New accurate diabatic potential energy surfaces for the two lowest 1A′′ states of H2S and photodissociation dynamics in its first absorption band

被引:5
|
作者
Chen, Junjie [1 ]
Zhang, Hanzi [1 ]
Zhou, Linsen [2 ]
Hu, Xixi [3 ,4 ]
Xie, Daiqian [1 ,4 ]
机构
[1] Nanjing Univ, Inst Theoret & Computat Chem, Sch Chem & Chem Engn, Key Lab Mesoscop Chem, Nanjing 210023, Peoples R China
[2] China Acad Engn Phys, Inst Mat, Mianyang 621907, Sichuan, Peoples R China
[3] Nanjing Univ, Inst Brain Sci, Kuang Yaming Honors Sch, Nanjing 210023, Peoples R China
[4] Hefei Natl Lab, Hefei 230088, Peoples R China
基金
中国国家自然科学基金;
关键词
CONFIGURATION-INTERACTION CALCULATIONS; 193 NM PHOTODISSOCIATION; HYDROGEN-SULFIDE; EXCITED-STATES; ULTRAVIOLET PHOTODISSOCIATION; EMISSION-SPECTROSCOPY; DISSOCIATING H2S; SPECTRUM; ABINITIO; SCF;
D O I
10.1039/d3cp03026a
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
In this work, state-to-state photodissociation dynamics of H2S in its first absorption band has been studied quantum mechanically with a new set of coupled potential energy surfaces (PESs) for the first two 1A '' excited states, which were developed at the explicitly correlated internally contracted multi-reference configuration interaction level with the cc-pVQZ-F12 basis set and a large active space. The calculated absorption spectrum, product state distributions, and angular distributions are in excellent agreement with available experimental data, validating the accuracy of the PESs and the non-adiabatic couplings. Detailed analysis of the dynamics reveals that there are strong non-adiabatic couplings between the bound 1(1)B(1) and dissociative 1(1)A(2) states around the Franck-Condon region, leading to very fast predissociation to ro-vibrationally cold SH(X<combining tilde>) fragments, during which marginal angular anisotropy of the PESs is involved. This study provides quantitatively accurate characterization of the electronic structure and detailed fragmentation dynamics of this prototypical photodissociation system, which is desirable for improving astrochemical modelling.
引用
收藏
页码:26032 / 26042
页数:11
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