He2+和He2++分子离子基态和激发态的特性研究

采用SAC/SAC-CI方法在CC-PV5Z基组下, 计算研究了He2+、He2++的基态及低激发态的分子特性, 给出了其基态和一些激发态的势能函数和光谱数据(Be、αe、ωe和ωeχe). 从群论出发推导了相应状态的离解极限；与已有实验结果的He2+(X2Σu+)相比, 计算结果令人满意. 还计算了激发态2Πu、4Σu+和4Πg的结构与光谱数据. 对于He2++, 计算的九个电子态中只有三个态(X1Σg+、1Σg+和1Σu+)属束缚态, 并得到了其光谱常数. 用价键理论模型的不相交规则对He2++基态的势能曲线极大点产生的原因做了较好的分析.     

硫族铅化物阳离子低电子态的理论研究

采用我们最近发展的含旋轨耦合的运动方程耦合簇计算电离能(EOMIP-CC)方法,在CCSD级别上计算了硫族铅化物PbS、PbSe、PbTe阳离子低电子态的平衡键长和谐振频率以及绝热和垂直电离能,得到的结果与已有的实验值吻合较好.不考虑旋轨耦合(SOC)的情况下通过与CCSD(T)的计算结果比较,考察了三重激发对计算结果的影响,结果显示考虑三重激发的贡献后得到的键长和频率结果与实验值吻合更好.计算结果表明PbTe+中2Π态的能量分裂明显大于PbS+和PbSe+中2Π态的能量分裂,但是PbTe+中2Π1/2和2Σ1/2态之间的相互耦合则明显弱于PbS+和PbSe+中这两个态之间的耦合.PbTe+中2Π1/2和2Σ1/2态之间耦合很弱,一方面是因为2Σ+态和2Π态的能量差比PbS+和PbSe+中2Σ+态和2Π态的能量差大,另一方面还由于PbTe+中2Π1/2和2Σ1/2态之间的旋轨耦合矩阵元只是PbS+和PbSe+中2Π1/2和2Σ1/2态之间的旋轨耦合矩阵元的一半.这些计算结果为PbS+、PbSe+、PbTe+阳离子的低电子态性质提供了新的理论数据,可以为将来的实验数据提供参考.     

OCS+经由A2Π←X2Π激发的光解离光谱

在超声分子束条件下,由423、420、412.2和408.4 nm的电离激光使OCS分子通过[3+1]共振增强多光子电离(REMPI)制备出OCs+ (X2Π)离子后,在260-325 nm范围内扫描解离激光获得了OCS+离子经由A2Π3/2←X2Π3/2 (000)和A2Π1/2←X2Π1/2 (000,001)跃迁的分质量光解离谱(母体离子OCS+的凹陷谱和碎片离子S+的增强谱).其中A2Π1/2←X2Π1/2 (001)跃迁的光解离谱是首次观察到.A2Π3/2←X2Π3/2(000)光解离谱得到了A2Π3/2电子态的光谱常数T0=31411.3 cm-1,v1=814.3 cm-1;由A2Π1/2←X2Π1/2 (000)光解离谱得到了A2Π1/2电子态的光谱常数v1=816 cm-1,v2=(380.4±2.8) cm-1,v3=(2052.7±5.1) cm-1,而从A2Π1/2←X2Π1/2 (001)光解离谱拟合出的A2Π1/2电子态的V1 (786.4 cm-1)稍有不同,表明在A2Π1/2←X2Π1/2(001)跃迁中A2Π1/2电子态的C-O键振动(V3)激发影响了A2Π1/2电子态C-S键的振动(V1).实验结果表明:在A2Π1/2←X2Π1/2(000,001)跃迁的光解离谱中能够显著观察到属于A2Π电子态的V2弯曲振动模激发的谱峰,例如A2Π1/2(020,120,021,…),而在A2Π1/2(v1v2v3)←A2Π3/2(000)跃迁的光解离谱中几乎没有观察到属于V2弯曲振动模激发的谱峰.这种弯曲振动激发和A2Π电子态的旋轨分裂分量(Ω)的相关性可以通过A2Π电子态的Fermi共振和Renner-Teller效应来解释.     

