Reaction dynamics of Mg(3s3p P-1(1)) with CH4: Elucidation of reaction pathways for the MgH product by the measurement of temperature dependence and the calculation of ab initio potential energy surfaces

被引:18
|
作者
Liu, DK
Ou, YR
Lin, KC
机构
[1] NATL TAIWAN UNIV,DEPT CHEM,TAIPEI 10764,TAIWAN
[2] NATL TAIWAN UNIV,INST ATOM & MOLEC SCI,TAIPEI 10764,TAIWAN
来源
JOURNAL OF CHEMICAL PHYSICS | 1996年 / 104卷 / 04期
关键词
D O I
10.1063/1.470794
中图分类号
O64 [物理化学(理论化学)、化学物理学];
学科分类号
070304 ; 081704 ;
摘要
Using a pump-probe method, we have obtained the nascent bimodal rotational distribution of MgH (v ''=0 and 1) products formed in the reaction of Mg(3s3p P-1(1)) with CH4. The low-N component of the distribution in the v ''=0 state is much larger than that in the v ''=1 state, whereas the high-N component in the v ''=0 state is roughly equivalent to that in the v ''=1 state. The MgH (v ''=0) rotational distributions at three temperatures, 770, 830, and 880 K, were measured. The bimodal distribution does not change with temperature within a small experimental error. The findings suggest that the bimodal nature results from the same process, supporting a mechanism of Mg insertion into the C-H bond, irrespective of the geometry of the entrance approach. The result is consistent with that of Kleiber et al. using the far-wing scattering technique, and is supported by Chaquin et al.'s theoretical calculations. We also calculated two-dimensional potential energy surfaces for the excited and ground states of the reaction system. The calculation suggests that two possible trajectories are responsible for the production of MgH following a nonadiabatic transition. One trajectory, weakly dependent on the bending angle of H-Mg-CH3, is related to formation of the low-N component. The other trajectory evolves through a linear geometry of the intermediate complex prior to dissociation, causing a strong anisotropy in the PES. This second trajectory corresponds to the population of rotationally and vibrationally hot states. An alternative explanation of the low-N distribution is also discussed. (C) 1996 American Institute of Physics.
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收藏
页码:1370 / 1379
页数:10
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