Ab initio MO study of the triplet C3H4 potential energy surface and the reaction of C(P-3(j)) with ethylene, C2H4

Citation
Tn. Le et al., Ab initio MO study of the triplet C3H4 potential energy surface and the reaction of C(P-3(j)) with ethylene, C2H4, J PHYS CH A, 105(10), 2001, pp. 1847-1856
Citations number
82
Categorie Soggetti
Physical Chemistry/Chemical Physics
Journal title
JOURNAL OF PHYSICAL CHEMISTRY A
ISSN journal
10895639 → ACNP
Volume
105
Issue
10
Year of publication
2001
Pages
1847 - 1856
Database
ISI
SICI code
1089-5639(20010315)105:10<1847:AIMSOT>2.0.ZU;2-A
Abstract
The potential energy surface for the reaction of C(P-3(j)) with ethylene, C 2H4((XAg)-Ag-1), has been investigated using the G2M method. Structures of the stationary points and transition states for various isomerization and d issociation pathways of triplet C3H4 have been studied. The results show th at at the initial step of the C(P-3(j)) + C2H4(X(1)A(g)) reaction carbon at om attacks the pi -orbital of the C2H4 molecule yielding cyclopropylidene i i without entrance barrier, ii then isomerizes to the triplet allene i3 via ring opening. The latter either splits a hydrogen atom producing the propa rgyl radical p3 + H or undergoes a 1,2-H shift to vinylmethylene, which in turn gives H2CCCH (p3) + H. The propargyl radical is concluded to be a near ly exclusive product of the C(P-3) + C2H4 reaction. At the internal energy of 9.2 kcal/mol above the reactants level, Rice-Ramsperger-Kassel-Marcus ca lculations show about 93% of H2CCCH comes from fragmentation of triplet all ene and 7% from vinylmethylene. The formation of CH2(B-3(1)) + C2H2 via the vinylmethylene intermediate gives only 2% of the reaction products; the fo rmation of triplet C3H2 + Hz is unlikely. This study completes a comprehens ive investigation of the C(P-3(j)) + C2H4 reaction; its rate constants have been measured in a broad temperature range from 10 to 800 K, the reaction dynamics has been unraveled by crossed molecular beam experiments, and the reaction potential energy surface has now been explored by ab initio calcul ations.