OCS+经由A2П←X2П激发的光解离光谱

在超声分子束条件下,由423、420、412.2和408.4nm的电离激光使OCS分子通过[3+1]共振增强多光子电离(REMPI)制备出OCS+(X2Π)离子后,在260-325nm范围内扫描解离激光获得了OCS+离子经由A2Π3/2←X2Π3/2(000)和A2Π1/2←X2Π1/2(000,001)跃迁的分质量光解离谱(母体离子OCS+的凹陷谱和碎片离子S+的增强谱).其中A2Π1/2←X2Π1/2(001)跃迁的光解离谱是首次观察到.由A2Π3/2←X2Π3/2(000)光解离谱得到了A2Π3/2电子态的光谱常数T0=31411.3cm-1,ν1=814.3cm-1;由A2Π1/2←X2Π1/2(000)光解离谱得到了A2Π1/2电子态的光谱常数ν1=816cm-1,ν2=(380.4±2.8)cm-1,ν3=(2052.7±5.1)cm-1,而从A2Π1/2←X2Π1/2(001)光解离谱拟合出的A2Π1/2电子态的ν1(786.4cm-1)稍有不同,表明在A2Π1/2←X2Π1/2(001)跃迁中X2П1/2电子态的C-O键振动(ν3)激发影响了A2Π1/2电子态C-S键的振动(ν1).实验结果表明:在A2Π1/2←X2Π1/2(000,001)跃迁的光解离谱中能够显著观察到属于A2Π电子态的ν2弯曲振动模激发的谱峰,例如A2Π1/2(020,120,021,…),而在A2П3/2(υ1υ2υ3)←X2Π3/2(000)跃迁的光解离谱中几乎没有观察到属于ν2弯曲振动模激发的谱峰.这种弯曲振动激发和A2П电子态的旋轨分裂分量(Ω)的相关性可以通过A2Π电子态的Fermi共振和Renner-Teller效应来解释.     

PdO~(0,±1),PdH~(0,±1)及PdOH分子结构和电子性质的从头计算

利用多种从头计算方法对PdO0,±1,PdH0,±1以及PdOH的结构和电子性质进行了理论研究.优化了PdO分子两个能量相近的态(3Π和3Σ-),结果表明PdO的3Π态较3Σ-态更为稳定,在单双激发耦合簇理论(CCSD)水平下3Σ-态的总能量比3Π态的高出0.286eV.在结构优化的基础上计算了PdO以及PdH的绝热电离能(AIE)和电子亲和能(AEA),计算结果与实验值符合得很好.PdOH的基态为Cs对称性的角型结构Pd—OH(2A′态),另外还优化得到两个2A″态的亚稳结构,分别对应于Pd—OH和O—Pd—H,CCSD水平下两个亚稳态的总能量较基态分别高0.405和2.284eV,优化得到了连接这两个2A″态的过渡态,并计算了相应的反应能垒.     

理论研究BrCl~ 低激发电子态势能曲线和光谱性质

应用量子化学中高等级的多参考组态相互作用方法计算了环境科学中重要的分子离子BrCl 的基态和低激发态的势能曲线与光谱常数,详细分析了旋轨耦合作用对电子结构和光谱性质的影响,确认了基态X2Π和低激发电子态的多组态特征,得到了基态X2Π的旋轨耦合分裂能1814cm-1,与实验值2070cm-1接近.预测了2Π(Ⅱ)态的旋轨耦合分裂能为766cm-1.估算了3/2(Ⅲ)-X3/2和1/2(Ⅲ)-1/2(Ⅰ)跃迁的偶极跃迁矩和Frank-Condon因子,讨论了它们的跃迁辐射寿命.     

氰基铝(AlCN)及其阴阳离子低能激发态的理论研究

在C2v对称性下,采用全活化空间自洽场(CASSCF)和多组态二级微扰理论(CASPT2)方法研究氰基铝(AlCN)及其阴阳离子的基态和低能激发态.在ANO-L基组水平下,计算了AlCN及其阴阳离子低能电子态的几何,组态及其相互作用系数,谐振频率,绝热激发能,垂直激发能和振子强度.在CASSCF/CASPT2理论水平下,计算得到AlCN的11Π电子态的绝热激发能为352.4kJ·mol-1,与实验值344.0kJ·mol-1符合得很好.另外,预测AlCN的跃迁X1Σ+→21Π发生在673.1kJ·mol-1.激发能和振子强度的计算为研究AlCN的吸收光谱提供理论指导.     

