CUO分子结构与势能函数

用密度泛函理论的B3LYP方法,对铀原子采用14个价电子的准相对论有效原子实势及(6s5p2d4f)[3s3p2d2f]收缩价基集合,碳、氧原子采用6311G全电子基集合,应用Gaussian98程序对一氧化碳气体与铀表面相互作用的可能分子结构CUO(角形Cs和线形C∞v构型)分子进行几何优化计算,得到了稳定结构的几何构形、能量、谐振频率、力学性质和电性质,并用微观可逆性原理分析了其可能的离解极限.结果表明,势能函数等值势能面图能清晰地再现CUO分子的结构特征和离解能;铀原子与一氧化碳的反应是势垒较低、容易进行的反应 关键词： CUO 密度泛函理论 分子结构 势能函数     

铀碳氧系统分子结构的DFT计算

用密度泛函理论(DFT)的Bexke3lyp方法,对铀原子采用相对论有效原子实势及(6s5p2d4f)/[3s3p2d2f]收缩价基集合,碳、氧原子采用6-311G价基集合,应用Gaussian98程序对一氧化碳气体与铀表面相互作用的可能分子结构U-C-O、U-O-C、C-U-O(角形Cs和线形C∞v)等,进行abinitio优化计算.得到了十二种三重态或五重态的相对稳定结构的电子状态、几何构形、能量、谐振频率、力学性质和电性质等,并给出了角形和线形结构的正则振动分析图.结果表明,Cs构型的能量都比较低,尤其以U-C-O角形结构(3A″)为最低;通过对各成键原子间重叠布居数及键能分析知,U与CO的结合力较弱,O原子比C原子与U原子的结合力稍强.     

YFe2B2电子结构的第一性原理计算

基于密度泛函理论,从头计算了具有ThCr₂Si₂型四方晶系的稀土金属化合物Yfe₂B₂体相的物理特性.能量计算结果表明Yfe₂B₂体相处于顺磁金属态;而能带结构、态密度、布居数以及差分电荷　分布的计算结果表明Y原子的5s,5p电子具有很强的局域性;Fe原子的3d电子和B的1s,2s和2p电子强烈耦合,使得最近邻Fe原子与B原子形成了Fe—B共价键;最近邻的两个Fe原子之间由于 关键词： 稀土金属化合物 第一性原理计算 能带结构 态密度     

OsSi2电子结构和光学性质的研究

采用基于第一性原理的密度泛函理论赝势平面波方法,对正交相OsSi₂的电子结构、态密度和光学性质进行了理论计算,能带结构计算表明它是一种间接带隙半导体,禁带宽度为0813 eV;其价带主要由Os的5d和Si的3p态电子构成;导带主要由Si的3s,3p以及Os的5d态电子构成;静态介电常数ε₁（0）=1543; 折射率n＝393并利用计算的能带结构和态密度分析了OsSi₂的介电函数、吸收系数、折射率、反射率、 关键词： 2')" href="#">OsSi₂ 第一性原理 电子结构 光学性质     

锕系双原子分子的从头算研究

用相对论有效原子实势（RECP）和密度泛函方法（B3LYP）,采用U和Pu原子的紧缩价基集合[5s4p3d4f]/[3s3p2d2f],优化了U2和Pu2分子的平衡结构,得到它们的键长（LBL）和短键长（SBL）分别为：U2分子是0．38965和0．29927nm,Pu2分子是0．45375和0．35202nm;导出了基态和最低激发态的势能函数,计算出它们的力常数、光谱数据和离解能。     

含酯基和吡啶环苯并菲衍生物分子的电荷传输和三阶非线性光学性质

采用密度泛函理论在B3LYP/6-31G**理论水平计算研究含酯基和吡啶环的苯并菲衍生物分子的电荷传输速率．结果表明，酯基双取代的苯并菲衍生物分子具有较高的空穴和电子传输速率，分别为0.22 cm2/v•s和1.51 cm2/v•s．同时引入酯基和吡啶环均不利于空穴和电子传输．使用有限场(FF)方法计算分子的三阶非线性光学性质．结果显示，在酯基和吡啶环之间引入柔性碳链的分子与不含吡啶环分子的三阶非线性光学性质基本一致，均具有较高的电荷传输速率和良好的三阶非线性光学性质．     

