卤素双原子分子部分电子态的完全振动能谱和离解能

用代数方法(AM)可以获得双原子分子包含最高振动能级在内的所有高阶振动能级的完全振动能谱; 基于Leroy和Bernstein的能级表达式, 研究了卤族元素双原子分子Cl2-A’3∏(2u)、Br2-X1∑+g和I2-0+u电子态的完全振动能谱和离解能, 得到的理论结果与实验符合得很好.     

HXeBr分子的振动频率和离解途径的理论研究

采用MP2和CCSD(T)方法对HXeBr分子的振动光谱进行了理论研究. 计算结果表明, 经非谐性和基质效应修正后的H—Xe伸缩振动、弯曲振动以及Xe—Br伸缩振动频率分别为1492, 509和174 cm-1, 与实验结果吻合得较好. 此外分别采用单参考组态的CCSD(T)方法和多参考组态耦合簇(MR-AQCC)方法研究了HXeBr分子的稳定性和离解途径. 研究结果表明, 离解途径HXeBr→Xe＋HBr和HXeBr→H＋Xe＋Br的能垒分别为1.39和0.89 eV, 三体离解途径是HXeBr分子的主要离解途径.     

低初始振动激发van der Waals分子HeI_2振动预离解三维含时波包动力学研究

用含时黄金规则波包法,计算了低初始振动激发HeI_2分子振动预离解总和分衰变宽度,寿命和速率及它们随初始振动态υ的变化.计算结果与实验外推数据符合得相当好.计算所需很短的波包总传播时间(不超过1ps)是由离解碎片在振动去激发绝热势能面(υ-1)上驻留时间决定的.较强的终态相互作用的影响是很重要的.预言并解释了终转动态分布随着υ的移动而改变的动力学规律.     

面向有机光电材料的电子激发态结构与过程的计算方法

共轭聚合物与有机分子材料中的电子激发结构与过程决定了材料的光电功能：根据Kasha规则,低能级激发态的排序决定能否发光;最低激发态至基态的辐射跃迁与无辐射跃迁之间的竞争决定了发光效率,后者主要由非绝热耦合（声子作用）决定;电荷激发态载体的传输由电子分布与振动耦合或杂质和无序的散射弛豫过程决定．本文针对有机功能材料的发光性能,介绍两种理论方法的研究进展,即可用于计算共轭聚合物激发态结构的量子化学密度矩阵重整化群方法和计算发光效率的多模耦合无辐射跃迁速率方法．这些方法被应用于有机功能材料的性能预测和分子设计中．     

复合物C6H5CH3…Ar分子间的外部振动频率

利用双光子共振电离光谱和飞行时间质谱技术在超声分子束中观察到C6H5CH3…Ar的振动光谱.借助同位素光谱效应、内转动能级和分子间振动能级的理论计算,合理地归属了涉及CH3转动和Ar原子振动的光谱,并由此获得复合物分子间各种模式的振动频率.     

水分子配位对叶绿素a氧化还原势与红外光谱的影响

以光系统I反应中心电子传递链上的辅助叶绿素a为目标,采用密度泛函理论中的B3LYP方法,结合三种基组,系统计算了该叶绿素及其两种配位分子模型在气相、模拟蛋白质环境和水中的氧化还原势和离解能;同时计算了这三种模型在气相中的几何结构、红外光谱及其13C、15N和2H的同位素标记谱.计算及分析结果表明:水分子配位引起镁离子偏离叶绿素a的卟啉环平面中央,导致以镁原子为中心的键角减小,Mg—N键长增长;而天冬酰胺对配位的水分子施加氢键影响后,使得Mg—N键进一步增长,镁离子与水分子中氧原子的配位键Mg—O键长减小,离解能增加,合成分子的氧化还原势减少;另外,分子的氧化还原势和配位键离解能随着相对介电常数的增加以及计算基组的增大而减小;三种分子模型的羰基(C襒O)和卟啉环上C襒C键的特征振动频率差值小于7cm-1,而同位素标记引起其峰位变化量的差值小于3cm-1.该计算为研究光合反应中心电子传递链上叶绿素a的作用与功能提供理论参考依据.     

双原子分子振动对热力学性质的影响

本文在分析了双原子分子振动能级的完备性和有限性及其对统计计算带来的影响的基础上,借助代数（AM）方法得到的双原子分子振动能级完全集合,采用量子力学统计系综方法,讨论了双原子分子振动能量对宏观热力学性质的统计贡献,并以氮气为例计算了相应的热力学函数和振动热容量．结果表明,真实的双原子分子振动能级是有限的;确定最高振动量子数和振动能级完全集合是正确进行统计分析的基础和关键;考虑振动能级的完备性和有限性后,只能导致数值解而不是解析解,所得的结果优于谐振子模型的解析结果,与实验数据吻合得很好．     

D_2在Ni(100)表面离解吸附的量子动力学研究

用量子含时波包法研究了Ｄ２在镍表面顶－桥位上离解吸附量子动力学．计算了不同入射动能及初始振转态的离解几率．讨论了分子的同核对称性、转动取向和振动激发对离解几率的影响，并与其他理论计算结果做了比较．     

尿素分子振动光谱的密度泛函理论研究

用密度泛函理论方法BLYP/6-31¹⁺+G(2df,2pd)对尿素分子的平衡几何构型进行了优化,并计算了该分子的谐力场.使用Wilson的GF矩阵方法,对尿素分子的振动基频进行了理论研究.根据振动频率的势能分布对此分子的振动基频进行了理论归属,计算的振动频率和能级指认均同实验结果吻合较好.     

