Sin-1N和Sin-2N2(n=3～8)离子团簇结构及其光电子能谱的研究

利用密度泛函理论中的B3LYP方法,在6-311G(d)基组上对Sin-1N和Sin-2N2(n=3~8)阴阳离子团簇的几何结构和光电子能谱进行了系统研究。结果得到了各团簇的最稳定结构,Sin-2N2离子团簇对称性比Sin-1N离子团簇对称性好;Sin-1N(n=3~8)离子团簇的几何结构在总原子数n≤4时为平面结构,n>4时为立体结构;Sin-2N2(n=3~8)离子团簇的几何结构在总原子数n≤6时为平面结构,n>6时为立体结构;对于Sin-1N 团簇,总原子数是偶数的团簇比总原子数为奇数的团簇稳定;对于Sin-1N-及Sin-2N2阴阳离子团簇,总原子数是奇数的团簇比总原子数为偶数的团簇稳定。     

Gam Pn和Gam P-n团簇结构及其光电子能谱的理论研究

采用密度泛函理论中B3LYP泛函方法,在6-31 G*水平上,对GamPn(m+n≤5)团簇及其阴离子的几何构型和振动光谱性质进行了研究.在相同水平下计算了GamP-n(m+n≤5)的垂直电离能和GamPn(m+n≤5)的绝热电子亲核势.结果表明:单线态稳定结构有较高的对称性,二重态的稳定结构对称性相对较低.     

Ga_nN_3(n=1～8)团簇几何结构及光电子能谱的研究

用密度泛函理论的B3LYP方法在6-31G*的水平上,对GanN3(n=1～8)团簇的结构进行优化,并对体系的成键特性、光电子能谱及稳定性进行了计算与分析,得到了GanN3(n=1～8)团簇的最稳定结构.结果表明,当n≤5时,其基态几何结构为平面结构,N-N键在这些团簇的形成过程中起着决定性的作用;当n≥6时,其基态几何结构为立体结构,Ga-N键起主导作用;在所研究的团簇中,Ga4N3、Ga7N3的基态结构最稳定;随着n值的增大,平均极化率逐渐增强;通过对光电子能谱的分析,得到Ga-N键的振动频率与六方晶系纤锌矿结构GaN的光学声子峰值相近.     

GamPn和GamP-n团簇结构及其光电子能谱的理论研究

采用密度泛函理论中B3LYP泛函方法，在6—31G^*水平上，对Ga_mP_n(m+n≤5)团簇及其阴离子的几何构型和振动光谱性质进行了研究. 在相同水平下计算了Ga_mP^-_n(m+n≤5)的垂直电离能和Ga_mP_n(m+n≤5)的绝热电子亲核势. 结果表明：单线态稳定结构有较高的对称性，二重态的稳定结构对称性相对较低. 关键词： mP_n和Ga_mP^-_n团簇')" href="#">Ga_mP_n和Ga_mP^-_n团簇 密度泛函理论 光电子能谱     

TiGen-(n=7~12)团簇的光电子能谱及密度泛函理论研究

利用光电子能谱及密度泛函理论计算对TiGe_n^-(n=7~12)团簇的几何结构及电子特性等进行了系统研究. 对于TiGe_n^-负离子及中性TiGe_n,在n=8时出现了钛原子半内嵌的船型结构;在n=9~11时,新增的锗原子加盖到这种船型结构上,逐步形成钛原子完全内嵌的结构. TiGe₁₂^- 团簇具有一种钛原子内嵌的变形六棱柱结构. 自然布居分析结果显示,对于n=8~12的TiGe_n^-/0 团簇,随着内嵌结构的形成,有电子从锗原子转移到钛原子,说明其电荷转移方式与结构演变密切相关.     

第一性原理对GanP-m阴离子团簇结构及其光电子能谱的研究

本文利用密度泛函理论(DFT)对GanP-(n=2-7)和GanP2-(n=1-6)阴离子团簇的几何结构、电子态及稳定性进行了研究.在B3LYP/6-31G*水平上进行了结构优化和频率分析,得到了GanP-(n=2-7)和GanP2-(n=1-6)团簇的基态结构.这些阴离子团簇的几何结构随着n的增大,在n=5时由平面结构转化为立体结构;在GanP2-(n=1-6)团簇中,P-P比Ga-P容易成键;在GanP-(n=2-7)和GanP2-(n=1-6)阴离子团簇中,Ga3P2-,Ga4P2-,Ga5P2-和Ga6P-的基态结构最稳定.     