取代基对8-羟基喹啉金属配合物电子光谱和二阶非线性光学性质的影响

在B3LYP/LANL2DZ/6-31G^*水平上优化目标化合物分子的几何结构,并分别在TD- B3LYP/LANL2DZ/6-31++G^**和B3LYP/LANL2DZ/6-31++G^**水平计算目标化合物分子的电子吸收光谱和二阶非线性光学性质.计算结果表明,引入共轭给电子基使配合物分子的最大吸收波长红移,强共轭吸电子基的引入使配合物的最大吸收波长蓝移,取代基的引入使IrQ₃型配合物的二阶非线性光学性质明显增大.对AgQ型配合物,电子跃迁属于配体内部的电荷转移（LLCT）.对PtQ₂和IrQ₃型配合物,电子跃迁属于LLCT和部分金属向配体的电荷转移.取代基对AgQ,PtQ₂,IrQ₃型配合物分子的跃迁性质几乎无影响. 关键词： 8-羟基喹啉金属配合物 电子光谱 二阶非线性光学性质 密度泛函理论     

硅基外延OsSi2电子结构及光电特性研究

基于第一性原理密度泛函理论的赝势平面波方法,对Si（111）基外延稳定正交相OsSi₂的能带结构、态密度以及光电特性进行了研究.研究结果表明,Si（111）基外延稳定正交相的OsSi₂是一种间接带隙半导体,禁带宽度为0.625 eV;其价带主要是由硅的3s,3p态电子和锇的5d态电子构成,导带主要由锇的5d态电子与硅的3s,3p态电子构成;其静态介电函数为15.065,折射率为3.85,吸收系数最大峰值为3.9665×10⁵cm^-1.利用理论计算的能带结构和态密度研究了Si（111）基外延稳定正交相OsSi₂的介电函数、折射率、吸收系数、光电导率和能量损失函数的变化规律,为Si（111）基外延OsSi₂的应用提供了理论基础.     

新型含氧亚甲基和亚胺桥键液晶化合物分子结构与光谱的密度泛函理论研究

采用密度泛函理论方法在B3LYP/6-31G*水平上对6个新型含氧亚甲基和亚胺桥键液晶化合物分子的几何结构进行优化计算,讨论了取代基H,CH3,CH3O,C2H5O,NO2,Cl对分子电荷、前线轨道能量和电子吸收光谱等性质的影响.在此基础上使用含时密度泛函理论方法计算了分子第一激发态的电子垂直跃迁能,得到最大吸收波长λmax.计算表明,取代基的引入导致最大吸收波长红移.     

铀的原子模型

在U价电子采用(5s4p3d4f)/[3s3p2d2f]收缩基函数,原子实采用相对论原子实势进行处理的条件下,通过B3LYP杂化交换-相关泛函对U₂分子的电子态和势能数据进行了第一性原理计算．结果表明U₂分子的基态电子态为X⁹∑⁺_g ．同时用Murrell-Sorbie解析势能函数对对势数据进行拟合．在自旋极化水平和广义梯度近似下,采用密度泛函理论(DFT)和Perdew-Burke     

Highly accurate coupled-cluster singlet and triplet pair energies from explicitly correlated calculations in comparison with extrapolation techniques

Coupled-cluster singles and doubles (CCSD) valence shell correlation energies of the systems CH₂ (<¹A₁ state), H₂O, HF, N₂, CO, Ne, and F₂ are computed by means of standard calculations with correlation-consistent basis sets of the type cc-pVxZ (x = D, T, Q, 5, 6) and by means of explicitly correlated coupled-cluster calculations (CCSD-R12/B) with large uncontracted basis sets of the type 19s14p8d6f4g3h for C, N, O, F, and Ne and 9s6p4d3f for H. These CCSD-R12/B calculations provide reference values for the basis set limit of CCSD theory. The computed correlation energies are decomposed into singlet and triplet pair energies. It is established that the singlet pair energies converge as X^?3 and the triplet pair energies as X^?5 with the cardinal number of the correlation-consistent basis sets, and an extrapolation technique is proposed that takes into account their different convergence behaviour. Applied to the cc-pV5Z and cc-pV6Z results, this new extrapolation yields pair energies with a mean absolute deviation of 0.02 mE_h from the CCSD-R12/B reference values. For the seven systems under study, the extrapolated total valence shell correlation energies agree to within 0.2 mE_h with the CCSD-R12/B benchmark data.     