H2SiCl2分子Si-H振动"基座"SiCl2的有效质量

用傅立叶变换光谱仪和激光腔内吸收光谱仪记录了H2SiCl2分子2000～9000和12000～12900 cm-1的红外吸收光谱.依据局域模理论的非谐性耦合非谐振子(ACAO)模型,分析并拟合了Si-H的对称伸缩振动和反对称伸缩振动,得到描述Si-H伸缩振动的Morse离解能De 、 Morse振子参数α和键振子势能耦合系数frr′.分析中忽略了SiCl2"基座"对Si-H伸缩振动的影响,拟合结果与实验值符合的很好,拟合方差小于 1 cm-1,表明这一近似是可取的.分析拟合结果表明, Si-H振动时"基座"SiCl2的有效质量为75.     

Resonant vibrational excitation and de-excitation of CO(v) by low energy electrons

Integral cross sections and rate coefficients for vibrational excitation of the excited carbon-monoxide molecule, via the (2)Pi shape resonance in the energy region from 0 to 5 eV have been calculated. Cross sections are calculated by using our recently measured cross sections for the ground level CO excitation and the most recent cross sections for elastic electron scattering, applying the principle of detailed balance. Rate coefficients are calculated for Maxwellian electron energy distribution, with mean electron energies below 5 eV. By using extended Monte Carlo simulations, electron energy distribution functions (EEDF) and rate coefficients are determined in nonequilibrium conditions, in the presence of homogeneous external electric field. Nonequilibrium rates are calculated for typical, moderate values of the electric field over gas number density ratios, E/N, from 1 to 220 Td. Maxwellian and nonequilibrium rate coefficients are compared and the difference is attributed to a specific shape of the electron energy distribution functions under considered conditions.     

Kinetic processes in non-equilibrium carbon monoxide discharges. I. Vibrational kinetics and dissociation rates

Vibrational distributions and dissociation rates of carbon monoxide under non-equilibrium conditions have been calculated by solving the vibrational master equation coupled to the plasma chemistry and to the Boltzmann equation for the electron energy distribution function. The results show the predominance of a vibrational mechanism in dissociating CO and the strong coupling between the vibrational distribution of CO and the concentration of the species (C, O and CO₂), generated by the dissociation process, due to the large V-T (vibration-translation) energy transfer of these species. Finally the dependence of the vibrational distribution and of the dissociation rates on the recombination is analyzed by means of a simple model which allows the insertion of loss terms for the species C, O and CO₂ in the relevant plasma chemistry equations.     

Electron energy distribution functions and dissociation kinetics of HCl in non-equilibrium plasmas

Electron energy distribution functions (edf) have been calculated by numerically solving the Boltzmann equation coupled to a system of vibrational master equations which simulates both the vibrational relaxation due to e—V (electron—vibration), V—V (vibration—vibration) and V—T (vibration—translation) energy exchanges and the dissociation process. The calculated edf strongly depend on the vibrational nonequilibrium present in the gas phase, even though the atoms coming from the dissociation process tend to destroy the vibrational energy content of the molecules. Vibrationally excited molecules determine a joint vibro—electronic mechanism in the dissociation of HCl. This mechanism is the more efficient the smaller the gas temperature and pressure. Finally the contribution of a purely vibrational mechanism in the dissociation of HCl is presented and discussed.     

A DFT study of the adsorption and dissociation of CO on Fe(100): influence of surface coverage on the nature of accessible adsorption states.

