相对论赝势的从头计算法研究铀酰离子电子结构

用相对论赝势的从头算法研究了铀酰离子的几何构型和电子结构.得到了与实验数据较一致的键长、键角和IR振动频率.铀氧间以U5f与O2p相互作用为主,U6d与O2p间的键合较小;同时,U6p、U7s、U6d和Usd杂化轨道与O2s间也有强的相互作用.不同自旋多重度时对铀酰离子总能量计算结果表明,UO22+的基态为1∑g+的可能性更大.     

构型与构象对苯双自由基体系基态自旋多重度及其稳定性的影响

利用AM1-CI方法计算了构象对邻、间、对二取代苯双自由基体系基态自旋多重度及其稳定性的影响. 结果表明单 - 三重态能量差(△ES－T)和部分占据分子轨道的能量劈裂(△EPOMO)随自由基与苯环间的二面角而变化. 当二面角接近90°时, 分子具有平面或近平面构象时强的铁磁或反铁磁耦合单元, 由于具有近简并的高自旋和低自旋基态, 而变成弱的反铁磁或铁磁耦合单元. 由此提出为获得具有稳定高自旋基态的高自旋分子, 实验上应尽量避免选用强烈扭曲的邻、对苯分子构象.     

NiCO电子能级的自旋非限制X_α—SW法计算

利用自旋非限制X_α-SW法计算了不同状态的NiCO电子能级。结果表明基态是~1∑~+态而不是~3△态。和~3△态相比,~1∑~+态有较强的σ给予作用和π反馈作用。和自由CO配体比较,CO配体的5σ能级位移1π的要大。和实验一致,基态~1∑~+是反磁性的。我们还计算了基态~1∑~+的电荷密度、轨道电离能和跃迁能。     

小镍团簇Nin(n=2～6)电子结构和拓扑分析

在UBP86/TZVP水平上计算了小镍团簇(Ni<,n>,n=2～6)的稳定基态结构并用自然键轨道(NBO)和分子中的原子量子理论(QTAIM)分析了这些团簇的电子结构.计算结果表明,Ni团簇基态结构具有较高自旋多重度.QTAIM分析表明镍团簇中Ni-Ni键均为金属键.除Ni<,2>团簇中Ni-Ni键为纯粹的σ键外,其...     

多组态含时自旋非限制HartreeFock理论

基于自旋非限制HartreeFock理论,发展了自旋非限制多组态含时HartreeFock理论方法来研究激光场中的多电子相关动力学．自旋向上和自旋向下的自旋轨道分别在他们各自的子空间内传播;并通过约化密度矩阵和平均场算符相互作用．分别利用了自旋限制和非限制的多组态含时HartreeFock方法虚时和实时传播计算氦原子基态能量和电离几率．自旋非限制的计算结果与其他报道相吻合．     

ZnSe: Fe2+中的动态Jahn-Teller效应和远红外光谱的研究

推导了3d4/3d6离子基态 5D在立方晶体场、自旋-轨道耦合和动态Jahn-Teller效应作用下的哈密顿矩阵,并用对角化该哈密顿矩阵的方法研究了Fe2+在ZnSe中的远红外光谱,理论计算与实验符合得好.研究表明,在ZnSe∶ Fe2+中,比晶体场理论分析多出的分裂谱线是Fe2+与ZnSe晶格间的动态Jahn-Teller效应引起的.还预测了其它Jahn-Teller效应分裂谱.所推导的哈密顿矩阵对研究3d4/3d6离子在立方晶体中的精细光谱、电子顺磁共振谱和动态Jahn-Teller分裂都是有用的.     

C2F5I分子C-I键解离的自旋-轨道从头算研究

采用考虑相对论效应的6-311G**全电子基组与多参考微扰理论, 计算了该分子的包含自旋-轨道耦合效应的垂直激发能和基态、激发态C—I键解离势能曲线. 理论计算发现, 势能曲线33A'与11A', 21A'出现交叉, 交叉区域在C—I键长为0.241 nm附近; 基态11A'到激发态33A'(3Q0)的垂直激发能为4.658 eV, 与实验值4.662 eV非常吻合. 讨论了C2F5I分子作为碘激光介质的可行性.     

