BO分子α带系A~2Π-X~2Σ~ 及β带系B~2Σ~ -X~2Σ~ Franck-Condon因子的计算

在双原子分子核运动的波动方程中，计入分子的振转相互作用项，得出的波函数除与振动量子数有关外，还与转动量子数有关。用该波函数编程计算了ＢＯ分子α带系Ａ２Π－Ｘ２Σ＋及β带系Ｂ２Σ＋－Ｘ２Σ＋的Ｆｒａｎｃｋ－Ｃｏｎｄｏｎ因子。计算中转动量子数的取值由Ｊ＝０取至Ｊ＝２００，结果适用于低温、高温和强激波条件。     

激波管壁AlO自由基B~2Σ~+-X~2Σ~+和C~2Π_r-X~2Σ~+带系辐射光谱的研究

爆轰驱动过程中产生的高温高压气流对铝质膜片、激波管壁产生烧蚀和冲刷作用,以致激波管壁、端盖上附有氧化铝等杂质,而高温下AlO自由基在气体分子的高速碰撞下被激发并产生强烈的辐射,从而干扰了高温气体辐射光谱的分析。用爆轰驱动加热技术将空气加热到4 000~7 000 K,利用多通道光学分析仪对AlO自由基辐射光谱进行分析,实验发现在460~530 nm波长范围内有多支辐射非常强烈的AlO自由基B2Σ+-X2Σ+(T00=20 689 cm-1)带系辐射谱带,且每支谱带都由多个带头组成,带头间隔约为2 nm,带头处于高频位置并向低频方向伸延。通过实验与理论计算相结合,重点分析了AlO自由基B2Σ+-X2Σ+带系辐射光谱的结构特征。AlO自由基C2Πr-X2Σ+(T00=33 047 cm-1)带系辐射光谱处于270~335 nm波长范围内,其辐射强度相对于B2Σ+-X2Σ+带系较弱,并且与OH基A2Σ+-X2Π(T00=32 682 cm-1)带系辐射光谱互相干扰而难以分辨,对该波段高温空气的辐射光谱分析产生不利的影响。     

MgO分子B~1Σ~ -X~1Σ~ 带系及MgH分子A~2Π-X~2Σ~ 带系振子强度的计算

选用ＳＴＯ４Ｇ双ζ扩展基组,用单组态自洽场方法计算分子轨道,然后作较大规模的组态相互作用计算,得到分子电子态的能量和波函数。在偶极近似下,进一步计算了ＭｇＯ分子Ｂ１Σ＋－Ｘ１Σ＋带系及ＭｇＨ分子Ａ２Π－Ｘ２Σ＋带系的振子强度,其值分别为ｆ１＝１．６２２×１０－３,ｆ２＝１．８１４×１０－３。     

Molecule opacities of X~2Σ~+, A~2Π, and B~2Σ~+ states of CS~+

Carbon sulfide cation(CS~+) plays a dominant role in some astrophysical atmosphere environments. In this work, the rovibrational transition lines are computed for the lowest three electronic states, in which the internally contracted multireference configuration interaction approach(MRCI) with Davison size-extensivity correction(+Q) is employed to calculate the potential curves and dipole moments, and then the vibrational energies and spectroscopic constants are extracted. The Frank–Condon factors are calculated for the bands of X~2~+Σ~+–A~2Π and X~2Σ~+–B~2Σ~+systems, and the band of X~2Σ~+–A~2Π is in good agreement with the available experimental results. Transition dipole moments and the radiative lifetimes of the low-lying three states are evaluated. The opacities of the CS~+ molecule are computed at different temperatures under the pressure of 100 atms. It is found that as temperature increases, the band systems associated with different transitions for the three states become dim because of the increased population on the vibrational states and excited electronic states at high temperature.     

