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Electronic quenching of sulfur induced by argon collisions
Physical Chemistry Chemical Physics ( IF 2.9 ) Pub Date : 2025-01-24 , DOI: 10.1039/d4cp04586f
David M. G. Williams, Nicole Weike, Manuel Lara, Kevin M. Dunseath, Alexandra Viel
Physical Chemistry Chemical Physics ( IF 2.9 ) Pub Date : 2025-01-24 , DOI: 10.1039/d4cp04586f
David M. G. Williams, Nicole Weike, Manuel Lara, Kevin M. Dunseath, Alexandra Viel
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An accurate potential energy model, explicitly designed for studying scattering and treating the spin–orbit and nonadiabatic couplings on an equal footing, is proposed for the S + Ar system. The model is based on the Effective Relativistic Coupling by Asymptotic Representation (ERCAR) approach, building the geometry dependence of the spin–orbit interaction via a diabatisation scheme. The resulting full diabatic model is used in close-coupling calculations to compute inelastic scattering cross sections for de-excitation from the S(1D2) fine structure level into the 3P multiplet. The energy grid is tuned to resolve the many resonances present and to guarantee converged thermal rates from 1 to 300 K. At temperatures above 100 K, the computed thermal rate coefficients for quenching of S(1D2) are in good agreement with results from an earlier experimental and theoretical study. The branching ratio at 296 K for de-excitation into the S(3P0) level agrees well with the value obtained by a different experiment. A discrepancy however remains between theory and experiment at lower temperatures. This is discussed in light of the interference mechanisms at play during this quenching process.
中文翻译:
氩碰撞诱导的硫的电子淬火
为 S + Ar 系统提出了一个精确的势能模型,该模型专门用于研究散射和平等地处理自旋-轨道和非绝热耦合。该模型基于渐近表示的有效相对论耦合 (ERCAR) 方法,通过绝热化方案构建自旋-轨道相互作用的几何依赖性。所得的全非绝热模型用于紧耦合计算,以计算非弹性散射截面,以便从 S(1D2) 精细结构水平去激发到 3P 多重态。对能源网进行了调整,以解决存在的许多共振,并保证从 1 到 300 K 的收敛热速率。在高于 100 K 的温度下,计算出的 S(1D2) 淬火热速率系数与早期实验和理论研究的结果非常一致。在 296 K 时去激发到 S(3P0) 水平的支化比与通过不同实验获得的值非常吻合。然而,在较低温度下,理论和实验之间仍然存在差异。根据此淬灭过程中起作用的干扰机制对此进行了讨论。
更新日期:2025-01-29
中文翻译:

氩碰撞诱导的硫的电子淬火
为 S + Ar 系统提出了一个精确的势能模型,该模型专门用于研究散射和平等地处理自旋-轨道和非绝热耦合。该模型基于渐近表示的有效相对论耦合 (ERCAR) 方法,通过绝热化方案构建自旋-轨道相互作用的几何依赖性。所得的全非绝热模型用于紧耦合计算,以计算非弹性散射截面,以便从 S(1D2) 精细结构水平去激发到 3P 多重态。对能源网进行了调整,以解决存在的许多共振,并保证从 1 到 300 K 的收敛热速率。在高于 100 K 的温度下,计算出的 S(1D2) 淬火热速率系数与早期实验和理论研究的结果非常一致。在 296 K 时去激发到 S(3P0) 水平的支化比与通过不同实验获得的值非常吻合。然而,在较低温度下,理论和实验之间仍然存在差异。根据此淬灭过程中起作用的干扰机制对此进行了讨论。