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氢化质子化多环芳烃(PAH)分子电子光谱的含时密度泛函理论计算:对弥散星际带起源的启示?

TD-DFT calculations of electronic spectra of hydrogenated protonated polycyclic aromatic hydrocarbon (PAH) molecules: implications for the origin of the diffuse interstellar bands?

作者信息

Hammonds Mark, Pathak Amit, Sarre Peter J

机构信息

School of Chemistry, The University of Nottingham, University Park, Nottingham, UK NG7 2RD.

出版信息

Phys Chem Chem Phys. 2009 Jun 14;11(22):4458-64. doi: 10.1039/b903237a. Epub 2009 Apr 21.

Abstract

We report the application of time-dependent density functional theory (TD-DFT) to the calculation of electronic spectra of hydrogenated protonated polycyclic aromatic hydrocarbon (PAH) molecules. The hydrogen atoms lie on the periphery of the PAH structure and those considered here may be written Hn-HPAH+, where n is even. It is found, in common with protonated PAH molecules, HPAH+, that some of the electronic transitions fall in the visible spectral region. The implications of the results are discussed in the context of the long-standing enigmatic astronomical problem of the diffuse interstellar absorption bands.

摘要

我们报道了含时密度泛函理论(TD-DFT)在氢化质子化多环芳烃(PAH)分子电子光谱计算中的应用。氢原子位于PAH结构的外围,这里所考虑的分子可写成Hn-HPAH+,其中n为偶数。与质子化PAH分子HPAH+一样,发现一些电子跃迁落在可见光谱区域。我们在长期存在的弥漫星际吸收带这一神秘天文问题的背景下讨论了这些结果的意义。

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