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Modeling formation of molecules in the interstellar medium by radical reactions with polycyclic aromatic hydrocarbons
Authors:Yenner Bentarcurt  Fernando Ruette  Morella Sánchez
Institution:1. Laboratorio de Química Computacional, Centro de Química, IVIC, Apartado 21827, Caracas 1020‐A, Venezuela;2. Departamento de Química, IUT FR Palácio, Apartado 401047, Caracas 1040‐A, Venezuela
Abstract:Adsorptions of CH°2, CH°3, NH°2, and OH° radicals and molecule formation on a partially hydrogenated surface of a polycyclic aromatic hydrocarbon (PAH) (C24H27+) were modeled. It was found that radical adsorptions are feasible with important modifications of surface bond strengths and bond distances. Adsorbed hydrogen may diffuse due to adsorbate‐surface interactions. Formations of CH4, NH3, H2O, CH3NH2, and CH3OH were studied by Eley‐Rideal (ER) and Langmuir‐Hishelwood (LH) mechanisms. Potential energetic surfaces were performed for both mechanisms and the ER presents lower reaction energy barriers than the LH one, in all cases. Parametric quantum program (CATIVIC) was employed and comparisons with DFT results were performed. © 2010 Wiley Periodicals, Inc. Int J Quantum Chem 110:2560–2572, 2010
Keywords:ISM reactions  parametric quantum method  coronene  radical reactions  surface reactions
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