首页> 外文期刊>The Astrophysical journal >THE INFRARED AND UV-VISIBLE SPECTRA OF POLYCYCLIC AROMATIC HYDROCARBONS CONTAINING (5, 7)-MEMBER RING DEFECTS: A THEORETICAL STUDY
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THE INFRARED AND UV-VISIBLE SPECTRA OF POLYCYCLIC AROMATIC HYDROCARBONS CONTAINING (5, 7)-MEMBER RING DEFECTS: A THEORETICAL STUDY

机译:含(5,7)-成员环缺陷的多环芳烃的红外光谱和紫外可见光谱:理论研究

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摘要

We report a theoretical investigation of the infrared (IR) spectra of polycyclic aromatic hydrocarbons (PAHs) containing (5, 7)-member ring defects based on a C48H18 model. Calculations are mostly performed using the hybrid B3LYP density functional theory (DFT) with a 6-31G(d) or 4-31G basis set. The results show that the Stone-Wales defect in PAHs can yield a strong IR band at 1448?cm–1 and a weak band at 611?cm–1, which may contribute to the UIR (unidentified infrared) bands at 6.9 μm and 16.4 μm observed in the interstellar medium. The charge effect on the IR spectra is discussed. The stability of the ring defected PAHs is also addressed by exploring the minimum energy pathway on the potential energy surface and through their UV-visible spectra, which are computed using a TDDFT method.
机译:我们报告了基于C48H18模型的含(5,7)成员环缺陷的多环芳烃(PAHs)的红外(IR)光谱的理论研究。计算主要使用具有6-31G(d)或4-31G基集的混合B3LYP密度泛函理论(DFT)进行。结果表明,多环芳烃的Stone-Wales缺陷可以在1448?cm-1处产生强IR波段,而在611?cm-1处产生弱的波段,这可能有助于6.9μm和16.4的UIR(未识别的红外)波段在星际介质中观察到的μm。讨论了电荷对红外光谱的影响。还可以通过探索势能表面上的最小能量路径并通过使用TDDFT方法计算的UV-可见光谱来解决环缺陷PAH的稳定性。

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