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首页> 外文期刊>The Journal of Chemical Physics >Accurate prediction of excitation energies to high-lying Rydberg electronic states:Rydbery states of acetylene as a case study
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Accurate prediction of excitation energies to high-lying Rydberg electronic states:Rydbery states of acetylene as a case study

机译:精确预测高能Rydberg电子态的激发能:以乙炔的Rydbery态为例

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摘要

Ab initio outer-valence Green functions (OVGF),equation-of-motion coupled cluster (EOM-CCSD),and Hartree-Fock (HF)calculations with specially constructed basis sets have been carried out to predict excitation energies to Rydberg electronic states of acetylene with principal quantum numbers n up to 11.A comparison fo calculated energies with experiment shows that the OVGF method gives acdurate results for a broad energy range of 8-11.5eV.The deviations from experimental data are as low as 0.03-0.04 eV for n=5-8 and are slightly larger for the higher states,~0.05 eV FOR N=9-11.The OVGF calculations are thus demonstrated to be able to repoduce excitation energies for high-lying Rydberg states wtih a good precision,higher than that provided by the EOM-CCSD method,if one uses experimental or high-level calcualted values off the ionization potential.With an increase of the principal quantum number for the Rydberg state,the OVGF corrections to teh HF-calculated energies decrease adn one can use the HF approach to compute orbital energy levels and excitation energies for higher Rydberg states.The energy levals for high-lying Rydberg states are shown to be insensitive to the molecular geometry,so that the energy gaps between vertical absorption and vertical emission for these states should be similar and can be estimated by the relaxatin energy of the neutral system starting from geometry of the positive ion.
机译:从头算出外价格林函数(OVGF),运动方程耦合簇(EOM-CCSD)和Hartree-Fock(HF)计算具有特殊构造的基集,可以预测Rydberg电子态的激发能。主要量子数n最高为11的乙炔。与实验计算的能量比较表明,OVGF方法在8-11.5eV的宽能范围内给出了准确的结果,与实验数据的偏差低至0.03-0.04 eV n = 5-8且对于更高的状态稍大,对于N = 9-11则为〜0.05 eV。因此,OVGF计算被证明能够以较高的精度来抵消高处Rydberg态的激发能。由EOM-CCSD方法提供的结果,如果使用电离势的实验或高级计算值。随着Rydberg态主量子数的增加,对HF计算的能量的OVGF校正会减少ü通过HF方法计算较高里德堡态的轨道能级和激发能。高处里德堡态的能级对分子几何形状不敏感,因此这些态的垂直吸收和垂直发射之间的能隙应当是相似的,并且可以由中性系统的弛豫能量从正离子的几何形状开始估算。

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