C2H6分子电离能谱的SAC-CI计算

采用对称匹配簇组态相互作用(SAC-CI)的方法计算了乙烷分子的电离能谱，计算结果很好地与乙烷分子价壳层的实验电离能谱符合．在内价壳层能区内，理论结果预测了3个主要的伴线带．其中能量较低的伴线带可以被描述为单电子电离过程2a1g-1和双电子振激过程1eg-24a1g的混合；而能量较高的两个伴线带则分别由数个双电子振激过程形成．     

洞态Ar原子K_α和K_β伴线和超伴线的理论计算

基于全相对论多组态Dirac-Fock方法,对L壳层旁观空穴下Ar原子退激衰变辐射K-X射线K_(α1,2)(K→L_(3,2))和K_(β1,3)(K→M_(3,2))的6908条伴线和超伴线跃迁能、跃迁概率进行了系统计算,计算结果与文献已有数据比较具有很好的一致性.通过对(K~(-1)L~(-1),l=0-8)伴线和(K~(-2)L~(-l),l=0-8)超伴线跃迁谱线卷积得了其合成谱,给出了L壳层不同空穴数下K-X射线伴线和超伴线的平均能量和平均跃迁强度.结果表明,退激辐射X射线能量以及能移与L壳层空穴个数呈现明显的线性关系.基于结论,进一步给出了跃迁能移与L壳层空穴个数之间的关系表达式.研究结果可以为解释离子、原子碰撞过程中产生的X射线谱提供重要的理论支持.     

异二氯乙烯价壳层轨道电子结构的电子动量谱研究

本文报道了异二氯乙烯分子价壳层轨道电子结构的电子动量谱研究.实验由一台(e,2e)电子动量谱仪在非共面对称的几何条件下开展,入射电子能量为1200 eV.实验获得了异二氯乙烯价壳层各个轨道的电离能谱和电子动量分布.采用Hartree-Fock方法和密度泛函方法结果与实验数据基本一致.研究发现,干涉效应会对2a_2和5b_2这两个Cl孤对电子轨道的电子动量分布产生显著影响.     

异二氯乙烯价壳层轨道电子结构的电子动量谱研究（英文）

本文报道了异二氯乙烯分子价壳层轨道电子结构的电子动量谱研究.实验由一台(e,2e)电子动量谱仪在非共面对称的几何条件下开展,入射电子能量为1200 eV.实验获得了异二氯乙烯价壳层各个轨道的电离能谱和电子动量分布.采用Hartree-Fock方法和密度泛函方法结果与实验数据基本一致.研究发现,干涉效应会对2a_2和5b_2这两个Cl孤对电子轨道的电子动量分布产生显著影响.     

共轭聚合物中受激吸收与受激辐射的量子动力学研究

基于扩展的一维SSH紧束缚模型结合非绝热的分子动力学方法,理论研究了共轭聚合物分子(PPV)在光脉冲作用下受激吸收和受激辐射的量子动力学过程.首先,设定分子初始处于基态,讨论了受激吸收过程中不同的电子受激跃迁模式与光激发脉冲的关系.通过对终态的分析,发现分子受激后只能产生电子-空穴的束缚态,包括:激子、双激子和高能激子.计算了各种激发态的产率,特别是,给出了各种激发态产率与光激发能量的定量关系.此外,基于实验,分别讨论了光激发强度对高能激子和双激子产率的影响,并与实验结果进行了比较.最后,设定分子初始分别处于激子和双激子态,研究了分子内定域能级之间的受激辐射过程,并简单讨论了激子和双激子受激辐射与光激发能量及强度的关系.     

LaCl分子结构与基态X 1Σ+势能函数

用能量一致相对论有效核芯势和参阅文献基础上添加极化函数4f2g的价基组,在密度泛函理论(DFT)、多体微扰MPn和组态相关理论QCISD水平上计算了LaCl分子结构、离解能和振动频率.根据原子分子反应静力学原理,导出LaCl分子基态可能的电子状态和离解极限,用DFT中的B3LYP方法计算了基态X 1Σ+势能曲线,拟合得到了Murrell-Sorbie解析势能函数及其在平衡位置附近的Dunham展开式,由此计算的振转常数与实验光谱数据完全符合.得到的解析势能函数可用于计算振转光谱精细跃迁结构和原子分子碰撞反应动力学过程.     

