Extensive time-dependent DFT calculations of the electronic vertical excitation energies with BLYP/6-31++G** and B3LYP/6-31++G** functionals/basis sets and the Casida-Salahub asymptotic correction were performed to assign the observed electronic absorption bands of the neutral species. Although the observed low-energy absorption bands are predicted well by theory, the higher-energy bands (S_n ← S_0 transitions, n ≥ 4) have been assigned only tentatively. However, the observed electronic absorption bands for the parent, singly dehydrogenated cationic and neutral species are in accord with TDDFT (BLYP/6-31G**) results. The possibility that the 2,3-benzofluorene cation contributes to the unidentified infrared (UIR) bands observed from interstellar space is discussed briefly.
机译:苯并芴(C_(17)H_(12))已通过傅立叶变换红外和紫外-可见吸收光谱法在氩气基质中进行了研究。谐波模式频率的密度泛函理论(DFT)B3LYP / 6-311 + G **计算支持中性和阳离子2,3-苯并芴的红外吸收光谱分析。使用BLYP / 6-31 ++ G **和B3LYP / 6-31 ++ G **功能/基本集以及Casida-Salahub渐近校正对电子垂直激发能进行了时间依赖性的DFT计算,从而确定了观察到中性物质的电子吸收带。尽管从理论上可以很好地预测观察到的低能吸收带,但暂仅分配了高能带(S_n←S_0跃迁,n≥4)。但是,对于母体,单个脱氢的阳离子和中性物质,观察到的电子吸收带与TDDFT(BLYP / 6-31G **)结果一致。简要讨论了2,3-苯并芴阳离子有助于从星际空间观测到的未识别的红外(UIR)波段的可能性。

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