X-ray absorption spectra of plasmas

In this paper we present a theoretical method to calculate the absorption spectra of hot dense plasmas. Based on our fully relativistic treatment incorporated with the quantum defect theory to handle the huge number of transition arrays from many configurations with high principal quantum number, we can calculate the absorption spectra for any element or multi-element plasmas with little computational efforts. We calculate the absorption spectra of C10H1605 plasmas, which are in good agreement with the experimental spectra. We can then provide diagnostic analysis for plasmas in relevant inertial confinement fusion (lCF) experiments; namely not only to determine plasmas' temperatures and densities, but also to provide the population densities of various ionic stages. Our theoretical method verified by "benchmark experiments" will be a basic tool to provide "precise" opacity data for the ICF research.``     

等离子体X射线吸收谱及发射谱研究

 报道计算高温高密等离子体吸收谱和发射谱（光学薄）的理论方法；该方法基于相对论原子理论，可以计算任何单元素以及多元素等离子体的谱分辨X射线吸收谱和发射谱（光学薄）；应用了量子亏损理论，可以减少计算量。利用该方法计算金等离子体LTE吸收谱，计算结果与实验符合良好。本文还对金等离子体LTE的光学薄发射谱进行了研究, 这将有利于对实验进行进一步的诊断分析。该理论计算方法还可提供等离子体内各电离度能级布居等重要物理参数。因此经“标准实验”检验的该理论计算方法将是提供ICF“精密”物理辐射参数的重要基础。     

Theoretical Analysis of Ionic Autoionization Spectra of Lanthanum in the Energy Region of 90650—915—00cm^—1

Eigenquantum defects μα and transformation matrix Uiα of La are calculated from the first principles byrelativistic multichannel theory, and dipole matrix elements Dα are obtained by fitting the experimental spectra.With these parameters, ionic autoionization spectra of lanthanum via an intermediatestate (Xe)5d6d^-1 P1 of La . in the energy region of 90650-91500 cm^-1 are calculated within the framework of multichannel auantum defecttheory. Our calculated spectra are in general agreement with the experimental data.     

Theoretic Study of C Ⅱ Recombination Line

Using the R-matrix method, we carry out theoretical calculations for recombination line λ 8794 A(3d′-3p′) of C Ⅱ, which is important to estimate the abundances of carbon in planetary nebulae. Our calculations are based on three sets of target orbital basis, through which we elucidate the electron correlation and static polarization effects in the dielectronic recombination processes.     

Sc原子高激发态理论研究

利用相对论性多通道量子亏损理论计算了Sc的原子里德堡态能级 .计算结果显示 ,由于通道间的相互作用 ,使得光谱非常复杂 ,这与实验测量结果是一致的. The energy levels of Rydberg series of Sc atom have been calculated by Relativistic Multichannel Theory (RMCT). The calculations reveal that the Rydberg spectra are complex due to the channel interactions, which is consistent with the experimental spectra.     

等离子体X射线吸收谱研究

计算高温高密等离子体吸收谱的理论方法;该方法基于相对论原子理论,可以计算任何单元素以及多元素等离子体的谱分辨X射线吸收谱;应用了量子数亏损理论,可以减少计算量. 利用该方法计算有机材料C_１０Ｈ_１６Ｏ_５等离子体的吸收谱,计算结果与实验符合良好.通过理论计算与实验相比较,可对惯性约束核聚变(ICF)等离子体进行诊断分析;不但可判断等离子体的温度和密度,还可提供等离子体内各电离度能级布居等重要物理参数. 同时经过有关“标准实验”验证的理论计算方法将是提供ICF“精密”辐射参数的重要基础.