LaCl分子结构与基态X1Σ+势能函数

用能量一致相对论有效核芯势和参阅文献基础上添加极化函数4f2g的价基组,在密度泛函理论(DFT)、多体微扰MPn和组态相关理论QCISD水平上计算了LaCl分子结构、离解能和振动频率.根据原子分子反应静力学原理,导出LaCl分子基态可能的电子状态和离解极限,用DFT中的B3LYP方法计算了基态X1Σ+势能曲线,拟合得到了MurrellSorbie解析势能函数及其在平衡位置附近的Dunham展开式,由此计算的振转常数与实验光谱数据完全符合.得到的解析势能函数可用于计算振转光谱精细跃迁结构和原子分子碰撞反应动力学过程 关键词： LaCl 相对论有效核芯势 解析势能函数 振转光谱常数     

单、双洞态镁离子的退激发及末电离态离子分布的研究

在分析双洞相关退激发对双洞态退激发的贡献较小的基础上，依据辐射-俄歇-双俄歇级联退激发模型(RACDA)研究了Mg¹⁺(1s^-1)（K壳层单洞态镁离子）和Mg²⁺(1s^-2)（K壳层双洞态镁离子）的退激发过程，计算了它们的末电离态离子的分布，并与辐射-俄歇级联退激发模型的结果进行了比较.RACDA模型计算的Mg¹⁺(1s^-1)的4价末电离态离子的相对丰度较大，而辐射-俄歇级联退激发模型(RAC)的结果中就没有出现4价离子；两种模型计算Mg²⁺(1s^-2)的6价末电离态离子的丰度非常大，而RAC模型下的Mg²⁺(1s^-2)退激发后不产生6价离子. 关键词： 双洞态退激发 RACDA退激发模型     

LaF分子结构与基态X1Σ+势能曲线研究

用能量一致相对论有效核芯势和含极化函数4f2g和弥散函数1s1p1d的价基组, 在各种计算水平上计算了LaF分子结构、振动频率和离解能. 根据原子分子反应静力学原理导出LaF分子基态可能的电子状态和离解极限, 用密度泛函理论中的B3LYP方法计算了基态X1Σ+势能曲线, 拟合得到了Murrell-Sorbie解析势能函数及其在平衡位置附近的Dunham展开式, 由此计算的振转常数和实验光谱数据完全吻合. 得到的解析势能函数可用于计算振转光谱精细跃迁结构和原子分子碰撞反应动力学过程, 具有重要的实用意义.     

等离子体屏蔽效应对Ar~(16+)基态和激发态能级的影响

基于Rayleigh-Ritz变分原理,发展了一套处理弱耦合等离子体环境中多电子原子(离子)非相对论能量及其相对论修正的解析方法.通过考虑电子间交换相互作用以及内外壳层电子的屏蔽效应,计算了Ar~(16+)基态1s~2~1S、单激发态1sns~(1,3)S (n=2—5), 1snp~(1,3)P (n=2—5)和双激发态2snp~1P (n=2—5)非相对论能量及其相对论修正值(包括质量修正、单体和双体达尔文修正以及自旋-自旋接触相互作用项),讨论了等离子体屏蔽效应对能级的影响.结果表明:相对论质量修正和第一类达尔文修正占主导,比其他相对论修正项高出三个数量级.此外,等离子体屏蔽效应具有明显的态选择性,屏蔽效应对外壳层电子的影响大于内壳层电子,随着等离子体屏蔽参数的增加,外壳层电子轨道向外延展,激发态越高,延展程度越大.     