Chromium dihydride (CrH2): theoretical evidence for a bent 5B2 ground state

Ab initio molecular electronic structure theory has been used to study two likely candidates for the quintet ground state of CrH₂ at the self-consistent field, the single and double excitation configuration interaction (CISD), the single and double excitation coupled cluster (CCSD), and the single, double, and perturbative triple excitation coupled cluster (CCSD(T)) levels of theory. The largest basis sets utilized for geometry optimizations, designated two-f TZ2P, have a contraction scheme of Cr(14s11p6d2f/10s8p3d2f), H(5s2p/3s2p). At the CCSD(T) level of theory using this two-f TZ2P basis, a bent (C_2v symmetry) ⁵B₂ state is predicted to lie a mere 4·2 kcal mol^-1 (4·5 kcal mol^-1 including zero-point vibrational energy correction) lower in energy than linear (D_∞h symmetry) ⁵Σ_g ⁺ HCrH. Theoretical predictions for the equilibrium geometry, harmonic vibrational frequencies, and isotopic frequency shifts of the ⁵B₂ state compare favourably with the results of recent matrix isolation FT-IR work by Xiao, Hauge, and Margrave. The two-f TZ2P CCSD(T) optimized geometry of ⁵B₂ CrH₂ is r _e = 1·658 Å and ?_e = 114·4° (118° ± 5° is the experimentally estimated bond angle), while the harmonic vibrational frequencies are ω₁(a₁) = 1710, ω₂(a₁) = 582, and ω₃(b₂) = 1683 cm^-1 (experimentally assigned fundamentals in an argon matrix are the symmetric stretch 1651 cm^-1 and asymmetric stretch 1615 cm^-1). Isotopic frequency shifts of CrD₂ relative to CrH₂ are Δω₁(a₁) = -492 and Δω₃(b₂) = -477 cm^-1 (compared with symmetric stretch -462 cm^-1 and asymmetric stretch -448-cm^-1 from experiment).     

Determination of the 5d6p 3F4-5d2 3F transition probabilities of Ba I

Whether the transitions between 6s5d ³D and 5d6p ³F can be used for laser cooling of barium heavily depends upon the transition probabilities of 5d6p ³F-5d^{2 3}F. Taking the transition 6s5d ³D₃-5d6p ³F⁴ as a scale, the leakage rate of 5d6p ³F₄-5d^{2 3}F was used to evaluate the transition probabilities. 706 nm laser pulses with different durations were applied to a barium atomic beam for 6s5d ³D₃-5d^{2 3}F₄ optical pumping, and the remaining percentages in 6s5d ³D₃ were measured. After exponential fitting, the transition probability of 5d6p ³F₄-5d^{2 3}F_3,4 was determined to be 2.1(4)×10⁴ s^?1, which is in agreement with theoretical calculations using the scaled Thomas-Fermi-Dirac method.     

Revised and extended analysis of Br VI

The spectrum of five times ionized bromine (Br VI) has been studied in the 150–2060 Å wavelength region. The spectrum was recorded on a 3-m normal incidence vacuum spectrograph at the Antigonish laboratory (Canada) and 6.65-m grazing incidence spectrograph at the Zeeman laboratory (Amsterdam) using a triggered spark light source. The ground configuration of Br VI is 3d¹⁰4s² and the excited configurations 3d¹⁰4s (4p+5p+6p+7p+4f+5f)+3d¹⁰4p4d+3d¹⁰4p5s in the odd parity system and 3d¹⁰4s (4d+5d+6d+5s+6s+7s+8s+5g+6g)+3d¹⁰4p² in the even parity system have been studied. Relativistic Hartree–Fock (HFR) and least squares fitted (LSF) parametric calculations were used to interpret the observed spectrum. Sixty-eight levels of Br VI have now been established, out of which 28 are new levels. Two previously reported levels viz. 4p4d ¹D₂ and ³F₄ were revised. Among one hundred and fifty-eight spectral lines, 69 are newly classified. The accuracy of our wavelength measurements for sharp and unblended lines is ±0.005 Å. The value of the ionization potential has been determined as 704850±200 cm^?1 (87.390±0.025 eV).     

