Infrared Cooling in an Anharmonic Cascade Framework: 2-Cyanoindene, the Smallest Cyano-PAH Identified in Taurus Molecular Cloud-1.

IF 2.9 3区 化学 Q2 CHEMISTRY, MULTIDISCIPLINARY
ACS Earth and Space Chemistry Pub Date : 2025-02-04 eCollection Date: 2025-02-20 DOI:10.1021/acsearthspacechem.4c00381
Mark H Stockett, Vincent J Esposito, Eleanor K Ashworth, Ugo Jacovella, James N Bull
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Abstract

Infrared (IR) cooling of polycyclic aromatic hydrocarbon (PAH) molecules is a major radiative stabilization mechanism of PAHs present in space and is the origin of the aromatic infrared bands (AIBs). Here, we report an anharmonic cascade model in a master equation framework to model IR emission rates and emission spectra of energized PAHs as a function of internal energy. The underlying (simple harmonic cascade) framework for fundamental vibrations has been developed through the modeling of cooling rates of PAH cations and other carboneaous ions measured in electrostatic ion storage ring experiments performed under "molecular cloud in a box" conditions. The anharmonic extension is necessitated because cyano-PAHs, recently identified in Taurus Molecular Cloud-1 (TMC-1), exhibit strong anharmonic couplings, which make substantial contributions to the IR emission dynamics. We report an experimental mid-IR (650-3200 cm-1) absorption spectrum of 2-cyanoindene (2CNI), which is the smallest cyano-PAH that has been identified in TMC-1 and model its IR cooling rates and emission properties. The mid-IR absorption spectrum is reasonably described by anharmonic calculations at the B3LYP/N07D level of theory that include resonance polyad matrices, although the CN-stretch mode frequency continues to be difficult to describe. The anharmonic cascade framework can be readily applied to other neutral or charged PAHs and is also readily extended to include competing processes, such as recurrent fluorescence and isomerization.

非谐波级联框架中的红外冷却:金牛座分子云-1 中发现的最小的氰基-PAH-2-氰基茚。
多环芳烃(PAH)分子的红外冷却是多环芳烃在空间中存在的主要辐射稳定机制,是芳烃红外带(AIBs)的来源。在这里,我们报告了一个主方程框架下的非谐波级联模型,该模型将激活多环芳烃的红外发射率和发射光谱作为内能的函数进行建模。基本振动的底层(简谐级联)框架已经通过模拟在“盒子里的分子云”条件下进行的静电离子存储环实验中测量的多环芳烃阳离子和其他碳离子的冷却速率而开发出来。由于最近在金牛座分子云-1 (TMC-1)中发现的氰基多环芳烃具有强的非谐波耦合,这对红外发射动力学有重要贡献,因此必须进行非谐波扩展。我们报道了在TMC-1中发现的最小的氰基多环芳烃- 2-氰胺(2CNI)的中红外(650-3200 cm-1)吸收光谱,并模拟了其红外冷却速率和发射特性。中红外吸收光谱可以通过B3LYP/N07D理论水平的非谐波计算来合理地描述,其中包括共振多阵矩阵,尽管cn -拉伸模式频率仍然难以描述。非调和级联框架可以很容易地应用于其他中性或带电的多环芳烃,也很容易扩展到包括竞争过程,如反复荧光和异构化。
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来源期刊
ACS Earth and Space Chemistry
ACS Earth and Space Chemistry Earth and Planetary Sciences-Geochemistry and Petrology
CiteScore
5.30
自引率
11.80%
发文量
249
期刊介绍: The scope of ACS Earth and Space Chemistry includes the application of analytical, experimental and theoretical chemistry to investigate research questions relevant to the Earth and Space. The journal encompasses the highly interdisciplinary nature of research in this area, while emphasizing chemistry and chemical research tools as the unifying theme. The journal publishes broadly in the domains of high- and low-temperature geochemistry, atmospheric chemistry, marine chemistry, planetary chemistry, astrochemistry, and analytical geochemistry. ACS Earth and Space Chemistry publishes Articles, Letters, Reviews, and Features to provide flexible formats to readily communicate all aspects of research in these fields.
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