Electronic excitation spectra of doublet anion radicals of cyanobenzene and nitrobenzene derivatives: SAC-CI theoretical studies†

Electronic ground and excited states of anion radicals of cyanobenzene derivatives: 1,3,5-tricyanobenzene, 1,2,4,5-tetracyanobenzene, and tetracyanoquinodimethane (TCNQ) and nitrobenzene derivatives: nitrobenzene, p-nitroaniline, m-nitroaniline, and o-nitroaniline were theoretically investigated by the symmetry adapted cluster-configuration interaction (SAC-CI) method, which is able to produce accurate theoretical electronic excitation spectra even for radical doublet states. For all the target molecules, the present calculations reproduced the positive electron affinities, which were mostly in good agreement with the experimental values, and their features, especially for TCNQ, were characterised by singly occupied molecular orbitals as well as the number of the electron-withdrawing terminal groups. The excitation energies and their oscillator strengths by the SAC-CI method were also in good agreement with the corresponding experimental UV/VIS/NIR spectra observed by one of the authors and other experimental evidences. Except for TCNQ, the present theoretical calculations were successful to first predict the existences of the forbidden (or very low intense) pure valence excited states in near-infrared region. The physical natures of the observed intense spectral bands were clarified and some new assignments to their electronic states were provided. By extending the present work, photo-related molecular designs of new functional electron acceptors may be challenged.     

The theoretical study on the potential energy curves for X^1 ∑^＋, A^1 ⅡI and C^1 ∑^- states of SiO molecule

This paper applies the symmetry-aziapted-cluster/symmetry-adapted-cluster configuration-interaction （SAC/SACCI） method to optimize the structures for X^1∑^＋, A^1 Ⅱ and C^1 ∑^- states of SiO molecule with the basis sets D95＋＋, 6-311＋＋G and 6-311＋＋G^＊＊. Comparing the obtained results with the experiments, it gets the conclusion that the basis set 6-311＋＋G^＊＊ is most suitable for the optimal structure calculations of X^1.∑^＋, A^Ⅱ and C^1∑^- states of SiO molecule. The whole potential energy curves for these electronic states are further scanned by using SAC/6-311＋＋G^＊＊ method for the ground state and SAC-CI/6-311＋＋G^＊＊ method for the excited states, then use a least square method to fit Murrell~Sorbie functions, at last the spectroscopic constants and force constants are calculated, which are in good agreement with the experimental data.     

BH分子势能函数研究

应用SAC(Symmetry Adapted Cluster)/SAC-CI(Configuration Interaction)方法,采用cc-pVDZ基组,分别对BH分子X1∑ 、B1∑ 和C′1Δ电子态进行了单点扫描计算.在此基础上,拟合得到了基态和C′1Δ态的Murrell-Sorbie函数形式的解析势能函数,同时也计算了这两个电子态的光谱项常数和力常数,并与实验和其它理论结果进行了比较.最后也对具有双极小值的B1∑ 态势能函数进行了简单研究,给出了一些有用的量化信息.     

The observation of “forbidden” transitions in He II photoelectron spectra

Anomalous bands are reported in the He II spectra of diatomic and triatomic molecules which are attributed to excitation of a second electron along with the primary ionization. This dual process is made possible by the mixing of ionized states of the same symmetry but different configurations i.e. by configuration interaction between ionized states. The close relationship between the observed bands and those reported in X-ray spectra which result from the so-called shake-up process is discussed.     

SAC/SAC-CI方法研究LiH基态(X1∑+)以及A1∑+、B1∏激发态结构与性质

利用SAC(Symmetry-Adapted Cluster)/SAC-CI(Configuration Interaction)理论中的SAC-CI-NV(Non-variational)and SAC-CI-V(Variational)方法,以及6-311 g**基组对LiH分子的基态(X1∑ )和A1∑ 、B1∏激发态的平衡结构以及性质进行了研究计算.两种方法对LiH分子的三个态进行处理,并将优化结果与现有实验值进行了比较,结果显示,理论计算值都与实验值符合较好.同时利用SAC/SAC-CI方法中的AllProperties关键字对我们所关心的LiH分子的基态(X1∑ )和A1∑ 、B1∏激发态进行了计算,并给出各个态在其平衡点位置处的偶极矩、振子强度和抗磁化率等一些性质参数,对以后的实验作理论参考.     

