IO(X2π)-Ar cluster: ab initio potential energy surface and dynamical computations

被引:2
作者
Marzouk, S. [1 ,2 ]
Ajili, Y. [3 ]
Lique, F. [4 ]
Ben El Hadj Rhouma, M. [1 ]
Al Mogren, M. Mogren [5 ]
Hochlaf, M. [2 ]
机构
[1] Univ Monastir, Inst Preparatoire Etud Ingn Monastir, Lab Rech Etud Milieux Ionise & Reactifs EMIR, Monastir, Tunisia
[2] Univ Gustave Eiffel, COSYS LISIS, 5 Bd Descartes 77454, Champs Sur Marne, France
[3] Univ Tunis El Manar, LSAMA, Tunis, Tunisia
[4] Univ Havre, CNRS, LOMC UMR 6294, 25 Rue Philippe Lebon,BP 1123, F-76063 Le Havre, France
[5] King Saud Univ, Dept Chem, Fac Sci, POB 2455, Riyadh 11451, Saudi Arabia
关键词
ABSORPTION CROSS-SECTIONS; INELASTIC-COLLISIONS; IODINE OXIDE; PHOTOELECTRON-SPECTROSCOPY; IO RADICALS; BASIS-SETS; BRO; SCATTERING; KINETICS; STATE;
D O I
10.1039/c9cp05310g
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
Iodine oxide (IO) is an important tropospheric molecule. In the present paper, we mapped the potential energy surfaces (PESs) of the doubly degenerate IO(X-2 pi)-Ar van der Waals system using single- and double-excitation coupled cluster approaches with non-iterative perturbation treatment of triple excitations [RCCSD(T)] extrapolated to the complete basis set (CBS) limit. In addition to bent local minima, we identified a linear Ar-IO complex as a global minimum. Afterwards, we performed scattering calculations on these PESs, considering the non-zero spin-orbit contribution and the Renner-Teller effect. The integral cross-sections exhibit an oscillatory structure vs. the final rotational state, as already observed for the NO(X-2 pi)-Ar system. Moreover, computations reveal that the Ar-IO complex is stable toward dissociation into IO and Ar. Therefore, it can be found in the atmosphere and participates in iodine compound physical chemical processes occurring there.
引用
收藏
页码:740 / 747
页数:8
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