Photo-fragmentation behavior of methyl- and methoxy-substituted derivatives of hexa-peri-hexabenzocoronene (HBC) cations

Q2 Physics and Astronomy Molecular Astrophysics Pub Date : 2016-11-01 DOI:10.1016/j.molap.2016.08.001
Junfeng Zhen , Pablo Castellanos , Harold Linnartz , Alexander G.G.M. Tielens
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引用次数: 8

Abstract

A systematic study, using ion trap time-of-flight mass spectrometry, is presented for the photo-fragmentation of methyl- and methoxy-substituted derivatives of HBC cations, (OCH3)6HBC+ and (CH3)4(OCH3)2HBC+. Both substituted HBC cations fragment through sequential loss of CH3CO units upon laser (595nm) irradiation, resulting in a PAH-like derivative C36H12+ and a methyl-substituted PAH derivative C44H24+, respectively. Upon ongoing irradiation, these species further fragment. For lower laser energy C44H24+ dehydrogenates and photo-fragments through CH3 and CHCH2 unit losses; for higher laser energy isomerization takes place, yielding a regular PAH-like configuration, and both stepwise dehydrogenation and C2/C2H2 loss pathways are found. C36H12+ follows largely this latter fragmentation scheme upon irradiation.

It is concluded that the photo-dissociation mechanism of the substituted PAH cations studied here is site selective in the substituted subunit. This work also shows experimental evidence that photo-fragmentation of substituted PAHs may contribute to the formation in space of smaller species that are normally considered to form by merging atoms and molecules.

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六-邻六苯并冠烯(HBC)阳离子甲基和甲氧基取代衍生物的光断裂行为
采用离子阱飞行时间质谱法对HBC阳离子的甲基和甲氧基取代衍生物(OCH3)6HBC+和(CH3)4(OCH3)2HBC+进行了系统的光破碎研究。在激光(595nm)照射下,这两种取代的HBC阳离子通过CH3CO单元的连续损失而分裂,分别产生类多环芳烃衍生物C36H12+和甲基取代的多环芳烃衍生物C44H24+。在持续的照射下,这些物种进一步分裂。对于较低的激光能量,C44H24+通过CH3和CHCH2单位损失脱氢和光碎片;当激光能量较高时,发生异构化,生成规则的类多环芳烃构型,并发现了逐步脱氢和C2/C2H2损失途径。辐照后C36H12+主要遵循后一种破碎方案。结果表明,本文研究的取代多环芳烃阳离子的光解离机制在取代亚基上具有选择性。这项工作还显示了实验证据,取代多环芳烃的光碎片可能有助于在空间中形成较小的物种,通常被认为是由原子和分子合并形成的。
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Molecular Astrophysics
Molecular Astrophysics ASTRONOMY & ASTROPHYSICS-
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期刊介绍: Molecular Astrophysics is a peer-reviewed journal containing full research articles, selected review articles, and thematic issues. Molecular Astrophysics is a new journal where researchers working in planetary and exoplanetary science, astrochemistry, astrobiology, spectroscopy, physical chemistry and chemical physics can meet and exchange their ideas. Understanding the origin and evolution of interstellar and circumstellar molecules is key to understanding the Universe around us and our place in it and has become a fundamental goal of modern astrophysics. Molecular Astrophysics aims to provide a platform for scientists studying the chemical processes that form and dissociate molecules, and control chemical abundances in the universe, particularly in Solar System objects including planets, moons, and comets, in the atmospheres of exoplanets, as well as in regions of star and planet formation in the interstellar medium of galaxies. Observational studies of the molecular universe are driven by a range of new space missions and large-scale scale observatories opening up. With the Spitzer Space Telescope, the Herschel Space Observatory, the Atacama Large Millimeter/submillimeter Array (ALMA), NASA''s Kepler mission, the Rosetta mission, and more major future facilities such as NASA''s James Webb Space Telescope and various missions to Mars, the journal taps into the expected new insights and the need to bring the various communities together on one platform. The journal aims to cover observational, laboratory as well as computational results in the galactic, extragalactic and intergalactic areas of our universe.
期刊最新文献
Chemistry on Interstellar Grain Surfaces Molecular Emission and Absorption Gas Phase Chemical Processes Diffuse Clouds Molecular Spectroscopy
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