PdⅩⅣ-CdⅩⅥ离子4s24p3和4s4p4组态精细结构能级与跃迁的扩展分析

用多组态HXR理论方法对KrⅣ-CdⅩⅥ离子4s^24p^3和4s4p^4组态的精细结构能级进行了分析计算。在已有研究工作的基础上，通过对4s^24p^3和4s4p^4组态能级的实验观测值与HXR计算结果之差AE沿等电子序列变化规律的分析．找出了△E随有效核电荷数Zc变化的规律，预言并计算了PdⅩⅣ-CdⅩⅥ离子4s^24p^3和4s4p^4组态能级，大部分预言计算值与实验结果的偏差小于100cm^-2。由此还进一步计算了PdⅩⅣ-CdⅩⅥ离子4s^24p^3—4s4p^4跃迁的谱线波长、振子强度和跃迁概率。结果表明：除了4s^24p^3D5/2-4s4p^4^2D5/2跃迁的谱线波长(29．992nm)与实验值相差0．018nm外．对于其余5条谱线．预言值与实验值的偏差均不超过0．005nm。     

A Study of S(3P2,1,0; 1D2; 1S0) Production in the 193 nm Photodissociation of CH3SH

The dynamics of S(³P_2,1,0; ¹D₂; ¹S₀) production from the 193 nm photodissociation of CH₃SH has been examined by 2+1 resonance-enhanced-multiphoton-ionization (REMPI) techniques. Using the rate equation scheme, we have rationalized the intensities of S(³P_2,1,0; ¹D₂; ¹S₀) observed according to the sequential two-photon dissociative pathways, (A): CH₃SH + hv (193 nm) → CH₃S + hv (193 nm) → S and (B): CH₃SH + hv (193 nm) → HS + hv (193 nm) → S, as the major mechanisms for S production. We have satisfactorily fitted the photodissociation laser power dependencies for S(³P) and S(¹D) produced from CH₃SH by invoking photodissociation cross sections and branching ratios S(³P)/S(¹D) for CH₃S and HS similar to those determined previously in the 193 nm photodissociation of CH₃SCH₃ and H₂S. This observation supports that the 193 nm photodissociation of CH₃S and HS prepared from CH₃SH yield predominantly S(^lD) and S(³P), similar to the cases for CH₃S prepared from CH₃SCH₃ and for HS prepared from H₂S, respectively. A small amount of S(¹S₀) observed from the 193 nm photodissociation of CH₃SH is attributed to pathway (B).     

Collisional–radiative studies of carbon plasmas

A detailed plasma kinetics model for carbon is presented which has been calculated using the Los Alamos suite of atomic kinetics codes. Models have been generated in the configuration-average approximation and the fine-structure approximation, which includes configuration-interaction and intermediate-coupling effects. These models have been used to generate relevant plasma quantities, ranging from the average ionization stage to detailed emission spectra. For many of the quantities examined, and for certain plasma conditions, significant differences exist between the configuration-average model and the detailed fine-structure model, indicating that such a detailed fine-structure model is necessary to accurately model atomic properties in such plasmas.     

Cr20+、Cu25+和Lr99+离子精细结构能级和辐射寿命的计算

用扩展的全相对论多组态自洽场方法,计算了类铍离子Cr20+、Cu25+和Lr99+的170个精细结构能级和辐射寿命以及其他各种跃迁参数,能级的计算值和实验值符合得很好.     

类硅离子精细结构能级和辐射寿命

用全相对论多组态自洽场方法,计算了类硅离子的1s、2s、2p-、2p 、3s、3p-、3p、3d-、3d、4s、4p-、4p、4d-、4d、4f-、4f、5s、5p-、5p、 5d-、5d、5f-、5f、5g-、5g、6s、6p-、6p轨道的912个精细结构能级和辐射寿命以及各种跃迁参数.能级的计算值和实验值符合得很好.从计算结果中发现了一些亚稳态能级.     

类锂离子里德堡态中的自旋-其它轨道相互作用

以多电子原子精细结构哈密顿的球张量形式和三价原子的非相对论性能级结构理论为基础,借助不可约张量理论,建立了计算类锂离子里德堡态中的自旋-其它轨道相互作用能的一种解析理论形式.完成了所有的角向积分和自旋求和计算,自旋-其它轨道相互作用能最终用径向积分来表示.应用所建立的理论对类锂离子(1s2np)2Pj态的自旋-其它轨道相互作用能进行了具体分析.     

类镁离子Mn XIV和Zn XIX的精细结构能级和辐射寿命

 用全相对论多组态自洽场方法，计算了类镁离子Mn XIV和Zn XIX的两百多个精细结构能级和辐射寿命以及各种跃迁参数。结果分析表明，能级的计算值和实验值符合得很好。     

类硼等电子序列磁偶极M1 1s^22s^22p^2P_(3/2)—~2P_(1/2)能级间隔和光谱跃迁

采用相对论量子力学GRASP2程序,扩展平均能级EAL模型,有限核模型,考虑Breit和QED的高阶微扰修正,系统地研究了类硼等电子序列磁偶极M11s22s22p2P3/2—2P1/2(Z=10～100)光谱跃迁的精细能级结构间隔,跃迁概率和振子强度,所得结果和最近的实验数据及理论计算值进行了比较。计算结果表明:在ICF高温高密度激光等离子体中磁偶极矩M1跃迁几率过程不容被忽视。     

60-GHz oxygen band: precise broadening and central frequencies of fine-structure lines, absolute absorption profile at atmospheric pressure, and revision of mixing coefficients

The 60-GHz band of ¹⁶O₂ was studied at room temperature and at low (up to 4 Torr) and atmospheric pressures. Precision measurement of central frequencies, self-broadening, and N₂-broadening parameters of fine-structure transitions up to N = 27 was performed by use of a spectrometer with radio-acoustic detection (RAD). The measured parameters are compared with GEISA/HITRAN databanks, MPM92, and other known data. An improved set of the oxygen fine-structure spectroscopic constants is obtained. The absorption profile was recorded in the range 45-96 GHz for laboratory air and pure oxygen at atmospheric pressure by use of a resonator spectrometer with noise level of about ± 0.05 dB/km, and used for deducing the first-order line mixing coefficients and for quantitative assessment of second-order mixing effects. A refined set of MPM parameters is derived from the new data and presented here.     

Fundamental constants and their time variation

We discuss the fundamental constants of physics within the Standard Model of particle physics. In this model there are 28 fundamental constants, e.g. the constant of gravity or the fine-structure constant. We consider possible changes of these constants on the cosmological time scale.