NaC分子基态及其低电子激发态

运用包含Davidson修正的多参考组态相互作用(MRCI+Q)方法结合6-311++G(3df,3pd)基组计算了NaC分子基态(X4∑)以及三个低电子激发态(a2Π, b2∑, A4Π)的势能曲线(PECs), 确定出相应态的平衡键长Re和垂直激发能Te. 然后将PECs拟合到Murrel-Sorbie(MS)解析势能函数形式, 继而获得各态的光谱数据: 谐振频率ωe、离解能De、非谐性常数ωeΧe、转动常数Be、Drot和振转耦合常数αe. 计算结果表明: X4∑、a2Π、b2∑是三个束缚电子态. 基态X4∑的平衡键长为0.2259 nm, 谐振频率为431 cm-1, 离解能为1.92 eV, 目前计算值与实验结果和其它理论值一致. a2Π和b2∑激发态的核间距、谐振频率分别为0.2447、0.2369 nm 和329、335 cm-1, Te分别为1.58 和1.75eV, De则为0.71和0.42 eV. A4Π态为排斥态, 其相对基态的垂直激发能为2.48 eV. 通过求解核运动的薛定谔方程找到了转动量子数J=0时NaC分子三个低电子态(X4∑, a2Π, b2∑)的全部振动能级和转动惯量.     

AuX(X=O,S)低电子态的理论研究

通常要用多参考态方法才能合理处理需考虑旋轨耦合(SOC)效应的开壳层分子如AuO和AuS的低电子态.事实上,通过选取合适的参考态,采用运动方程耦合簇方法(EOM-CC)也能计算这些分子的一些低电子态,而且EOM-CC方法是单参考态方法,使用起来比多参考态方法更加简单.本文采用最近发展的含旋轨耦合的EOM-CC计算电离能的方法(EOMIP-CC),选取对应的负离子为参考态,在CCSD级别上计算了AuO和AuS低电子态的性质.在不考虑旋轨耦合时,通过比较EOMIP-CCSD和EOMIP-CCSDT的结果考察EOMIPCCSD的精度.此外,与EOMIP-CCSDT结果相比,如果自旋污染较为显著而且T1的模较大时,UCCSD(T)方法对能量最低的某一特定对称性的电子态的所对应的电离能误差约为0.1-0.15 eV.在考虑了旋轨耦合效应后,我们的方法得到的键长和振动频率与实验值吻合较好.另一方面,虽然EOMIP-SOC-CCSD高估了能量较高的2Δ3/2态、2Σ+1/2态和2Π1/2态的能量,但是对于其它能量更低的电子态,它们的能量与已有实验值误差在0.2 eV左右.这显示我们所用的含SOC的EOMIP-CCSD方法对原本需要用多参考态方法才能处理的AuO和AuS低电子态能给出可靠的结果.     

超声射流下12C16O+离子A2Π1/2,3/2←X2Σ+激光诱导荧光激发谱

用一束波长为230.1nm的激光,通过(2 1)共振增强多光子电离(REMPI)过程激发超声射流冷却的CO分子制备处于基电子态X2Σ 的CO ,随后引入另一束可调谐激光将CO 离子激发至A2Π1/2,3/2态,利用光电倍增管(PMT)检测发射的荧光信号强度随激发光波长的变化,分别在487-493nm和453-459nm波长范围内获得了CO 离子A2Π1/2,3/2←X2Σ 电子态跃迁(0,0)和(1,0)带的激光诱导荧光(LIF)激发谱.     

ZnNe低激发态的量子化学研究

用相对论赝势ＣＡＳＳＣＦ／ＣＩ方法,对ＺｎＮｅ的基态和低激发态进行了计算,得出了它们的电子结构,势能曲线及光谱常数。计算结果表明,ＺｎＮｅ的基态分子是范德华分子,它的几个低激发态分子中的主要作用力为范德华力,这些态的分子仍为范德华分子。     

Experimental investigation of electronic states of LiCs dissociating to Li(2(2)S) and Cs(5(2)D) atoms

Polarization labeling spectroscopy technique was used to measure excitation spectra of LiCs molecule in the spectral range of 16,000-18,500 cm(-1). Four band systems were observed and assigned to transitions from the ground X(1)Σ(+) state to excited states (4)Ω = 0(+), (5)Ω = 0(+), (5)Ω = 1, and (6)Ω = 1 (in Hund's case (c) notation proper here), the latter three states being fine structure components of the states d(3)Π and e(3)Σ(+), nominally of triplet symmetry. The observed states are characterized spectroscopically and the experimental results are compared with predictions of theoretical calculations, showing accuracy of the theoretical electronic term values better than 100 cm(-1) and of the ω(e) and R(e) constants within 5%.     

