���³��ܸ����������຤kα��Ư�Ƶ����

采用离子球自洽玻尔兹曼方程和泊松方程,得到了类氦Cr离子kα线系的两条电偶极辐射光谱能量随不同等离子体环境的变化关系.分析了光谱能量漂移量和kα线交换能随等离子体环境变化的关系,给出了光谱能量漂移量随等离子体环境参数变化的公式.结果表明,光谱能量漂移量随等离子体电子密度变化呈现出很好的线性.关系.     

Ti类氦Kα线在高温稠密等离子体中的漂移

采用离子球模型,通过自洽求解Dirac方程和Poisson方程,得到类氦Ti离子Kα线系的两条电偶极辐射光谱能量随不同等离子体环境的变化关系.同时分析了束缚电子交换能随等离子体环境的变化规律.结果表明：光谱能量漂移量随等离子体电子密度变化呈现出很好的线性关系.对此,拟合得到Ti类氦Kα线光谱能量漂移量随等离子体环境参数变化的公式,对探索高温高密度等离子体诊断方法具有一定意义. 关键词： 类氦离子 自洽场离子球模型 光谱漂移 等离子体诊断     

Relativistic corrections to Coulomb energy calculations

Coulomb energies of nuclei have been calculated using a recently introduced relativistic nuclear shell model¹). The results are very close to those of the usual non-relativistic, isotropic harmonic oscillator shell model, showing the most deviation for heavy elements such as lead.     

类氦氪离子双电子复合的相对论计算

本文采用相对论性的Flexible Atomic Code (FAC)程序计算类氦氪离子的双电子复合截面及速率系数。其中自电离速率的计算采用相对论扭曲波近似，并考虑了组态相互作用的影响。文中还将所得的自电离和总辐射速率与采用MCDF和HULLAC计算得到的结果作了比较。我们检验了n-3标度律的有效性并用它对速率系数做了外推。文中还讨论了辐射分支比随不同共振峰和原子序数的变化以及级联辐射的影响。     

41≤z≤48类氟离子精细结构能级和跃迁波长的相对论多组态狄拉克-福克的计算

本文用相对论多组态狄拉克-福克(Draic-Fock)广义平均能级(MCDF-EAL)模型计算可能成为激光工作物质的类氟NbXXXIII、MoXXXIV、TcXXXV、RuXXXVI、RhXXXVII、PdXXXVIII、AgXXXIX和CdXXXX的2s~22p~5、2s2p~6、2s~22p~43s、2s~22p~43p组态的各30个精细结构能级和若干3s—3p组态跃迁波长。除最低两级外的所有计算值都是本文首次作出的理论预言。     

Fokker-Planck analysis of energy deposition of laser-produced relativistic electrons in dense plasmas

Evaluation of the energy deposition region of a laser-produced relativistic electron beam in dense core plasma is essential in the fast ignition approach to ICF. Recently, we have developed a two-dimensional relativistic Fokker-Planck code “RFP-2D” for fast electron transport in dense plasmas to investigate the energy deposition profiles. In this paper, we compare the sizes of the energy deposition region derived from RFP-2D and another RFP-type calculation model with stochastic treatments. It is found to be considerably important to take into account the influence of the self-generated electromagnetic field when evaluating the energy deposition region.     

类氮VXVII CrXVIII MnXIX和FeXX精细结构能级和跃迁波长的相对论多组态Dirac-Fock计算

本文用相对论多组态Dirae—Fock广义平均模型(MCDF-EAL)计算了可能成为激光工作物质的类氮VXVII、CrXVIII、MnXIX和FeXX的2s~22p~3、2s2p~4、2p~5、2s~22p~23s、2~2s2p~23p组态的各44个精细结构能级和33个3s—3p组态跃迁波长。其中关于VXVII、CrXVIII、MnXIX离子3s、3P组态的计算值是本文首次预言的。     

Relativistic thermal equilibrium of non-neutral plasmas

Finite temperature effects on the relativistic radial equilibrium of a non-neutral plasma are analyzed. An equation for an effective potential governing the self-consistent radial density profile is derived in the case of global thermal equilibrium. The effect of a finite temperature turns out to be particularly strong for the fast mode of rigid plasma rotation, where the density profile can extend beyond the cold limiting radius.     

