4.4 微米左右的氯化萘延伸在氰基多环芳烃的红外吸收光谱中占主导地位

Q1 Earth and Planetary Sciences Monthly Notices of the Royal Astronomical Society: Letters Pub Date : 2024-05-06 DOI:10.1093/mnrasl/slae037
V. J. Esposito, R. C. Fortenberry, C. Boersma, A. Maragkoudakis, L. Allamandola
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引用次数: 0

摘要

非谐波量子化学计算显示,在氰基取代的多环芳烃(CN-PAHs)氰基萘、氰基蒽、氰基菲和氰基芘的吸收光谱的 4.3-4.5 μm 波段中,存在一个较强的窄带(宽度 = 0.075 μm)。这种具有强烈红外线的窄窗口意味着,各种形状和大小的 CN-PAHs 在这一区域的波长和强度变化都很小。因此,这一波段可用作 CN-PAHs 的示踪剂。构成该频带的明显特征是由 CN 伸展基带和各种组合带组成的混合振动状态,包括面内 CH 弯曲、CC 骨架弯曲和 CC 骨架呼吸运动。通过非谐波耦合,CN 基本伸展的超大本征强度被重新分配到附近的状态,使用二阶振动扰动理论和共振多矩阵时,可以很容易地捕捉到这一点。这种强度的重新分布导致了复杂的光谱。该波长区域的高强度波段可能是 JWST NIRSpec 最近观测到的基线连续波和起伏宏观结构的组成部分。
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CN stretches around 4.4 microns dominate the IR absorption spectra of cyano-polycyclic aromatic hydrocarbons
Anharmonic quantum chemical computations reveal a strong, narrow (width = 0.075 μm) band in the 4.3–4.5 μm region of the absorption spectra of the cyano-substituted polycyclic aromatic hydrocarbons (CN-PAHs) cyanonaphthalene, cyanoanthracene, cyanophenanthrene, and cyanopyrene. This narrow window with intense IR lines implies that CN-PAHs of various shapes and sizes offer little variation in both wavelength and intensity in this region. Subsequently, this band can be used as a tracer for CN-PAHs. The distinct features making up the band are assigned to mixed vibrational states consisting of the CN stretch fundamental and various combination bands, including in-plane CH bends, CC skeletal bends, and CC skeletal breathing motions. The extraordinarily large intrinsic intensity of the fundamental CN stretch is redistributed to nearby states via anharmonic coupling, which is readily captured when using second order vibrational perturbation theory with resonance polyad matrices. This redistribution of intensity leads to a complex spectrum. The intense bands in this wavelength region may contribute to the baseline continuum and undulating macroscopic structure seen in recent JWST NIRSpec observations.
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来源期刊
Monthly Notices of the Royal Astronomical Society: Letters
Monthly Notices of the Royal Astronomical Society: Letters Earth and Planetary Sciences-Space and Planetary Science
CiteScore
8.80
自引率
0.00%
发文量
136
期刊介绍: For papers that merit urgent publication, MNRAS Letters, the online section of Monthly Notices of the Royal Astronomical Society, publishes short, topical and significant research in all fields of astronomy. Letters should be self-contained and describe the results of an original study whose rapid publication might be expected to have a significant influence on the subsequent development of research in the associated subject area. The 5-page limit must be respected. Authors are required to state their reasons for seeking publication in the form of a Letter when submitting their manuscript.
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