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Theoretical survey of the NH+CH3 potential energy surface in relation to Titan atmospheric chemistry
Authors:P Redondo  Y Ellinger
Institution:a Departamento de Quimica Fisica, Facultad de Ciencias, Universidad de Valladolid, 47005 Valladolid, Spain
b LETMEX (USM 205), Museum National d’Histoire Naturelle, Paris
c LCT (UMR-CNRS 7616), Université Pierre et Marie Curie, 4 Place Jussieu 75252 Paris cedex, France
Abstract:This paper looks at the possibilities opened by reaction of NH with methyl radical. A general survey of the potential surface by ab initio Möller-Plesset (MP2) and density functional theory has been performed, including determination of transition states on the pathways considered and vibrational analysis of all stationary points. Energetical data have been obtained using coupled cluster molecular orbital methods (CCSD(T)). It is shown that HCN is not formed from these starting reactants, but that CH2double bond; length as m-dashNH, a possible precursor of tholins and of prebiotic compounds through hydration is the major product.
Keywords:Astrochemistry  Quantum chemistry  Titan chemistry
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