SiN团簇光电子能谱的指认

应用含时密度泛函理论研究了SiN团簇低能激发态的性质.将计算结果与前人已有的计算结果进行了比较，此外还根据计算得到的低能激发能对SiN^-阴离子的光电子能谱进行了理论指认.研究表明，SiN^-阴离子的基态为¹Σ态，而光电子能谱上的X峰和A峰分别对应于¹Σ→²Σ和¹Σ→²Π的跃迁.研究结果还表明，用含时密度泛函的方法来处理激发态的问题是成功的. 关键词： 团簇 光电子能谱 基态 激发态     

Si6N2团簇结构与性质的密度泛函理论研究

用密度泛函理论（DFT）中的杂化密度泛函B3LYP方法，在6—31G（d）的水平上对Si6N2团簇的可能结构进行了几何结构优化和电子结构计算，得到了16个可能的异构体．Si6N2团簇的最稳定结构是有4个Si-N键和4个Si—Si键的三维结构．自然键轨道方法分析成键性质的结果表明，Si—N键中Si原子向N原子有较大的电荷转移，因此Si-N原子间有较强的电相互作用；最强的IR和Raman谱峰分别位于1359．14cm^-1和1366．29cm^-1处；并计算了Si6N2团簇的最稳定结构的极化率和超极化率．     

Bn (n=2-8)团簇结构和稳定性的密度泛函理论研究

本文采用密度泛函理论（DFT）中的B3LYP方法,在6－31G*水平上对Bn（n＝2－8）团簇的各种可能的几何构型和电子结构进行了优化和振动频率计算,得到了多个平衡构型。结果表明,Bn微团簇的稳定结构大部分为平面结构,只有极少数立体结构属于基态稳定结构。平面结构又分为链状和环状结构两种,链状结构的所有原子均处于同一平面,而且处于链状结构两端的键长稍短,原子向内部收缩。环状稳定结构都是一个n元环中心有一个配位的硼原子。通过对基态结构的平均原子结合能和能量二次差分的计算,得到n为奇数时团簇较为稳定。     

Bn (n=2-8)团簇结构和稳定性的密度泛函理论研究

本文采用密度泛函理论(DFT)中的B3LYP方法,在6-31G*水平上对Bn(n=2-8)团簇的各种可能的几何构型和电子结构进行了优化和振动频率计算,得到了多个平衡构型。结果表明,Bn微团簇的稳定结构大部分为平面结构,只有极少数立体结构属于基态稳定结构。平面结构又分为链状和环状结构两种,链状结构的所有原子均处于同一平面,而且处于链状结构两端的键长稍短,原子向内部收缩。环状稳定结构都是一个n元环中心有一个配位的硼原子,通过对基态结构的平均原子结合能和能量二次差分的计算,得到n为奇数时团簇较为稳定。     

Energy of Clusters Emitted During Ion Sputtering of a Metal

A procedure for calculating the energy spectra of clusters with numbers of atoms N 5 during ion sputtering of a metal is suggested. The results are presented in the form of simple formulas. The energy distributions of clusters in the bombardment of niobium and iron by atomic gold and xenon ions, calculated in the present work, are compared with the available experimental data.     

Atomic Structure and Cohesion Energy of Isolated SiC Clusters

Physics of the Solid State - Ab initio calculations of the atomic and electronic structure and cohesion energy of Si60C60 fullerene-like clusters have been performed. For the first time, a model of...     

Atomic Structure and Cohesion Energy of ZnSe and CdSe Clusters

Physics of the Solid State - The first-principle calculations of the atomic and electronic structures of fullerene-like ZnnSen and CdnSen have been carried out for n = 12, 36, 48, and 60. A model...     

Ab Initio Investigation of the Microspecies and Energy in Hydrated Strontium Ion Clusters

Quantum chemistry calculations were used to study the structure and energy of strontium (Sr) ion hydrated clusters [Sr(H₂O)_1?25]²⁺. The saturated hydration number of the first hydration layer of Sr²⁺ was 8, and the hydration distance was 2.58 Å. The second hydration layer had 1–9 hydration numbers, and the hydration distance was in the range of 4.4–4.6 Å. This work also developed the relationship between the thermodynamic data (average water binding energy E_n and successive water binding energy ΔE_n,n?1, etc.) of the aforementioned low-energy structure and the hydration structures. The first hydration layer was formed by the strong electrostatic interaction between Sr²⁺ and water molecules, and the decrease in ΔE_n,n?1 was relatively large. Hydrogen bonds were formed between water molecules of the second hydration layer and water molecules of the inner layer, and the decrease in ΔE_n,n?1 was relatively small. When one water molecule was added beyond the second hydration layer, ΔE_n,n?1 was close to the hydrogen bond energy 8.88 kcal/mol (37.1 kJ/mol) of dimer water molecule, indicating that there was very weak interaction between Sr²⁺ and the water molecules beyond the second hydration layer.     

