首页> 美国卫生研究院文献>Philosophical transactions. Series A Mathematical physical and engineering sciences >Ab initio infrared vibrational modes for neutral and charged small fullerenes (C20 C24 C26 C28 C30 and C60)
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Ab initio infrared vibrational modes for neutral and charged small fullerenes (C20 C24 C26 C28 C30 and C60)

机译:从头算红外振动模式用于中性和带电的小富勒烯(C20C24C26C28C30和C60)

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摘要

We calculate the infrared (IR) absorption spectra using DFT B3LYP(6–311G) for a range of small closed-cage fullerenes, Cn, n=20, 24, 26, 28, 30 and 60, in both neutral and multiple positive and negative charge states. The results are of use, notably, for direct comparison with observed IR absorption in the interstellar medium. Frequencies fall typically into two ranges, with C−C stretch modes around 1100–1500 cm−1 (6.7–9.1 μm) and fullerene-specific radial motion associated with under-coordinated carbon at pentagonal sites in the range 600–800 cm−1 (12.5–16.7 μm). Notably, negatively charged fullerenes show significantly stronger absorption intensities than neutral species. The results suggest that small cage fullerenes, and notably metallic endofullerenes, may be responsible for many of the unassigned interstellar IR spectral lines.This article is part of the themed issue ‘Fullerenes: past, present and future, celebrating the 30th anniversary of Buckminster Fullerene’.
机译:我们使用DFT B3LYP(6-311G)计算一系列小的闭笼式富勒烯Cn,n = 20、24、26、28、30和60的中性和多重正红外光谱的红外吸收光谱负电荷状态。该结果尤其可用于与星际介质中观察到的IR吸收进行直接比较。频率通常分为两个范围,其中C–C拉伸模式约为1100–1500 cm −1 (6.7–9.1μm),富勒烯特定的径向运动与碳在五角形位点的配位不足有关。范围600–800 cm −1 (12.5–16.7μm)。值得注意的是,带负电荷的富勒烯比中性物种表现出明显更强的吸收强度。结果表明小笼式富勒烯,尤其是金属性富勒烯可能是许多未分配的星际红外光谱线的原因。本文是主题``富勒烯:过去,现在和未来,庆祝巴克敏斯特·富勒烯30周年''的一部分'。

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