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The electronic structure of the triiodide ion from relativistic correlated calculations: A comparison of different methodologies

机译:相对论相关计算得出的三碘离子的电子结构:不同方法的比较

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The triiodide ion I_3~- exhibits a complex photodissociation behavior, the dynamics of which are not yet fully understood. As a first step toward determining the full potential energy surfaces of this species for subsequent simulations of its dissociation processes, we investigate the performance of different electronic structure methods [time-dependent density functional theory, complete active space perturbation theory to second order (CASPT2), Fock-space coupled cluster and multireference configuration interaction] in describing the ground and excited states of the triiodide ion along the symmetrical dissociation path. All methods apart from CASPT2 include scalar relativity and spin-orbit coupling in the orbital optimization, providing useful benchmark data for the more common two-step approaches in which spin-orbit coupling is introduced in the configuration interaction. Time-dependent density functional theory with the statistical averaging of model orbital potential functional is off the mark for this system. Another choice of functional may improve performance with respect to vertical excitation energies and spectroscopic constants, but all functionals are likely to face instability problems away from the equilibrium region. The Fock-space coupled cluster method was shown to perform clearly best in regions not too far from equilibrium but is plagued by convergence problems toward the dissociation limit due to intruder states. CASPT2 shows good performance at significantly lower computational cost, but is quite sensitive to symmetry breaking. We furthermore observe spikes in the CASPT2 potential curves away from equilibrium, signaling intruder state problems that we were unable to curb through the use of level shifts. Multireference configuration interaction is, in principle, a viable option, but its computational cost in the present case prohibits use other than for benchmarking purposes.
机译:三碘离子I_3-具有复杂的光解离行为,其动力学尚未完全了解。作为确定该物种的完整势能面以用于其解离过程的后续模拟的第一步,我们研究了不同电子结构方法的性能[时间依赖性密度泛函理论,完整的主动空间扰动理论至二阶(CASPT2) ,Fock-空间耦合的簇和多参考构型相互作用]描述了三碘化物离子沿着对称解离路径的基态和激发态。除CASPT2之外,所有方法都包括轨道优化中的标量相对论和自旋轨道耦合,为更常见的两步方法(在配置交互中引入自旋轨道耦合)提供了有用的基准数据。随时间变化的密度泛函理论和模型轨道势函数的统计平均值在该系统中不适用。官能团的另一种选择可以改善关于垂直激发能和光谱常数的性能,但是所有官能团都可能在远离平衡区的地方面临不稳定问题。结果表明,福克空间耦合聚类方法在离平衡点不太远的区域中表现最佳,但由于入侵者的状态而受到朝向解离极限的收敛问题的困扰。 CASPT2以低得多的计算成本表现出良好的性能,但对对称破坏非常敏感。此外,我们还观察到CASPT2电位曲线中的尖峰远离平衡状态,这表明入侵者状态问题是我们无法通过使用电平移动来抑制的。原则上,多引用配置交互是一个可行的选择,但是在当前情况下,其计算成本禁止将其用于基准测试以外的用途。

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