Potential energy functions for the ground state X3Σ- and excited state 1Σ+ of UO

Based on group theory and atomic and molecular reactive statics (AMRS), the ground state X³Σ^? and excited state ¹Σ⁺ of UO and their reasonable dissociation limits are derived successfully. Using the MP2 method with the relativistic e? ective core potential and valence electron basis set (5s4p3d4f)/[3s3p2d2f] for the U atom and basis set 6-311G* for the O atom, the present work has calculated the potential energy curves for the ground state Χ³Σ^? and excited state ¹Σ⁺ of UO. The equilibrium distance and dissociation energy are 0.1833 nm and 6.9241 eV for the Χ³Σ^? state, and 0.1825 nm and 8.8756eV for the ¹Σ⁺ state. Spectroscopic data are derived for the first time.     

The vertical spectrum of H2CO revisited: (SC)2-CI and CC calculations

The vertical electronic spectrum of formaldehyde has been studied by means of (SC)²-MR-SDCI and CCLR methods. Two basis sets of atomic natural orbitals (ANOs) complemented with a one-centre series of Rydberg orbitals were used. The first was taken from the CASPT2 study by Merchán, M., and Roos, B. O., 1995, Theoret. Chim. Acta, 92, 221, and may be described as C,O[4s3pld]/H[2slp] with a lslpld Rydberg series centred in the charge centroid of the ²B₂ state of the cation. The second was a larger basis set that may be described as C,O[6s5p3d2f]/H[4s3p2d] + 3s3p3d in the same centre. The (SC)² dressing may be applied efficiently to an MR-SDCI method and comparison with the dressed CAS-SDCI is satisfactory, in spite of the remarkable reduction in the CI space dimension. The consistency of the (SC)²-MR-SDCI results was tested also against the CCLR and CASPT2 results using the same basis sets and against the CCLR results using Dunning's aug- and daug-cc-pVQZ basis sets. The ³A₁(π → π *) state is correctly placed as the second excited triplet while the highly multi-configurational nature of the ¹A₁(π → π *) state is confirmed as well as its greatly mixed valence-Rydberg nature. This state is predicted as lying under the 10 eV level, on top of the (n_y → 3d) Rydberg states that are predicted in the 8.9–9.5eV region. The 5 ¹B₂(n^y → 4s) Rydberg state and the ¹B₂(σ_y → π*) also are predicted in this region. The triplet states also were calculated with the (SC)²-MR-SDCI method. The vertical ordering of the 2 ¹A₁(n_y → 3p_y) and 2 ¹B₂(n_y → 3p_z) states is discussed, as well as that of the ¹B₁(σ → π*) and the Rydberg ¹B₁(n_y → 3d_xy) states. This work shows the highly reliable values that may be reached applying the dressing method along with a large basis set. Such a procedure is made possible using an MR-SDCI selection of spaces instead of the CAS-SDCI that was used up to now in most (SC)² dressing applications.     

Two-photon spectroscopy of ytterbium

Two-photon laser spectra of the Yb vapor have been obtained. Transitions to highly excited 4f¹⁴ 6sns¹S₀ and 4f¹⁴ 6snd ¹D₂ states are seen in direct two-photon excitation. Hybrid resonances involving 4f¹⁴ 6s6p ¹P⁰₁ and 4f¹⁴ 5d6s ³D₂ intermediate states lead to transitions to 4f¹⁴ 6sns¹S₀, 4f¹⁴ 6snp ³P⁰_2,1 and 4f¹⁴ 6snd ¹D₂ levels.     