In the present article, we report adsorption energies, structures, and vibrational frequencies of CO on Fe(100) for several adsorption states and at three surface coverages. We have performed a full analysis of the vibrational frequencies of CO, thus determining what structures are stable adsorption states and characterizing the transition-state structure for CO dissociation. We have calculated the activation energy of dissociation of CO at 0.25 ML (ML = monolayers) as well as at 0.5 ML; we have studied the dissociation at 0.5 ML to quantify the destabilization effect on the CO(alpha3) molecules when a neighboring CO molecule dissociates. In addition, it is shown that the number and nature of likely adsorption states is coverage dependent. Evidence is presented that shows that the CO molecule adsorbs on Fe(100) at fourfold hollow sites with the molecular axis tilted away from the surface normal by 51.0 degrees. The asorprton energy of the CO molecule is -2.54 eV and the C-O stretching frequency is 1156 cm(-1). This adsorption state corresponds to the alpha3 molecular desorption state reported in temperature programmed desorption (TPD) experiments. However, the activation energy of dissociation of CO(alpha3) molecules at 0.25 ML is only 1.11 eV (approximately 25.60 kcal mol(-1)) and the gain in energy is -1.17 eV; thus, the dissociation of CO is largely favored at low coverages. The activation energy of dissociation of CO at 0.5 ML is 1.18 eV (approximately 27.21 kcal mol(-1)), very similar to that calculated at 0.25 ML. However, the dissociation reaction at 0.5 ML is slightly endothermic, with a total change in energy of 0.10 eV Consequently, molecular adsorption is stabilized with respect to CO dissociation when the CO coverage is increased from 0.25 to 0.5 ML.     

Application of the Monte Carlo Method to Modeling Kinetic Processes of Polyatomic Molecules and Clusters: II. Kinetics of Unimolecular Reactions of Polyatomic Molecules

The method for statistical modeling of the kinetics of unimolecular decomposition of polyatomic molecules based on the construction of nonequilibrium functions of the distribution over the energies of the vibrational excitation of molecules is developed. The rate constants for the two-channel decomposition of a model molecule depending on temperature and pressure are reported. The relaxation characteristics for the dissociation of the model molecule are determined.     

Vibrational relaxation and collision-induced dissociation of xenon fluoride by neon

Rate coefficients were calculated for vibrational relaxation and collision-induced dissociation of ground state xenon fluoride in neon at temperatures between 300 and 1000 K for each of nine vibrational levels. These coefficients were calculated using a pairwise additive potential energy surface, which consists of a Morse function for the XeF interaction and Lennard–Jones functions for the NeXe and NeF interactions. Rate coefficients are provided for both temperature and v- dependences. The vibrational relaxation and dissociation processes occur by multiquanta transitions. Dissociation can take place from all v-levels provided that the internal energy of the XeF molecule is close to the rotationless dissociation limit. The order of increase effectiveness of the various forms of energy in promoting dissociation in XeF was found to be translation–rotation-vibration. At room temperature, neon atoms were found to be more efficient than helium atoms in the dissociation processes; helium atoms were found to be more efficient than neon atoms in the vibrational relaxation of XeF. Strong vibration–rotation coupling in both vibrational relaxation and in the dissociation processes is demonstrated.     

Semiclassical calculation of energy transfer in polyatomic molecules. VIII. Theory for atom + non-linear triatom

The theory for collision of an atom with a non-linear triatomic molecule is presented and the He + H₂O system considered as an example. It is shown that both anharmonic and Coriolis coupling are important for the energy transfer. Seventeen rate constants for vibrational transitions in H₂O are calculated in the temperature range 300–2000 K.     

A DFT Study on the Stable Structures and Dissociation Mechanism of C3O6 Cluster

Using geometrical optimization and DFT method at the B3LYP/6-31G (d) level, nineteen equilibrium geometries were identified, and three transition states of dissociation reaction of C3O6 clusters were also found. The vibrational frequencies and intrinsic reaction coordinate (IRC) verification at the same level were computed to verify the transitions. And then we calculated the dissociation energies and analyzed the dissociation channels. The computational results show that the dissociation energies of C3O6 isomers relative to three CO2 are between 1.509 × 103 and 10.61 × 103 kJ·kg-1, and the energy barriers of the reactions are 92.857, 131.138 and 185.793 kJ·mol-1. Both the high dissociation energies and high energy barriers show that C3O6 clusters studied in this paper are stable enough to be used as high-energy-density materials.     

Optimal internal coordinates, vibrational spectrum, and effective Hamiltonian for ozone

In this paper the authors use the optimal internal vibrational coordinates previously determined for the electronic ground state of the ozone molecule to study the vibrational spectrum of the molecule employing the second empirical potential energy surface calculated by Tyuterev et al. [Chem. Phys. Lett. 316, 271 (2000)]. First, the authors compute variationally all the bound vibrational energy levels of the molecule up to the dissociation limit and state the usefulness of the optimal coordinates in this respect, which allows us to converge all the bound levels using relatively small anharmonic basis sets. By analyzing the expansion coefficients of the wave functions, they show then that a large portion of the vibrational spectrum of O3 can be structured in nearly separable polyadic groups characterized by the polyad quantum number N=n1+n2+n(theta) corresponding to the optimal internal coordinates. Accordingly, they determine an internal effective vibrational Hamiltonian for O3 by fitting the effective Hamiltonian parameters to the experimental vibrational frequencies, using as input parameters in the fit those extracted from an analytical second-order Van Vleck perturbation theory calculation. It is finally shown that the internal effective Hamiltonian thus obtained accurately describes the vibrational spectrum of ozone in the low and medium energy regimes.