CIV共振谱线的电子碰撞展宽的理论计算

 使用R-矩阵方法,利用碰撞近似和密耦理论,计算了确定CIV 2s²S-2p²P⁰共振谱线的碰撞参数,并由此得到了在电子密度为10¹⁷cm^-3 的条件下,共振谱线的线宽和线移随温度的变化关系。计算得到的线宽与半经典的理论计算值符合得比较好,但大约只有实验线宽的一半。     

Ar+17和 Ar+16谱线的电子碰撞展宽

利用修改后伦敦理工大学的UCL扭曲波程序, 本文计算了自由电子与原子或离子的碰撞反应矩阵, 以此得到它的散射矩阵和碰撞强度.利用碰撞强度, 研究电子碰撞对辐射谱线影响.具体地, 以Ar⁺¹⁷和Ar⁺¹⁶的α线和β线为例, 计算了不同电子温度和密度下谱线的展宽和位移.     

高Z等离子体中的双电子复合与电子碰撞激发

 采用准相对论性Hartree-Fock-Relativistic方法与不可分辨跃迁组模型相结合，对Au和Ta元素的类Ni离子的双电子复合速率，以及Au元素类Cu离子的电子碰撞激发速率进行了计算。计算结果表明，对于Au类Ni离子的3d¹⁰-3d⁹4l5f-3d¹⁰4l双电子复合过程以及类Cu离子的3d¹⁰4l-3d⁹4l5f电子碰撞激发过程，当电子温度高于1.0 keV时，电子离子碰撞激发速率随电子温度增加而增加，双电子复合速率随电子温度增加而减小，并且电子碰撞激发对谱线辐射的贡献要比双电子复合大得多。     

双光子共振非简并四波混频测量钡原子里德伯态碰撞展宽中的伴线研究

研究了采用双光子共振非简并四波混频技术测量原子里德伯态碰撞展宽时出现的伴线现象, 测量了不同缓冲气压下的钡原子里德伯态6snd ¹D₂ (n=16, 22, 36) 的四波混频谱线, 研究了伴线随主量子数n 的变化曲线以及伴线信号强度随缓冲气压压强的变化曲线, 分析了伴线对NFWM谱线的线宽的影响, 发现考虑伴线对四波混频谱线线宽的贡献, 可以对NFWM模型下测量到的碰撞展宽系数进行修正.     

镁原子碰撞激发微分截面和Stokes参数的理论研究

基于相对论扭曲波理论方法,并利用新发展的处理极化电子碰撞激发的计算程序REIE06, 系统计算了中性镁原子基态3s^{2 1}S₀到激发态3s3p ¹P₁, 3s4p ¹P₁的电子碰撞激发微分截面和角关联(Stokes)参数,计算过程中系统地考虑了相对论效应、电子关联效应等. 部分计算结果与已有的实验和理论结果进行了比较,得到了较好的一致性.     

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4s²4p³和4s4p⁴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4s²4p³和4s4p⁴组态能级的实验观测值与HXR计算结果之差ΔE沿等电子序列变化规律的分析，找出了ΔE随有效核电荷数Zc变化的规律，预言并计算了PdXIV-CdXVI离子4s²4p³和4s4p⁴组态能级，大部分预言计算值与实验结果的偏差小于100 cm^-1。由此还进一步计算了PdXIV-CdXVI子4s²4p³－4s4p⁴跃迁的谱线波长、振子强度和跃迁概率。结果表明：除了4s²4p³ 2D5/2－4s4p⁴ 2D5/2跃迁的谱线波长（29.992 nm）与实验值相差0.018 nm外，对于其余5条谱线，预言值与实验值的偏差均不超过0.005 nm。     

1.315 μm波长附近实际大气高分辨率吸收光谱

 用窄线宽、脉冲可调谐光参量振荡器（OPO）作光源，使用光程长达1 097m的怀特池，采用单探测器分时复用的探测方法，首次在吸收池中精确测量了实际大气中1.315 μm波长附近高分辨率吸收光谱，实验验证了实际大气中水汽是该波段的主要吸收气体；得到了实际大气中吸收分子在氧碘激光波长（7 603.14cm^-11）处的吸收截面为 (1.05±0.09)×10^-24 cm²(标准大气条件下）以及在该波段主要吸收谱线的参数，包括吸收线的位置、线强度、压力加宽半宽度等。利用实测的线参数计算了在氧碘激光波长附近大气分子的吸收截面，发现吸收最小的波长分别位于7 603.31和7 603.93cm^-1，其值约为(8.9±0.8)×10^-25 cm²，比氧碘激光波长处的吸收截面约小15%。     