N_2O~ 离子A~2Σ~ 电子态的光解动力学研究

用一束波长为 36 0 5 5nm的激光 ,通过N2 O分子的 (3 1 )共振多光子电离 (REMPI)过程制备纯净且布居完全处于X2 Π(0 0 0 )态的母体离子N2 O ,然后用另一束波长在 2 75— 32 8nm范围内的可调谐激光将制备的N2 O 离子激发至预解离电子态A2 Σ .实验发现 ,由于解离碎片NO 所具有的一定的反冲速度 ,其TOF质谱峰明显比N2 O 母体宽 .通过分析NO 碎片TOF质谱峰形状 ,得到了解离产物的总平均平动能〈ET〉 ;通过考察〈ET〉随光解能量的变化 ,发现光解能量在 32 0 0 0cm- 1 附近约 2 5 0cm- 1 的变化范围内 ,〈ET〉值由约 80 0 0cm- 1 突然减小至约 1 6 0 0cm- 1 .通过分析 ,在光解能量小于 32 0 0 0cm- 1 的区域 ,解离通道为NO (X1 Σ ) N(4 S) ;而在光解能量大于 32 0 0 0cm- 1 的区域 ,另一个具有较高解离限的解离通道 ,NO (X1 Σ ) N(2 D) ,开启并完全取代N(4 S)通道成为解离的惟一通道 .根据实验结果 ,对在所研究的光解能量范围内的N2 O 离子A2 Σ 电子态预解离机理进行了探讨     

Accurate potential energy function and spectroscopic study of the X~2Σ~+,A~2Ⅱ and B~2Σ~+ states of the CP radical

This paper calculates the equilibrium internuclear separations,the harmonic frequencies and the potential energy curves of the X 2 Σ +,A 2Ⅱ and B 2 Σ + states of the CP radical by the highly accurate valence internally contracted multireference configuration interaction method with correlation-consistent basis sets(aug-cc-pV6Z for C atom and aug-cc-pVQZ for P atom).The potential energy curves are all fitted with the analytic potential energy function by the least-square fitting.Employing the analytic potential energy function,we determine the spectroscopic constants(B e,α e and ω e χ e) of these states.For the X 2 Σ + state,the obtained values of D e,B e,α e,ω e χ e,R e and ω e are 5.4831 eV,0.792119 cm 1,0.005521 cm 1,6.89653 cm 1,0.15683 nm,12535.11 cm 1,respectively.For the A 2Ⅱ state,the present values of D e,B e,α e,ω e χ e,R e and ω e are 4.586 eV,0.703333 cm 1,0.005458 cm 1,6.03398 cm 1,0.16613 nm,1057.89 cm 1,respectively.For the B 2 Σ + state,the present values of D e,B e,α e,ω e χ e,R e and ω e are 3.506 eV,0.677561 cm 1,0.00603298 cm 1,5.68809 cm 1,0.1696 nm,822.554 cm 1,respectively.For these states,the vibrational states with the rotational quantum number J equals zero(J = 0) are studied by solving the radial nuclear Schro¨dinger equation using the Numerov method.For each vibrational state,the vibrational level,the classical turning points,the rotational inertial and the centrifugal distortion constants are calculated.Comparison is made with recent theoretical and experimental results.     

CN（B~2Σ~＋）激发态光谱的研究

研究亚稳态原子Ｈｅ（２３Ｓ）与ＣＨ３ＣＮ的能量转移反应，获得了ＣＮ（Ｂ２Σ＋－Ｘ２Σ＋）的近紫外辐射光谱。根据光谱强度，研究了ＣＮ（Ｂ２Σ＋）的形成速率和振动布居，并探讨了传能反应机理。     