MRDCI study of the low-lying electronic states of PbSi

Electronic states of the PbSi molecule up to 4 eV have been studied by carrying out ab initio based MRDCI calculations which include relativistic effective core potentials (RECPs) of both the atoms. The use of semicore RECPs of Pb produces better dissociation limits than the full-core one. However, the (3)P(0)-(3)P(1) splitting due to Pb is underestimated by about 4000 cm(-1). At least 25 bound electronic states of the Λ-S symmetry are predicted for PbSi. The computed zero-field-splitting in the ground state is about 544 cm(-1). A strong spin-orbit mixing changes the nature of the potential energy curves of many Ω states. The overall splitting among the spin components of A(3)Π is computed to be 4067 cm(-1). However, the largest spin-orbit splitting is reported for the (3)Δ state. A number of spin-allowed and spin-forbidden transitions are predicted. The partial radiative lifetime for the A(3)Π-X(3)Σ(-) transition is of the order of milliseconds. The computed bond energy in the ground state is 1.68 eV, considering the spin-orbit coupling. The vertical ionization energy for the ionization to the X(4)Σ(-) ground state of PbSi(+) is about 6.93 eV computed at the same level of calculations.     

Photo-acoustic detection on electronic quenching rate constants of NO excited states

The electronic quenching rate constants of NO A(2)Σ (υ'=0, 1), E(2)Σ (υ'=2, 3, 4) and F(2)Δ (υ'=1, 2, 3) states by gas air are reported. The experiments were carried out by measuring the total fluorescence intensity of A(2)Σ (υ'=0, 1)→X(2)Π (υ″) transition at various air pressures. It gives the Stern-Volmer plots. The quenching rate constants of A(2)Σ (υ'=0, 1) states are obtained from the slope of Stern-Volmer plots and the known radiative lifetime. Based on the primary results of the work, we have measured the quenching rate constants of high excited E(2)Σ (υ'=2, 3, 4), F(2)Δ (υ'=1, 2, 3) states for the first time with the technique of photo-acoustic (PA) spectroscopy. It is shown that the electronic quenching rate constants of NO E (υ') and F (υ') states are in the order of 10(-10)cm(3)/molecules. They are much larger than those of A(2)Σ (υ') state, whose rate constants are in the order of 10(-13)cm(3)/molecules. For E (υ') and F (υ') states, it is also found that the quenching rate constants increase with the vibrational energy levels. Similar result has been reported also for A(2)Σ (υ'≥2) states in existing literatures. The agreement indicates the potential use of PA spectroscopy for measuring the electronic quenching rate.     

C6H and C6D: electronic spectra and Renner-Teller analysis

Rotationally resolved spectra of the B(2)Π - X(2)Π 0(0)(0) electronic origin bands and 11(1)(1) μ(2)Σ-μ(2)Σ vibronic hot band transitions of both C(6)H and C(6)D have been recorded in direct absorption by cavity ring-down spectroscopy through a supersonically expanding planar plasma. For both origin and hot bands accurate spectroscopic parameters are derived from a precise rotational analysis. The origin band measurements extend earlier work and the 11(1)(1) μ(2)Σ-μ(2)Σ vibronic hot bands are discussed here for the first time. The Renner-Teller effect for the lowest bending mode ν(11) is analyzed, yielding the Renner parameters ε(11), vibrational frequencies ω(11), and the true spin-orbit coupling constants A(SO) for both (2)Π electronic states. From the Renner-Teller analysis and spectral intensity measurements as a function of plasma jet temperature, the excitation energy of the lowest-lying 11(1) μ(2)Σ vibronic state of C(6)H is determined to be (11.0 ± 0.8) cm(-1).     

CH3(2A′)自由基与臭氧反应机理的量子化学研究

用量子化学UMP2方法，在6-311++G**基组水平上研究了CH3(2A′)自由基与臭氧反应机理，全参数优化了反应过程中反应物、中间体、过渡态和产物的几何构型，在UQCISD(T)/6-311++G**水平上计算了它们的能量；并对它们进行了振动分析，以确定中间体和过渡态的真实性；同时应用经典过渡态理论计算了反应的速率常数，并与实验值进行了比较, CH3自由基与臭氧反应速率常数的理论计算结果为: 4.73×10－14 cm3•molecule－1•s－1，与实验报导的结果(k=2.52×10－14 cm3•molecule－1•s－1)很接近，同时发现CH3(2A′)自由基与O3的反应是强放热反应.     

