S2O‾自由基光电子能谱的Franck-Condon分析

本文考虑多振动模混合和热带效应,凭借谐振子模型,推得计算两维-四振动模Franck-Condon重叠积分的解析表示,且应用于S2O‾ 自由基光电子能谱的理论研究。对于S2O( 1A′) – S2O‾( 2A″) 光脱附过程,结合分子轨道从头算和密度泛函理论,计算Franck-Condon因子,从而得到电子跃迁振动谱线的相对强度,理论上得到的光电子能谱与实验上观测到的能谱达到较好的一致;进一步在光谱模拟过程中,拟合实验能谱得到可靠的负离子自由基S2O‾电子态（ 2A″）的几何结构参数：键长R(SS) = 2.008 +/-0.005Å 和 R(SO) = 1.519+/-0.005Å.     

硝酰自由基光电子能谱的理论研究

本文采用谐振子模型,考虑Duschinsky效应,推得计算三维Franck-Condon因子的代数表示,且应用于研究硝酰自由基的光电子能谱的强度分布及振动结构。对于HNO((?)~3A″)-HNO~-((?)~2A″)光脱附过程,通过Franck-Condon因子计算,得到光电子能谱的谱线相对强度,理论上计算的光电子能谱与实验观测到的光电子能谱达到较好的一致;另外,在光谱模拟过程中,通过迭代Franck-Condon分析,拟合实验能谱得到阴离子HNO~-自由基(?)~2A″电子态的几何结构:键长R(NO)是0.1335±0.0005 nm,键角∠(HN())是106.3±0.5°.     

二氧化铬阴离子光电子能谱的理论研究

凭借密度泛函理论,采用不同基组对中性分子CrO2的基态（ 3B1）以及阴离子CrO2‾的基态（ 4B 1）进行几何优化和振动频率分析;应用量化计算得到的力常数及结构和光谱参数,基于推得的两维四模Franck-Condon重叠积分的代数表示,对CrO2 ( 3B1)－CrO2‾ ( 4B1) 的光脱附过程进行Franck-Condon分析和光谱模拟,理论上得到光电子能谱的谱线相对强度及振动结构分布,理论谱与实验测得的二氧化铬阴离子光电子能谱达到一致,并对光电子能谱的振动结构进行归属及热带分析;另外,在光谱模拟过程中通过迭代Franck-Condon分析过程,推得CrO2‾（ 4B1）与CrO2（ 3B1）平衡几何结构之差：ΔR(Cr-O)= 0.05Å,Δ(O-Cr-O)=12o.     

Franck-Condon 因子计算及甲醛光电子能谱的理论研究

本文凭借多振动模混合下任意维Franck-Condon 重叠积分封闭表示,推导出三维三振动模Franck-Condon重叠积分的解析表示式;基于厄米多项式的级数形式,得到计算三维三振动模Franck-Condon 因子的一般代数表示式。 另外,应用Franck-Condon 因子的代数表示,研究甲醛光电子能谱的强度分布及振动结构。 对于H2CO+( 2A1)← H2CO( 1A1)离子化过程, 基于ab initio力常数及几何参数,计算Franck-Condon 因子,得到光电子能谱的谱线相对强度。 结果表明理论模拟得到的光电子能谱与实验上观测到的能谱达到较好的一致;基于光谱模拟使人们能够对实验谱给予合理解释以及对谱峰进行正确归属。     

Franck-Condon因子计算及甲醛光电子能谱的理论研究

本文凭借多振动模混合下任意维Franck-Condon重叠积分封闭表示,推导出三维三振动模FranckCondon重叠积分的解析表示式;基于厄米多项式的级数形式,得到计算三维三振动模Franck-Condon因子的一般代数表示式.另外,应用Franck-Condon因子的代数表示,研究甲醛光电子能谱的强度分布及振动结构.对于H2CO+(珟Β2A1)←H2CO(珘X1A1)离子化过程,基于ab initio力常数及几何参数,计算FranckCondon因子,得到光电子能谱的谱线相对强度.结果表明理论模拟得到的光电子能谱与实验上观测到的能谱达到较好的一致;基于光谱模拟使人们能够对实验谱给予合理解释以及对谱峰进行正确归属.     

CF-2光电子能谱的Franck-Condon分析

在Born-Oppenheimer近似下,结合分子轨道从头算,采用谐振子模型和产生函数方法计算了CF2(X1A1)←CF-2(X2B1)跃迁的Franck-Condon因子.用迭代Franck-Condon分析(IFCA)方法对CF-2的光电子能谱进行了拟合,得到了基态CF-2的几何构型:r CF=0.142 9±0.000 1 nm,θFCF=101.10±0.01度.     

二氧化铬阴离子光电子能谱的理论研究

凭借密度泛函理论,采用不同基组对中性分子CrO2的基态((X)3B1)以及阴离子CrO1-的基态((X)4B1)进行几何优化和振动频率分析;应用量化计算得到的力常数及结构和光谱参数,基于推得的两维四模Franck-Condon重叠积分的代数表示,对CrO2((X)3B1)-CrO2-((X)4B1)的光脱附过程进行Franck-Condon分析和光谱模拟,理论上得到光电子能谱的谱线相对强度及振动结构分布,理论谱与实验测得的二氧化铬阴离子光电子能谱达到一致,并对光电子能谱的振动结构进行归属及热带分析;另外,在光谱模拟过程中通过迭代Franck-Condon分析过程,推得CrO2-((X)4B1)与CrO2((X)3B1)平衡几何结构之差:△R(Cr-O)=0.05A,△∠(O-Cr-O)=12°.     