BS分子α带系A~2Π→X~2Σ~+及γ带系C~2Π→X~2Σ~+法兰克-康登因子的计算

在双原子分子核运动的薛定谔方程中，计入分子的振转相互作用项，在Ｍｏｒｓｅ势近似下得出的波函数除与振动量子数有关外，还与转动量子数有关。本文用该波函数编程计算了ＢＳ分子α带系Ａ２Π→Ｘ２Σ＋及γ带系Ｃ２Π→Ｘ２Σ＋法兰克－康登（Ｆｒａｎｃｋ－Ｃｏｎｄｏｎ）因子（简称Ｆ－Ｃ因子）。计算中转动量子数的取值由Ｊ＝０至Ｊ＝２００，其结果适用于低温、高温和强激波条件。     

HF的电子态X~1Σ~＋和B~1Σ~＋之势能函数和Δυ＝2泛频跃迁精细结构

用Ｍｕｒｒｅｌｌ—Ｓｏｒｂｉｅ函数表述ＨＦ（Ｘ１Σ＋和Ｂ１Σ＋）的势能函数。通过对ＨＦ振转能级的计算，得到Δｖ＝２泛频跃迁精细结构，所得结果中，基态之Ｐ支与Ｗ．Ｑ．Ｊｅｆｆｅｒｓ发表的实验结果进行了比较。     

Spectroscopic parameters and molecular constants of HI(X~1Σ~+),DI(X~1Σ~+) and TI(X~1Σ~+) isotope molecules

The potential energy curve (PEC) of HI(X¹Σ⁺) molecule is studied using the complete active space self-consistent field method followed by the highly accurate valence internally contracted multireference configuration interaction approach at the correlation-consistent basis sets, aug-cc-pV6Z for H and aug-cc-pV5Z-pp for I atom. Using the PEC of HI(X¹Σ⁺), the spectroscopic parameters of three isotopes, HI(X¹Σ⁺), DI(X¹Σ⁺) and TI(X¹Σ⁺), are determined in the present work. For the HI(X¹Σ⁺), the values of D₀, D_e, R_e, ω_e, ω_eχ_e, α_e and B_e are 3.1551 eV, 3.2958 eV, 0.16183 nm, 2290.60 cm^-1, 40.0703 cm^-1, 0.1699 cm^-1 and 6.4373 cm^-1, respectively; for the DI (X¹Σ⁺), the values of D₀, D_e, R_e, ω_e, ω_eχ_e, α_e and B_e are 3.1965 eV, 3.2967 eV, 0.16183 nm, 1626.8 cm^-1, 20.8581 cm^-1, 0.0611 cm^-1 and 3.2468 cm^-1, respectively; for the TI (X¹Σ⁺), the values of D₀, D_e, R_e, ω_e, ω_eχ_e, α_e and B_e are of 3.2144 eV, 3.2967 eV, 0.16183 nm, 1334.43 cm^-1, 14.0765 cm^-1, 0.0338 cm^-1 and 2.1850 cm^-1, respectively. These results accord well with the available experimental results. With the PEC of HI(X¹Σ⁺) molecule obtained at present, a total of 19 vibrational states are predicted for the HI, 26 for the DI, and 32 for the TI, when the rotational quantum number J is equal to zero (J = 0). For each vibrational state, vibrational level G(?), inertial rotation constant B_? and centrifugal distortion constant D_? are determined when J = 0 for the first time, which are in excellent agreement with the experimental results.     

Σ-N相互作用的研究及_Σ~4He结合能的计算

基于SU(3)夸克模型,用共振群方法研究了两种理论下的Σ-N相互作用,得到了它们的相互作用非定域位以及Σ超子与3He壳心核的相互作用势,并在此基础上计算了4ΣHe基态结合能。计算结果表明,SU(3)夸克模型能较好地描述两种理论下的Σ-N相互作用及Σ超子与3He壳心核的相互作用势,同时由其得到的Σ4He基态结合能也与实验值基本相吻合。     