化合物Mo(CO)~n^+(n=1～6)构型和键离能的密度泛函研究

采用DFT/B3LYP方法研究了化合物Mo(CO)~n^+(n=1～6)的基态可能构型,对于各n值,基态可能构型(电子态)依次为：直线型(^6∑^+),直线型(^6∑~g^+),C~2~υ(^2A~2)或D~3~h(^6A~1),D~4~H(^4A~1~g),C~2~ν(^2B~2)或C~4~ν'(^2B~1),D~3~d(^2A~1~g)。计算结果表明,对于n≥3时,碎片离子的构型与体系自旋多重度关系敏感。进一步计算了Mo－CO键的逐级解离能,计算值与实验结果能较好吻合,并从Mo原子4d和5s轨道杂化角度来解释该键解离能随n值的非单调变化。     

化合物Mo(CO)~n^+(n=1～6)构型和键离能的密度泛函研究

采用DFT/B3LYP方法研究了化合物Mo(CO)~n^+(n=1～6)的基态可能构型,对于各n值,基态可能构型(电子态)依次为：直线型(^6∑^+),直线型(^6∑~g^+),C~2~υ(^2A~2)或D~3~h(^6A~1),D~4~H(^4A~1~g),C~2~ν(^2B~2)或C~4~ν'(^2B~1),D~3~d(^2A~1~g)。计算结果表明,对于n≥3时,碎片离子的构型与体系自旋多重度关系敏感。进一步计算了Mo－CO键的逐级解离能,计算值与实验结果能较好吻合,并从Mo原子4d和5s轨道杂化角度来解释该键解离能随n值的非单调变化。     

SiBr~4及其不同离子态的电子结构研究: 紫外光 电子能谱(PES)和理论研究

本文详细报道了SiBr~4的紫外光电子能谱(PES)及该化合物不同离子态(X^2T~2,A^2T~1,B^2E,C^2T~2等)的电子结构和性质。实验测得对应基态离子态的绝热电离能I~a(X^2T~2←X^1A~1)=10.532eV,X^2T~2离子态的振动频率为(450±30)cm^-^1。结合理论计算对紫外光电子能谱进行了指认和分析,结果表明X^2T~2,A~2T~1两个离子态存在明显的自旋-轨道耦合作用,自旋-轨道耦合导致的分裂分别为：0.27ev和0.53eV。此外,不同计算方法比较显示外层格林函数方法计算得到电离能与实验吻合很好。     

内含式化合物X@Al12P12的结构与稳定性研究

采用B3LYP／6—31G*方法,对内含式化合物X@Al12P12(X=Li^0/ ,Na^0/ ,K^0/2 ,Be^0/2 ,Mg^0/2 ,Ca^0/2 ,H和He)的不同对称性构型进行计算,讨论其最稳定构型的几何参数、布居分析、偶极矩、电离势、包含能、频率、HOMO—LUMO能隙和自旋密度．发现X@Al12P12化合物中,客体X=Na^0/ ,K^0/ ,Mg和He几乎处在笼的中心,Be和Ca^0/2 处在中心附近0．033nm的半径内,Li^0/ ,Be^2 ,Mg^2 和H很大程度上偏离笼的中心位置．大部分金属内含式化合物的C3对称性构型稳定．Li^0/ 。,Be^0/2 ,Mg^2 ,Ca^2 和H与其它离子相比更易嵌入笼内形成稳定的内含式化合物．     

Theoretical Studies on the Interactions of Cations with Diazine

1 INTRODUCTION Interaction between cations and π electron systems is a kind of common and important non-covalent inter- action[1～21]. It could be observed in many systems, such as gas ion-molecule complexes and biological macromolecular proteins. Especially, in biological macromolecular systems, this interaction is signi- ficant for revealing the structures and functions of proteins or disclosing the atomic essence of protein- ligand effect. Interaction between benzene and metal ions h…     

铝原子团簇Al5、Al5-和Al5+稳定结构的密度泛函理论研究

采用密度泛函理论的四种方法:杂化密度泛函B3LYP与B3PW91、Perdew-Wang91交换与相关泛函WP91PW91、局域自旋密度近似SVWN,研究了A15、Al5-和Al5+团簇的多种可能结构,找到了它们稳定的结构与自旋态,与已有的理论结果作了比较,并计算了Al5-的绝热与垂直电子离解能、Al5的绝热与垂直电离势,同有关的实验数据比较,符合较好.同时对四种密度泛函方法的计算结果作了一些比较与讨论.     