Electronically excited-state properties and predissociation mechanisms of phosphorus monofluoride: a theoretical study including spin-orbit coupling

The 51 Ω states generated from the 22 Λ - S states of phosphors monofluoride have been investigated using the valence internally contracted multireference configuration interaction method with the Davidson correction and the entirely uncontracted aug-cc-pV5Z basis set. The spin-orbit coupling is computed using the state interaction approach with the Breit-Pauli Hamiltonian. Based on the calculated potential energy curves, the spectroscopic constants of the bound and quasibound Λ - S and Ω states are obtained, and very good agreement with experiment is achieved. Several quasibound states caused by avoided crossings are found. Various curve crossings and avoided crossings are revealed, and with the help of our computed spin-orbit coupling matrix elements, the predissociation mechanisms of the a(1)Δ, b(1)Σ(+), e(3)Π, g(1)Π, and (3)(3)Π states are analyzed. The intricate couplings among different electronic states are investigated. We propose that the avoided crossing between the A(3)Π(0 +) and b(1)Σ(0+) (+) states may be responsible for the fact that the A(3)Π ν' ≥ 12 vibrational levels can not be observed in experiment. The transition properties of the A(3)Π - X(3)Σ(-) transition are studied, and our computed Franck-Condon factors and radiative lifetimes match the experimental results very well.     

Spectroscopic analysis of the coupled 1(1)Π, 2(3)Σ+ (Ω = 0-, 1), and b(3)Π (Ω = 0±, 1, 2) states of the KRb molecule using both ultracold molecules and molecular beam experiments

We report the spectroscopic characterization of excited electronic states of KRb by combining spectra from molecular beam (MB) experiments with those from ultracold molecules (UM) formed by photoassociation (PA) of ultracold atoms. Spectra involving the 1(1)Π, 2(3)Σ(+), and b(3)Π states in a strongly perturbed region have been identified. This approach provides a powerful method to identify the vibrational levels of the excited electronic states perturbed globally by neighboring electronic states. This is because the two sets of spectra from the UM and the MB experiments probe the same energy region from very different initial electronic states. The UM experiments utilize high v' levels of the a(3)Σ(+) state with large internuclear separations, while the MB experiments utilize low v' levels of the ground X(1)Σ(+) state with near-equilibrium internuclear separations. Only the Ω = 1 levels of the 2(3)Σ(+) and b(3)Π states are observed in the MB spectra, while the Ω = 0(-), 1 levels of the 2(3)Σ(+) state and the Ω = 0(±), 1, 2 levels of the b(3)Π state are observed in the UM spectra.     

OH自由基的高精度量子化学研究

采用内收缩MRCI方法(Internally Contracted Multiconfiguration-Reference Configuration Interaction)研究了OH自由基, 计算得到其基态稳定构型的键长是0.09708 nm, 对应的实验值是0.096966 nm, 第一激发态的键长是0.10137 nm,实验值是0.10121 nm. 同时得到势能曲线PECs (Potential Energy Curve), 再分别由Murrell-Sorbie势能函数拟合计算和POLFIT程序计算得到OH自由基在基态X²Π和第一激发态A²Σ⁺时的光谱数据：平衡振动频率ω_e, 非谐性常数ω_eχ_e以及高阶修正ω_eY_e, 平衡转动常数B_e, 振转耦合系数α_e, 解离能D₀和垂直跃迁能量ν₀₀. 这些理论计算结果与最新的实验值非常吻合, 精确度比前人也有很大提高. 其中我们计算得到基态OH(X²Π)的解离能D₀＝35568.86 cm^－1, 第一激发态OH (A²Σ⁺)的解离能D₀＝18953.93 cm^－1, 从第一激发态A²Σ⁺ (ν＝0)到基态X²Π (v＝0)的垂直跃迁能ν₀₀＝32496.42 cm^－1.     

Excited electronic states, transition probabilities, and radiative lifetimes of CAs: a theoretical contribution and challenge to experimentalists

High-level CASSCF/MRCI calculations with a quintuple-ζ quality basis set are reported by characterizing for the first time a manifold of electronic states of the CAs radical yet to be investigated experimentally. Along with the potential energy curves and the associated spectroscopic constants, the dipole moment functions for selected electronic states as well as the transition dipole moment functions for the most relevant electronic transitions are also presented. Estimates of radiative transition probabilities and lifetimes complement this investigation, which also assesses the effect of spin-orbit interaction on the A (2)Π state. Whenever pertinent, comparisons of similarities and differences with the isovalent CN and CP radicals are made.