弯曲振动对CS_2分子~1B_2(~1Σ_u~+)态预解离寿命的影响

在209.5～216nm,采用光解碎片激发(PHOFEX)谱技术,对CS2分子1B2(1Σ+u)态预解离寿命进行了 考察.测量在超声射流中进行.信号来自解离碎片CS(A1Π,v′=0←X1Σ+,v″=0)Q支带头的激光诱导荧光 (LIF).预解离寿命是通过对谱带进行拟合来提取的.拟合中假定基态转动布居为Boltzmann分布,寿命加宽的转 动谱线为Lorentz线形.通过拟合共获得1B2(1Σ+u)态13个跃迁所对应的预解离寿命,其中6个数据是新得到的. 结果表明,基态振动角动量量子数l或激发态转动角量子数K(K=l)对预解离寿命有明显的影响.对于激发态的 同一振动能级,较大的K对应于较短的预解离寿命.实验中采用可加热的射流喷嘴,用以提高热带激发的强度, 以改善对较大转动角量子数K的影响的考察.     

碰撞诱导振动能量转移K_2[1~1Σ_u~+(v′=2)]+He,H_2→K2[1~1Σ_u~+(v′=1,3)]+He,H_2

在样品池条件下,利用激光诱导荧光方法研究了K2[11Σ+u(v′=2)]+He,H2→K2[11Σ+u(v′=1,3)]+He,H2的碰撞能量转移。池温保持在420 K,He和H2气压在40~250 Pa之间变化。脉冲激光激发K2基态至11Σ+u(v′=2)态,荧光中含有直接和碰撞转移荧光成分,记录直接11Σ+u(v′=2)→11Σ+g(v″=0)荧光发射的时间分辨强度。在发射开始时v′=2能级的布居未受v′=1,3→v′=2碰撞转移的影响,因此光强为一纯指数曲线,从强度的对数值给出的直线斜率得到有效寿命,由Stern-Volmer方程得到v′=2→v″=0的辐射寿命为(36±7)ns,v′=2与He和H2碰撞的总的转移截面分别为(3.0±0.5)×10-16cm2和(6.4±1.2)×10-15cm2。在不同的He和H2气压下,测量v′=1,2,3→v″=0的时间积分荧光强度,结合11Σ+u(v′=1,3)能量辐射率的测量,得到了v′=2→v′=1和v′=2→v′=3的碰撞转移面分别为(1.4±0.5)×10-16cm2,(1.2±0.4)×10-16cm2(对K2+He)和(3.2±1.0)×10-15cm2,(2.6±0.9)×10-15cm2(对K2+H2)。     

State-to-state quantum dynamics of the N(~4S)+H_2(X~1Σ~+) → NH(X~3Σ~-)+H(~2S) reaction and its reaction mechanism analysis

Quantum state-to-state dynamics of the N(4S) + H-2(X1+Σ) → NH(X3Σ) + H(2S) reaction is reported in an accurate novel potential energy surface constructed by Zhai et al.(2011 J. Chem. Phys. 135 104314). The time-dependent wave packet method, which is implemented on graphics processing units, is used to calculate the differential cross sections. The influences of the collision energy on the product state-resolved integral cross sections and total differential cross sections are calculated and discussed. It is found that the products NH are predominated by the backward scattering due to the small impact parameter collisions, with only minor components being forward and sideways scattered, and have an inverted rotational distribution and no inversion in vibrational distributions; both rebound and stripping mechanisms exist in the case of high collision energies.     

碰撞诱导钠分子 A~1Σ_u~ →Χ~1Σ_g~ 的荧光光谱

用532 0nm激光激发Na2分子到B1Πu电子态,记录了Na(3P)原子的跃迁和Na2分子的A1Σ u-Χ1Σ g的谱带。由Na与Na2激发态发射的光谱及其强度可以认定在Na-Na2系统中的碰撞过程,Na(3P)原子线是Na2(B1Πu)到Na(3P)的碰撞能量转移产生的,预解离过程也可产生原子线。而A1Σ u的辐射而引起的。在360℃,u-Χ1Σ g到A1Σ g谱带是由B1Πu到21Σ g的碰撞转移后再由21Σ 根据辐射衰变率和荧光强度,得到Na2(B1Πu)到Na2(21Σ g)碰撞转移率系数为7 1×10-10cm3s-1,而B1Πu的预解离率为2 3×106s-1。     

