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首页> 外文期刊>The Astrophysical journal >FAR-INFRARED SPECTROSCOPY OF CATIONIC POLYCYCLIC AROMATIC HYDROCARBONS: ZERO KINETIC ENERGY PHOTOELECTRON SPECTROSCOPY OF PENTACENE VAPORIZED FROM LASER DESORPTION
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FAR-INFRARED SPECTROSCOPY OF CATIONIC POLYCYCLIC AROMATIC HYDROCARBONS: ZERO KINETIC ENERGY PHOTOELECTRON SPECTROSCOPY OF PENTACENE VAPORIZED FROM LASER DESORPTION

机译:阳离子多环芳烃的远红外光谱:激光脱附蒸发的并五苯的零动能光电子能谱

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The distinctive set of infrared (IR) emission bands at 3.3, 6.2, 7.7, 8.6, and 11.3 μm are ubiquitously seen in a wide variety of astrophysical environments. They are generally attributed to polycyclic aromatic hydrocarbon (PAH) molecules. However, not a single PAH species has yet been identified in space, as the mid-IR vibrational bands are mostly representative of functional groups and thus do not allow one to fingerprint individual PAH molecules. In contrast, the far-IR (FIR) bands are sensitive to the skeletal characteristics of a molecule, hence they are important for chemical identification of unknown species. With an aim to offer laboratory astrophysical data for the Herschel Space Observatory, Stratospheric Observatory for Infrared Astronomy, and similar future space missions, in this work we report neutral and cation FIR spectroscopy of pentacene (C22H14), a five-ring PAH molecule. We report three IR active modes of cationic pentacene at 53.3, 84.8, and 266 μm that may be detectable by space missions such as the SAFARI instrument on board SPICA. In the experiment, pentacene is vaporized from a laser desorption source and cooled by a supersonic argon beam. We have obtained results from two-color resonantly enhanced multiphoton ionization and two-color zero kinetic energy photoelectron (ZEKE) spectroscopy. Several skeletal vibrational modes of the first electronically excited state of the neutral species and those of the cation are assigned, with the aid of ab initio and density functional calculations. Although ZEKE is governed by the Franck-Condon principle different from direct IR absorption or emission, vibronic coupling in the long ribbon-like molecule results in the observation of a few IR active modes. Within the experimental resolution of ~7?cm–1, the frequency values from our calculation agree with the experiment for the cation, but differ for the electronically excited intermediate state. Consequently, modeling of the intensity distribution is difficult and may require explicit inclusion of vibronic interactions.
机译:在各种各样的天体环境中,普遍看到3.3、6.2、7.7、8.6和11.3μm的一组独特的红外(IR)发射带。它们通常归因于多环芳烃(PAH)分子。然而,由于中红外振动带主要代表官能团,因此尚不能在空间中鉴定出单个PAH物种,因此不允许人们对单个PAH分子进行指纹识别。相反,远红外(FIR)带对分子的骨骼特征敏感,因此它们对于化学鉴定未知物种非常重要。为了向赫歇尔太空天文台,红外平流平流层天文​​台以及类似的未来太空任务提供实验室天体数据,在这项工作中,我们报告了五环PAH分子并五苯(C22H14)的中性和阳离子FIR光谱。我们报告了53.3、84.8和266μm的阳离子并五苯的三种IR激活模式,这可以通过太空任务(例如SPICA上的SAFARI仪器)检测到。在实验中,并五苯从激光解吸源中蒸发,并通过超音速氩气束冷却。我们已经从双色共振增强多光子电离和双色零动能光电子(ZEKE)光谱学中获得了结果。借助于从头算和密度泛函计算,分配了中性物质的第一个电子激发态和阳离子的几个电子激发态的骨架振动模式。尽管ZEKE受与直接红外吸收或发射不同的Franck-Condon原理支配,但长带状分子中的电子耦合导致观察到一些红外激活模式。在〜7?cm-1的实验分辨率范围内,我们计算得出的频率值与阳离子实验相符,但对于电子激发的中间态却有所不同。因此,强度分布的建模很困难,可能需要明确包含振动相互作用。

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