Spectroscopic and structural features of small thiocarbonyl molecules in low-lying excited states: Further applications of a variant of the orthogonal gradient method

Structural parameters of a set of five thiocarbonyl molecules in the lowest nπ* states are calculated by using a generalized orbital optimization algorithm (a variant of the orthogonal gradient method) in an INDO MCSCF framework. Transition energies, singlet-triplet splittings, planar inversion barriers, and dipole moments in nπ* states of different spin multiplicities are reported. Predicted structural features agree reasonably well with available experimental or theoretical data. Some interesting trends are noted in the computed inversion barrier heights, singlet-triplet splittings, and dipole moments in nπ* states.     

锥形硼烷B5H10X的结构和成键性质

采用从头算分子轨道法对锥型硼烷Ｂ５Ｈ１０Ｘ（Ｘ＝Ｂｅ＾－,Ｂ,Ｃ＾＋,ＢｅＨ,ＣＨ＾２＋,Ｂ＾２－,Ｃ＾－,Ｎ,Ｏ＾＋,ＢＨ＾－,ＣＨ,ＮＨ＾＋和ＯＨ＾２＋）进行了研究,结果表明,端氢和桥氢原子与帽基原子相对位置的变化是由帽基原子和环原子轨道的弥散程度及环的尺寸效应共同决定的,端氢原子对桥氢原子的空间位置有着制约作用。     

Relativistic corrections in the LCGTO–local-spin-density method. I. Atomic bases for transition metals

Compact orbital GTO basis sets optimized with a nonrelativistic Hamiltonian, then decontracted, are utilized in an SCF treatment with a quasi-relativistic scalar Hamiltonian including the mass–velocity and one-electron Darwin operators. Ionization and excitation energies, orbital energies, and radial mean values obtained from different expansion patterns have been tested in atomic calculations for Ag and generalized for Cu and Au atoms. The one-electron spin–orbit operator is also used in an SCF treatment. Spin–orbit coupling energies are calculated for Cu, Ag, and Au atoms.     

Energy correctors for accurate prediction of molecular energies

Energy correctors are introduced for the calculation of molecular energies of compounds containing first row atoms (Li-F) to modify ab initio molecular orbital calculations of energies to better reproduce experimental results. Four additive correctors are introduced to compensate for the differences in the treatment of molecules with different spin multiplicities and multiplicative correctors are also calculated for the electronic and zero-point vibrational energies. These correctors, individually and collectively yield striking improvements in the atomization energies for several ab initio methods. We use as training set the first row subset of molecules from the G1 basis of molecules; when the correctors are applied to other molecules not included in the training set, selected from the G3 basis, similar improvements in the atomization energies are obtained. The special case of the B3PW91/cc-pVTZ yields an average error of 1.2 kcal/mol, which is already within a chemical accuracy and comparable to the Gaussian-n theories accuracy. The very inexpensive B3PW91/6-31G** yields an average error of 2.1 kcal/mol using the correctors. Methods considered unsuitable for energetics such as HF and LSDA yield corrected energies comparable to those obtained with the best highly correlated methods.     

Communication: ROHF theory made simple

Restricted open-shell Hartree-Fock (ROHF) theory is formulated as a projected self-consistent unrestricted HF (UHF) model by mathematically constraining spin density eigenvalues. This constrained UHF (CUHF) wave function is identical to that obtained from Roothaan's effective Fock operator. The α and β CUHF Fock operators are parameter-free and have eigenvalues (orbital energies) that are physically meaningful as in UHF, except for eliminating spin contamination. This new way of solving ROHF leads to orbitals that turn out to be identical to semicanonical orbitals. The present approach removes ambiguities in ROHF orbital energies.     

Electron Spin Resonance(ESR)Spectroscopy of the Transition-metal Complexes and Clusters I.Systematic Investigations of Real-and Complex-Orbital Methods for Calculating the d-Orbital Energies of a Low-spin(S=1/2)nd~5(t_2~5,~2T_2)(n=3

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Strong spin-orbit effects in small Pt clusters: geometric structure, magnetic isomers and anisotropy

Ab initio density functional calculations including spin-orbit coupling (SOC) have been performed for Pt(n), n = 2-6 clusters. The strong SOC tends to stabilize planar structures for n = 2-5, whereas for clusters consisting of six atoms, three-dimensional structures remain preferred. SOC leads to the formation of large orbital magnetic moments and to a mixing of different spin states. Due to the spin-mixing the total magnetic moment may be larger or smaller than the spin moment in the absence of SOC. Both spin and orbital moments are found to be anisotropic. Because of the strong SOC the energy differences between coexisting magnetic isomers can be comparable to or even smaller than their magnetic anisotropy energies. In this case the lowest barrier for magnetization reversal can be determined by a magnetic isomer which is different from the ground state configuration.