Modified Heisenbeg Model and the Structure of Its Energy Spectrum

In this paper, we show the interesting structure of energy spectrum for a modified Heisenberg XX model, explicit examples for low dimensions N=2,3,…,6 are also provided.     

Energy Spectrum of La3Lu2Ga3O12：Cr^3＋ and Its Pressure-Induced R-Line-Shift Reversal

By means of both the theory for pressure-induced Shifts （PS） of energy spectra and the theory for shifts of energy spectra due to electron-phonon interaction （EPI）, the normal-pressure energy spectra of α and β centers of Cr^3＋ ions for LLGG：Cr^3＋ and the PS＇s of R1 lines and U band of these centers have been calculated at 10 K, respectively. The total calculated results are in very good agreement with the experimental data. For LLGG：Cr^3＋, the pressureinduced low-high crystal-field transition and the reversal of R1-line PS take place. The pressure-dependent variation of Rmix^ei （2E - 4T2） [mixing-degree of （t2^2 （^3T1）e^4T2） and （t2^3 E） base-wavefunctions in the wavefunction of R1 state without EPI] plays a key role for the reversal of R1-line PS. The behavior of the pure electronic PS of R1 line is quite different from that of the PS of R1 line due to EPI. It is the combined effect of them that gives rise to the total PS of R1 line. The comparison between R1-line PS＇s of GSGG：Cr^3＋ and LLGG：Cr^3＋ has been made. It is found that a peak of R1-line PS appears at Rmix^ei （^2E - ^4T2） ≈ 0.08.     

Energy Spectrum of La3Lu2Ga3O12:Cr3+ and Its Pressure-Induced R-Line-Shift Reversal

By means of both the theory for pressure-induced shifts (PS) of energy spectra and the theory for shifts of energy spectra due to electron-phonon interaction (EPI), the normal-pressure energy spectra of α andβ centers of Cr3 ions for LLGG:Cr3 and the PS‘s of R1 lines and U band of these centers have been calculated at 10 K, respectively.The total calculated results are in very good agreement with the experimental data. For LLGG:Cr3 , the pressureinduced low-high crystal-field transition and the reversal of R1-line PS take place. The pressure-dependent variation of Relmix (2E- 4T2) [mixing-degree of |t22(3T1)e4T2) and |t322E) base-wavefunctions in the wavefunction of R1 state without EPI] plays a key role for the reversal of R1-line PS. The behavior of the pure electronic PS of R1 line is quite different from that of the PS of R1 line due to EPI. It is the combined effect of them that gives rise to the total PS of R1 line.The comparison between R1-line PS‘s of GSGG:Cr3 and LLGG:Cr3 has been made. It is found that a peak of R1-line PS appears at Relmix (2E - 4T2) ≈ 0.08.     

Energy Spectrum of a Positronium Negative Ion in a Parabolic Quantum Well

The method of few-body physics is applied to calculating the energy levels of low-lying states ofa positro-nium negative ion in a parabolic quantum well. The results show that the energy levels of a positronium negativeion intwo-dimensional case are lower than those in three-dimensional case.     

Photoelectron spectra of Ga20, In20 and Tl20

The HeI photoelectron spectra of Ga₂O, In₂O, and Tl₂O, as well as atomic In, have been obtained. Some spectral features of the recently published photoelectron spectrum of Al₂O differ noticeably from the heavier suboxides. The assignment of spectral features is supported by fully relativistic DVM SSC X_α calculations, which have been extended to include Al₂O. Best agreement is obtained between calculation and experiment for linear Al₂O, but for bent heavier metal suboxides. In general, the spectral features are indicative of ionic bonding, analogous to the behavior of group IIIB monohalides. Along the sequence Al₂O:Ga₂O:In₂O:Tl₂O, the highest occupied orbital becomes less and less localized on the metal atoms, with a rather dramatic decrease in metal character occurring at Tl₂O. The latter effect is attributable to a change in relative energies of the charge-adjusted metal and oxygen atomic orbitais and relativistic effects., A decrease in the relative ionization cross-section for molecular orbitais which have a large metal ns contribution is correlated with a similar behavior of the relative (ns)⁻¹cross-section for the corresponding atoms.