MgH分子X2Σ+,A2Π和B2Σ+电子态的势能函数

利用QCISD(T),SAC-CI方法和cc-pVQZ,aug-cc-pVTZ,6-311 G及6-311 G(3df,2pd)基组,对MgH分子的基态X2Σ ,第一简并激发态A2Π和第二激发态B2Σ 的结构进行优化计算.通过对4个基组计算结果进行比较,得出6-311 G(3df,2pd)基组为最优基组.使用6-311 G(3df,2pd)基组和QCISD(T)方法对基态X2Σ ,SAC-CI方法对激发态A2Π和B2Σ 进行单点能扫描计算,然后采用Murrell-Sorbie函数及修正的Murrell-Sorbie C6函数进行拟合,得到了相应电子态的势能函数参数和对应的光谱常数.计算结果表明,用修正的Murrell-Sorbie C6函数计算得到的MgH分子基态和第一简并激发态的光谱常数ωe,ωexe,Be,αe与实验数据吻合很好.表明修正后的Murrell-Sorbie C6函数能更为准确地描述MgH分子的基态和第一激发态的势能函数.     

State-to-state dynamics of F(~2P) + HO(~2Π) → O(~3P) + HF(~1Σ~+)reaction on 1~3A〞 potential energy surface

State-to-state time-dependent quantum dynamics calculations are carried out to study F(~2P) + HO(~2Π) → O(~3P) +HF(~1Σ~+) reaction on 1~3A〞 ground potential energy surface(PES). The vibrationally resolved reaction probabilities and the total integral cross section agree well with the previous results. Due to the heavy–light–heavy(HLH) system and the large exoergicity, the obvious vibrational inversion is found in a state-resolved integral cross section. The total differential cross section is found to be forward–backward scattering biased with strong oscillations at energy lower than a threshold of 0.10 eV, which is the indication of the indirect complex-forming mechanism. When the collision energy increases to greater than 0.10 eV, the angular distribution of the product becomes a strong forward scattering, and almost all the products are distributed at θ_t = 0°. This forward-peaked distribution can be attributed to the larger J partial waves and the property of the F atom itself, which make this reaction a direct abstraction process. The state-resolved differential cross sections are basically forward-backward symmetric for v' = 0, 1, and 2 at a collision energy of 0.07 eV; for a collision energy of 0.30 eV,it changes from backward/sideward scattering to forward peaked as v increasing from 0 to 3. These results indicate that the contribution of differential cross sections with more highly vibrational excited states to the total differential cross sections is principal, which further verifies the vibrational inversion in the products.     

Mechanism analysis of reaction S~+(~2D)+H_2(X~1Σ_g~+) → SH~+(X~3Σ~-) + H(~2S) based on the quantum state-to-state dynamics

We present a state-to-state dynamical calculation on the reaction S~++ H_2→ SH~+ +H based on an accurate ~X2 A~″ potential surface. Some reaction properties, such as reaction probability, integral cross sections, product distribution, etc.,are found to be those with characteristics of an indirect reaction. The oscillating structures appearing in reaction probability versus collision energy are considered to be the consequence of the deep potential well in the reaction. The comparison of the present total integral cross sections with the previous quasi-classical trajectory results shows that the quantum effect is more important at low collision energies. In addition, the quantum number inversion in the rotational distribution of the product is regarded as the result of the heavy–light–light mass combination, which is not effective for the vibrational excitation. For the collision energies considered, the product differential cross sections of the title reaction are mainly concentrated in the forward and backward regions, which suggests that there is a long-life intermediate complex in the reaction process.