Drennhaus Jan Philipp, Ferino-Pérez Anthuan, Matz Florian, Jagau Thomas-C
Department of Chemistry, KU Leuven, Celestijnenlaan 200F, B-3001 Leuven, Belgium.
Phys Chem Chem Phys. 2024 Sep 18;26(36):23846-23855. doi: 10.1039/d4cp02085e.
Vacancies in the L shell of atoms and molecules can decay non-radiatively Coster-Kronig decay whereby the vacancy is filled by an electron from the L shell while a second electron is emitted into the ionization continuum. This process is akin to Auger decay, but in contrast to Auger electrons, Coster-Kronig electrons have rather low kinetic energies of less than 50 eV. In the present work, we extend recently introduced methods for the construction of molecular Auger spectra that are based on complex-scaled equation-of-motion coupled-cluster theory to Coster-Kronig decay. We compute ionization energies as well as total and partial decay widths for the 2s states of argon and hydrogen sulfide and construct the LLM Coster-Kronig and LMM Auger spectra of these species. Whereas our final spectra are in good agreement with the available experimental and theoretical data, substantial disagreements are found for various branching ratios suggesting that spin-orbit coupling makes a major impact on Coster-Kronig decay already in the third period of the periodic table.
原子和分子L壳层中的空位可以通过非辐射的科斯特-克勒尼希衰变而衰减,即空位由L壳层中的一个电子填充,同时另一个电子被发射到电离连续谱中。这个过程类似于俄歇衰变,但与俄歇电子不同的是,科斯特-克勒尼希电子的动能相当低,小于50电子伏特。在本工作中,我们将最近引入的基于复标度运动方程耦合簇理论构建分子俄歇谱的方法扩展到科斯特-克勒尼希衰变。我们计算了氩和硫化氢2s态的电离能以及总衰变宽度和部分衰变宽度,并构建了这些物种的LLM科斯特-克勒尼希谱和LMM俄歇谱。虽然我们最终的谱与现有的实验和理论数据吻合良好,但在各种分支比上发现了很大的差异,这表明自旋-轨道耦合在元素周期表的第三周期就已经对科斯特-克勒尼希衰变产生了重大影响。