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Title: Potential energy surface of the HNO + NO reaction. An ab initio molecular orbital study

Journal Article · · Journal of Physical Chemistry; (United States)
DOI:https://doi.org/10.1021/j100007a018· OSTI ID:6492294
; ;  [1];  [2]
  1. Emory Univ., Atlanta, GA (United States)
  2. Sandia National Lab., Livermore, CA (United States)

The potential energy surface of the HNO + NO reaction has been investigated by ab initio molecular orbital calculations at the QCISD(T)/6-311G(d,p)//UMP2/6-311G(d,p) + ZPE[UMP2/6-311G(d,p)] and Gaussian-2 (G2) levels of theory. The initial reaction step is NO association with the N atom of the HNO molecule to form the HN(O)NO intermediate, 2, overcoming the barrier 1[prime] of 9.5 kcal/mol. The reaction proceeds further by 1,3-hydrogen migration in HN(O)NO from nitrogen to oxygen via the transition state 3, which is much more favorable than 1,2-shift. This step is shown to be rate-determining, having a barrier of 21.6 kcal/mol. After the H shift, trans,cis-HONNO ([sup 2]A[double prime]) intermediate, 5a, is formed, which rearranges to trans,trans-HONNO ([sup 2]A[prime]), 7b. Finally, the latter dissociates to give the reaction products H[sub 2]O + OH. The energies of the transition states for internal rearrangements of HONNO as well as the transition state for HONNO ([sup 2]A[prime]) dissociation are calculated to be significantly lower than the rate-determining barrier for 1,3-hydrogen migration in HN(O)NO. 23 refs., 2 figs., 3 tabs.

OSTI ID:
6492294
Journal Information:
Journal of Physical Chemistry; (United States), Vol. 99:7; ISSN 0022-3654
Country of Publication:
United States
Language:
English