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Photodissociation dynamics of H_2S on new coupled ab initio potential energy surfaces

机译:H_2S在新的从头算起的势能面上的光解离动力学

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摘要

Three-dimensional potential energy surfaces for the electronic ground state as well as the lowest three ~1A" states have been computed using highly correlated CASSCF-MRCI wave functions and a large basis set. An approximate diabatization scheme has been employed to generate quasidiabatic potential energy surfaces for the lowest two ~1A" states. The diabatization is based on the condition that both the orbitals as well as the configuration coefficients of the diabatic wave functions change as little as possible as function of geometry. The diabatic potential energy surfaces are used in time-dependent simulations of the absorption spectrum as well as the vibrational and rotational product distributions. Excellent agreement between the computed and experimental absorption spectra and product distributions is obtained, indicating that the ab initio potentials as well as the diabatization scheme are accurate.
机译:使用高度相关的CASSCF-MRCI波函数和较大的基集,计算了电子基态的三维势能面以及最低的三个〜1A“状态。采用了近似的绝热方案来生成拟绝热势能最低的两个〜1A“状态的表面。绝热是基于这样的条件,即,绝热波函数的轨道以及构型系数都随几何形状的变化而变化尽可能小。绝热势能面用于吸收光谱以及振动和旋转产物分布的时间相关模拟。计算的和实验的吸收光谱与产物分布之间具有极好的一致性,表明从头算势和绝热方案是准确的。

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