The Existence Regions for Direct Three-Body Recombination of Cesium and Bromide Ions in the Presence of Krypton, Xenon, and Mercury Atoms

被引:1
作者
Azriel, V. M. [1 ]
Akimov, V. M. [1 ]
Ermolova, E. V. [1 ]
Kabanov, D. B. [1 ]
Kolesnikova, L. I. [1 ]
Rusin, L. Yu. [1 ]
Sevryuk, M. B. [1 ]
机构
[1] Russian Acad Sci, Semenov Fed Res Ctr Chem Phys, Talrose Inst Energy Problems Chem Phys, Moscow 119334, Russia
关键词
direct three-body recombination of ions; trajectory simulation; recombination region; opacity function; impact parameter; orientation angles; collision energies; COLLISION-INDUCED DISSOCIATION; DYNAMICS; MECHANISMS;
D O I
10.1134/S1990793123060155
中图分类号
O64 [物理化学(理论化学)、化学物理学]; O56 [分子物理学、原子物理学];
学科分类号
070203 ; 070304 ; 081704 ; 1406 ;
摘要
Within the framework of the quasiclassical trajectory method on semiempirical diabatic potential energy surfaces, we have considered the existence regions for direct three-body recombination Cs+ + Br- + R -> CsBr + R (R = Kr, Xe, Hg) in the case where the encounters of the Cs+ and Br- ions are central and the delay parameter vanishes. The recombination regions are determined using a much more precise procedure than in the previous works. Particular attention is paid to the recombination opacity functions and to the role of the orientation angles in the outcome of a three-body collision. The performed calculations demonstrate a great complexity of the structure of the recombination regions.
引用
收藏
页码:1270 / 1284
页数:15
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