Ab initio molecular orbital study of potential energy surface for the NH+NO2 reaction
1994; American Institute of Physics; Volume: 101; Issue: 5 Linguagem: Inglês
10.1063/1.467509
ISSN1520-9032
AutoresAlexander M. Mebel, Keiji Morokuma, M. C. Lin,
Tópico(s)Ammonia Synthesis and Nitrogen Reduction
ResumoThe reaction of NH with NO2, which can produce N2O+OH and HNO+NO by two distinct reaction paths, has been studied by ab initio molecular orbital calculations. The first reaction path taking place by initial N–N association forms an intermediate HNNO2, 1, which undergoes H-migration yielding NN(O)OH, 3, before reaching the N2O+OH product. The transition state 2 for the rate-determining 1→3 rearrangement, with the activation barrier of 30 kcal/mol at the G2-level of calculation, lies below the energy of the reactants. The O migration for the HNNO2 1 intermediate to produce HNO+NO is inaccessible at low temperatures due to the presence of a high migration barrier. The second path via initial N–O association forms an intermediate HNONO, 9, which is expected to dissociate readily to HNO+NO via a loose transition state lying 24 kcal/mol below the reactants. Since the initial N–N and N–O association reactions effectively occur with no barriers, the overall activation energy for NH+NO2 is expected to be negligible or slightly negative as was found experimentally.
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