磷基的几何结构与光电子能谱

基于ab initio/DFT理论,对磷基PH2分子X~2B1态和PH-2阴离子X~1A1态进行了几何结构优化和谐振频率计算.在B3LYP/6-311+G(2d,p)理论水平下,通过Franck-Condon因子计算模拟了PH-2实验的光电子能谱,计算得到的理论谱与实验谱完全一致,确认属于PH2(X~2B1)-PH-2(X~1A1)光脱附过程.另外,通过迭代Franck-Condon分析,得到优于ab initio/DFT理论计算的PH-2离子的几何结构参数R(PH)=0.1438±0.0002 nm和∠(HPH)=92.2±0.2°.     

磷基的几何结构与光电子能谱

基于ab initio/DFT理论,对磷基分子以其阴离子态进行了几何结构优化和谐振频率计算。在B3LYP/6-311+G(2d,p)理论水平下,通过Franck-Condon因子计算模拟了磷基的光电子能谱[K. M. Ervin and W. C. Lineberger, J. Chem. Phys. 122 (2005) 194303],计算得到的理论谱与实验谱完全一致。另外,通过迭代Franck-Condon分析,得到优于ab initio/DFT理论计算的离子的几何结构参数。     

DOO~-自由基光电子能谱的Franck-Condon分析（英文）

运用从头算方法优化了DOO基态~X2 A″、第一激发态~A2 A′及其负离子DOO-基态~X1 A′的几何结构,并进行了频率分析.且对~X2 A″-~X1 A′和~A2 A′-~X1 A′电子脱附过程进行了Franck-Condon分析和光谱模拟,得到的拟合光谱和实验谱吻合的非常好,通过光谱拟合确定了负离子DOO-基态和中性DOO第一激发态的几何结构.此外,还得到了DOO的电子亲和能和谱项能.     

关于"太阳在银河系中所受引力与到银心距离r的关系"的讨论

讨论了银道面内的引力场强分布和太阳在银河系中所受引力与到银心距离r的关系，指出引力场强g并不是与r的平方成反比，这是由于银河系的大小和形状不能忽略造成的．强调了万有引力定律的适用条件．     

On the calculation of the bremsstrahlung in the region of the plasma frequency

On the basis of the classical theory of radiation produced in incomplete Coulomb interaction, a formula is derived for the coefficient of the bremsstrahlung of fully ionized plasma. In the region of rectilinear approximation a comparison is made with the results of the quantum formula derived from the Born approximation. Furthermore, the influence of dispersion upon the emission coefficient is taken into account; some relations for the region of dispersion are given.     

Dependence of the Intensity of the Spectral Lines and the Composition of the Sample and the Plasma Parameters of the Unipolar Arc

The investigation was made of the dependence of the intensity of Tl, Ga, Mo, Mg, Mn, Sn, Bi, Ni, Zn, Pt and Au spectral lines and the plasma parameters (temperature T, electron concentration n_e, degree of 6 ionnization α) from concentration of lithium additive.     

On the predictability of the positions of the convergence zones in the ocean

The disagreement between the experimental and calculated positions of the first convergence zone are known from many publications. The most probable cause for such a disagreement, namely, the incorrect specification of the input data for the calculations, is considered. The lack of simultaneity between the hydrological surveys of the region and the acoustic experiments is emphasized. The experimental data obtained by the author in five ocean regions are presented. These data characterize the diurnal variability of the distance from the source to the nearest boundary of the convergence zone. The relations proposed by different researchers for calculating the sound speed from the temperature, salinity, and hydrostatic pressure are analyzed. It is shown that these relations lead to a substantial difference in the estimated depth dependence of the hydrostatic gradient of the sound speed. The position of the first convergence zone is calculated for the propagation conditions determined by vertical temperature and salinity profiles with the subsequent recalculation of these profiles into sound speed profiles by using eight different formulas known from the literature. It is shown that different formulas lead to different values of the distance to the first zone; this difference is substantially greater than that between the calculations and experiment. The necessity of improving the recalculation relations in view of the experimental data on sound propagation in natural oceanic waveguides, including the data on the actual positions of the convergence zones, is emphasized.     

Extracting the wavefunction of the LSP at the LHC

We consider associated production of squarks and gluinos with the lightest supersymmetric particle (LSP), or states nearly degenerate in mass with it. Though sub-dominant to pair production of color SU(3)-charged superpartners, these processes are directly sensitive to the wavefunction composition of the lightest neutralinos. Exploiting event-shape variables - including some introduced here for the first time - we are able to identify the composition of the LSP by selecting events involving a single high-pT jet recoiling against missing transverse energy. We illustrate the proposed technique on a set of benchmark cases and propose methods for applying these results in more realistic experimental environments.     

Set the controls for the heart of the Sun

In this paper we describe experiments conducted with high-power lasers that are attempting to replicate, for a very short time and in miniature, conditions found in the Sun. Experiments to date have reached conditions in the outer part of the Sun. To reach the Sun's centre requires compression of material to very much greater than solid density and heating to over ten million degrees. To achieve this, a new class of experiments and a new generation of high-power lasers are required.     

On the Question of the Source of the Apokamp

Technical Physics - The object of this work is the apokamp—a new type of plasma jet, which is formed from a bright offshoot emerging at the bending point of a channel of a high-voltage...