Superhydrogenated PAHs: Catalytic Formation of H2

J. Thrower, L. Nilsson, B. Jørgensen, S. Baouche, R. Balog, A. Luntz, I. Stensgaard, E. Rauls, L. Hornekær
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引用次数: 4

Abstract

The possible role of neutral PAHs as catalysts for H2 forma- tion in the interstellar medium is investigated by a combined exper- imental and density function theory study of the superhydrogenation of coronene (C24H12). The calculations suggest efficient hydrogenation of both edge and centre sites, along with competing abstraction reac- tions to form H2 in a series of catalytic cycles. Scanning tunneling microscopy and thermal desorption measurements have been used to provide direct evidence of the formation of superhydrogenated coronene as a result of exposure to D atoms. Lower limit estimates for the cross- sections of 1.8×10 �17 ,5 .5×10 �18 and 1.1×10 �18 cm 2 for the formation of singly, doubly and triply hydrogenated coronene are derived. The results suggest that superhydrogenated PAHs may play an important role in H2 formation in the ISM.
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超氢化多环芳烃:催化生成H2
通过对冕烯(C24H12)超氢化反应的实验和密度泛函理论相结合的研究,探讨了中性多环芳烃在星际介质中催化H2生成的可能作用。计算结果表明,在一系列催化循环中,边缘和中心位置都发生了有效的氢化反应,同时还发生了相互竞争的萃取反应,形成H2。扫描隧道显微镜和热解吸测量已经被用来提供由于暴露于D原子而形成超氢化冕烯的直接证据。推导了1.8×10′17、5 .5×10′18和1.1×10′18 cm 2形成单氢化、双氢化和三氢化冕烯截面的下限估计。结果表明,过氢化多环芳烃可能在ISM中H2的形成中起重要作用。
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