Hydrogen Balmer-alpha broadening in dense plasmas

This work presents a theoretical analysis of experimental results for the hydrogen Balmer-alpha line in dense plasmas, with electron densities between 2x10(18) and 9x10(18) e/cm(3) A simulation of both electrons and ions is employed to produce reliable theoretical widths. These results are essentially in agreement with standard theory results and, for the most part, disagree with the experimental results. Consequently, either mechanisms not accounted for in the theoretical results (such as quadrupoles) are more important than previously thought at these densities, or else there is a problem in the experimental data (such as a possible reabsorption, which is not ruled out by the experimental data).     

The impact of dense plasma environments on the 1s3l fine structure levels of He-like ions

Finite-temperature dense plasma relativistic atomic structure calculations are employed to study the energy eigenvalues and transition probabilities related to the 1s3l fine structure levels of He-like ions. We discovered a particular response of the level structure that is distinctly different from simple nuclear charge screening effects that exists also for atoms and ions in vacuum as Z decreases. It is demonstrated that characteristic level crossings are driven by the free electron screening due to a particular dependence on the quantum numbers of each level of the 1s3l-configuration. Levels with large l shift stronger to the continuum than levels with small l whereas spin dependent dense plasma effects are relatively small. As a result, the known energy level fine structure in vacuum is subject to characteristic changes (level crossings, level order). Numerical calculations performed for a wide range of density, temperature and different chemical elements indicate that induced level crossings and change in level order are general characteristics of dense plasma effects.     

Statistical description of ionization potentials in dense plasmas

The Thomas-Fermi model is used to investigate the influence of the density on the energies of ions in high-density plasmas (?10²¹?10²⁶ cm^?3). This model can be used to explain the two dominant high-density effects — continuum lowering and pressure ionization — by simple energy considerations. The result shows that only the outermost electrons are affected and that the inner region of the ion is hardly influenced by the density.     

Energy eigenvalues of helium-like atoms in dense plasmas

Calculations based on a variational method with wavefunctions including the correlation of electrons are carried out to obtain the energy eigenvalues of the Schrödinger equation for helium-like atoms embedded in dense plasmas, using the Debye-Hückel approximation. Energy eigenvalues for the 1 ¹S, 2 ¹S and 2 ³S states are obtained as a function of Debye screening length.     

Picosecond x-ray laser interferometry of dense plasmas

We present the first results from picosecond interferometry of dense laser-produced plasmas using a soft x-ray laser. The picosecond duration and short wavelength of the 14.7 nm Ni-like Pd laser mitigates effects associated with motion blurring and refraction through millimeter-scale plasmas. This enables direct measurement of the electron-density profile to within 10 microm of the target surface. A series of high-quality two-dimensional (2D) density measurements provide unambiguous characterization of the time evolution in a fast-evolving plasma suitable for validation of existing 1D and 2D hydrodynamic codes.     

Effects of valence-valence,core-valence and core-core correlations on the fine-structure energy levels in Zn-like ions

We report on large ab initio calculation for the 4s²4s^2–4s4p transitions in the Zinc-like sequence, using the multi-configuration Dirac-Hartree-Fock method. Results for fine-structure energy levels, the wavelengths, transition rates and lifetimes between Z = 70 (Yb) and Z= 92 (U) are presented and compared with other theories and experiments. The calculated values including core-valence correlation are found to be similar and to compare very well with other theories and experiments values. We believe that our extensive calculated values can guide experimentalists in identifying the fine-structure levels in their future work.