A complete and self-consistent evaluation of XPS spectra of TiN

The electron configuration in single crystalline (sc-)titanium nitride (TiN) has been quantitatively studied using angle resolved X-ray photoelectron spectroscopy (AR-XPS). All samples were fabricated and transferred in situ so that only minimal surface contaminations were observed. The residual oxygen contamination was separated from the bulk information by extrapolating angle resolved measurements. Special attention is given to the quantitative evaluation of the spectra based on basic principles. Shake-up features are observed on core level lines and appear due two final ionized states. The ratio of this shake-up and the main Ti 2p energy line are investigated in this paper. In order to quantify this shake-up a precise evaluation is required. Here we present an approach to evaluate the XPS spectra of the Ti 2p photoemission line in TiN in a self-consistent manner that accounts for all features observable in an energy window of 80 eV. The evaluation considers the appropriate Tougaard background correction, shake-up features as well as surface and bulk plasmons. The ratio of the Ti 2p_1/2 and Ti 2p_3/2 and the corresponding peaks in the energy loss features fulfill the requirements given by quantum mechanics. The energy loss ΔE due to the shake-up process and the shake-up ratio have been determined quantitatively for oxygen-free bulk titanium nitride. The origin of the shake-up, its intensity and energy difference ΔE are explained by a two electron excitation process.     

Ab initio calculations of the ionization spectrum of SO2

The ionization spectrum of sulfur dioxide has been successfully studied by using the symmetry-adapted-cluster configuration-interaction （SAC-CI） general-R and SD-R methods and the basis set correlation-consistent polarized valence triple-zeta （cc-pVTZ）. The SAC-CI general-R method reproduces the experimental spectrum well for both the main peaks and the satellite peaks of ionization spectrum of SO2. The sequence of ionic states corresponding to main peaks of SO2 has been re-determined according to the SAC-CI conclusions and it is reordered as X^2A1, A^2B2, B2A2, C^2B1,D^2A1, E^2B2 and F^2A1. Besides, the equilibrium structures and adiabatic ionization potentials （AIPs） of ionic states of main peaks of SO2 are calculated by using the SAC-CI SD-R method.     

Electron-induced KLL Auger electron spectroscopy of Fe,Cu and Ge

KLL Auger spectra excited by electrons with energies in the 30–35 keV range of Fe, Cu and Ge films were measured, using thin free-standing films. It was possible to obtain spectra with an energy resolution of about 1 eV. The observed spectra can not be described satisfactorily by just the multiplet splitting of the final state as calculated for an isolated atom. Additional features, due in part to intrinsic (shake satellites) and in part to extrinsic (energy loss of the escaping electron) processes formed a large fraction on the observed intensities. In particular a number of distinct satellite structures that are not predicted by the atomic Auger process are observed. For Fe and Cu the satellite peaks can be explained in terms of shake-up processes from the 3d_5/2–4d_5/2 states. Similar satellite structures observed in Ge are partly attributed to plasmon creation and partly to shake-up processes. It is demonstrated that both the thickness dependence of the observed intensity distributions and transmission electron energy loss measurements contain invaluable information for the interpretation of these spectra.     

ESCA studies of CO2, CS2 and COS

The core level electron spectra of CO₂, CS₂ and COS excited by Mg Kα radiation have been studied to identify shake-up satellite lines associated with ionization from these levels. A number of such lines have been seen and possible assignments have been suggested using the excited states of the molecule as a guide. The valence spectra have also been recorded and they too were found to be rich in shake-up structure. The observed variation of the valence line intensities is discussed and compared with predictions made from an intensity model. The validity of distinguishing between π and σ symmetries in linear molecules in applying the intensity model is confirmed.