The electronic structures of the core and valence ion states of metal oxides

SCF-Xα SW MO calculations on metal core ion hole states and X-ray emission (XES) and X-ray photoelectron (XPS) transition states of the non- transition metal oxidic clusters MgO₆^10?, AlO₄^5? and SiO₄^4? show relative valence orbital energies to be virtually unaffected by the creation of valence orbital or metal core orbital holes. Accordingly, valence orbital energies derived from XPS and XES are directly comparable and may be correlated to generate empirical MO diagrams. In addition, charge relaxation about the metal core hole is small and valence orbital compositions are little changed in the core hole state. On the other hand, for the transition metal oxidic clusters FeO₆^10?, CrO₆^9? and TiO₆^8? relative valence orbital energies are sharply changed by a metal core orbital or crystal field orbital hole, the energy lowering of an orbital increasing with its degree of metal character. Consequently O 2p nonbonding → M 3d-O 2p antibonding (crystal field) energies are reduced, while M 3d bonding → O 2p nonbonding and M 3d-O 2p antibonding → M 4s,p-O 2p antibonding (conduction band) energies increase. Charge relaxation about the core hole is virtually complete in the transition metal oxides and substantial changes are observed in the composition of those valence orbitals with appreciable M 3d character. This change in composition is greater for e _g than for t_2g orbitals and increases as the separation of the e_g crystal field (CF) orbitals and the O 2p nonbonding orbital set decreases. Based on the hole state MO diagrams the higher energy XPS satellite in TiO₂ (at about 13 eV) is assigned to a valence → conduction band transition. The UV PES satellites at 8.2 eV in Cr₂O₃ and 9.3 eV in FeO are tentatively assigned to similar transitions to conduction band orbitals, although the closeness in energy of the crystal field and O 2p nonbonding orbitals in the valence orbital hole state prevents a definite assignment on energy criteria alone. However the calculations do clearly show that charge transfer transitions of the e_g bonding → e_g crystal field orbital type would generally occur at lower energy than is consistent with observed satellite structure.A core electron hole has little effect upon relative orbital energies and is only slightly neutralized by valence electron redistribution for MgO and SiO₂. For the transition metal oxides a core hole lowers the relative energies of M3d containing orbitals by large amounts, reducing O → M charge transfer and increasing M 3d crystal field → conduction band energies. Large and sometimes overcomplete neutralization of the core hole is observed, increasing from CrO₆^9? to FeO₆^10? to TiO₆^8?. as the O → M charge transfer energy declines.High energy XPS satellites in TiO₂ may be assigned to O 2p nonbonding → conduction band transitions while lower energy UV PES satellites in FeO and Cr₂O₃ arise from crystal field or O 2p nonbonding → conduction band excitations. Our “shake-up” assignment for FeO₆^10?, CrO₆^9? and TiO₆^8? are less than definitive because no procedure has yet been developed to calculate “shake-up” intensities resulting from transitions of the type described. However the results do allow a critical evaluation of earlier qualitative predictions of core and valence hole effects. First, we find that the comparison of hole or valence state ionic systems with equilibrium distance systems of higher nuclear and/or cation charge (e.g. the comparison of the FeO₆^10? Fe 2p core hole state to Co₃O₄) is dangerous. For example, larger MO distances in the ion states substantially reduce crystal field splittings. Second, core and CF orbital holes sharply reduce O → M charge transfer energies, giving 2e_g → 3e_g energy separations which are generally too small to match observed satellite energies. Third, highest occupied CF-conduction band energies are only about 4–5 eV in the ground states, but increase to about 7–11 eV in the core and valence hole states of the transition metal oxides studied. The energetic arguments presented thus support the idea of CF and/or O 2p nonbonding → conduction band excitations as assignments for “shake-up” satellites, at least in oxides of metals near the beginning of the transition series.     

Theoretical study of the CH3 + NS and related reactions: mechanism of HCN formation

More than thirty equilibrium and transition structures on the [CH₃NS] potential energy surface have been located using the B3LYP/6-311 + + G(d,p) method. Thioformaldoxime (3) turns out to be the most stable isomer followed by thionitrone (2), a three-membered ring, thionitrosyl methane (1) and thiazyl methane. These isomers are connected to each other by 1,2H and 1,3H shifts and ring—chain rearrangement, but the associated energy barriers are rather high, making most of them stable with respect to unimolecular transformations. Starting from CH₃ + NS, a possible initial atmospheric reaction, HCN formation appears to be the most favoured process through a cascade involvement of 1, 2 and 3. The standard heats of formation, ΔH ⁰ _f,298 are calculated to be: 3, 149kJmol^?1; and 1, 218kJmol^?1; using the CCSD(T)/6-311+ +G(3df,2p) method, with an error of ±10kJ mol^?1.