高离化态硫离子光谱的理论分析

 在考虑组态相互作用的基础上,利用包含相对论修正的Hartree-Fock(HFR)理论对S⁸⁺-S¹³⁺离子的谱线波长及加权振子强度等有关原子参数进行了系统计算,并与最新的实验观测和其它理论计算结果进行了比较。计算结果表明：S⁸⁺-S¹¹⁺的各个原子态在LS耦合下纯度很高,随着离化度的增大,S¹²⁺和S¹³⁺离子的部分原子态能级出现混合,组态相互作用逐渐增强。通过对实验结果的分析,识别出32条实验谱线,其中大多数谱线来自S⁸⁺-S¹³⁺离子的2s²2p^k-2s2p^k+1和2s2p^k+1-2s2p^k+2(k=0,1,2,3,4)之间的跃迁,理论计算结果与实验谱线波长之间的绝对误差大多数都在实验的有效分辨力以内。     

低能电子与类锂碳离子碰撞的共振激发

 考虑了内壳层电子激发的组态相互作用后,采用R矩阵方法计算了电子碰撞类锂碳离子的共振激发碰撞强度。对于1s²2s²s-1s²2p²p跃迁,结果介于密耦方法和Coulomb-Born交换近似结果之间,而且除了紧靠近激发阈值的 能量区域外与实验结果符合。     

Al激光等离子体电子温度的时间分辨诊断

 将门控分幅相机与平面晶体谱仪耦合，构成时间分辨光谱测量系统，对Al激光等离子体的K壳层发射谱进行测量，获得了相对入射激光延迟约1ns，积累时间约200ps的光谱信号。利用稳态碰撞-辐射平衡（CRE）近似条件下的等离子体光谱辐射动力学模型，给出了Al激光等离子体Ly-β线与He-β线强度比以及Ly-γ线与He-γ线强度比与电子温度的函数关系。在此基础上，根据实验谱线强度比，得到激光强度为2.319×10¹⁴，1.937×10¹⁴和3.946×10¹⁴ W/cm²时，等离子体冕区电子温度分别为1.190(1±27%)，1.165(1±27%)和1.525(1±27%)keV。     

激光产生的等离子体透射谱模拟

 根据细致组态方法,采用不分辨的跃迁矩阵模型(UTA) 在组态平均近似下可以容易地计算由高功率激光产生的局域热动平衡状态下的等离子体的不透明度。 采用量子亏损理论计算在激光产生的中Z和高Z元素的等离子体中的高主量子数组态的UTA参数,可节省了大量的计算时间,采用全相对论处理的方法可以快速地计算任何高Z元素等离子体的不透明度。还可以很方便地确定最重要组态以及细致地分析跃迁矩阵。     

Opacity calculations for Non-Local-Thermodynamic-Equilibrium plasmas

In this paper, we presented a method to calculate the spectral-resolved opacity for Non-Local-Thermodynamic-Equilibrium (non-LTE) plasmas. By solving the rate equations, we get the population. In the rate equations, configuration-averaged rate coefficients are used and the cross sections are calculated based on the first-perturbation theory. Using the detailed configuration accounting with the term structures treated by the unresolved transition array model, we calculated the spectral-resolved opacity of Al plasmas. The results are compared with those of other theoretical models. From the comparison, we can see that the present results fit well with other models for low-Z plasmas. For high-Z plasmas, we will give detailed discussion in the future.     

Research into pulsed power-driven recombination lasers

Time-resolved measurements of XUV emissions from recombining Ne and Al plasmas are reported. The DNA/PITHON pulsed-power generator was used to produce hot, dense aluminum and neon plasmas in a Z-pinch configuration. The Al Xl, 4f-3d and 4 d-3p lines at 154.4 and 150.4 Å were observed to be anomalously bright compared to the Al Xl, 4d-2p line. This anomaly, which might be suggestive of recombination lasing, may also be explained by opacity, whereby the optically thick 4→2 lines are reduced in apparent intensity with respect to the 4→3 lines. The Ne X 4-3 line was observed to be spatially localized on axis where emissions from the Ne X 3-2 line were sharply reduced in intensity. On axis, the anomalous brightness of the Ne X 4-3 line suggests a strong inversion     

辐射加热铝Ka吸收谱测量

 铝K_a吸收谱是诊断辐射加热等离子体温度的重要方法之一。在星光Ⅱ激光装置上，利用激光金膜相互作用产生的X光辐射加热其背侧的铝夹层样品，采用天津Ⅲ号胶片记录的PET晶体谱仪测量了不同激光和样品参数条件下的铝Ka吸收谱。实验观察到非常清晰的类氦到类氟铝离子Ka吸收谱线，采用细致组态模型开展了铝Ka吸收谱的模拟计算，模拟计算结果与实验结果符合得较好，研究结果可应用于辐射不透明度样品温度诊断。     

Validity of formulae for nuclear widths used in pion cascade codes

Cascade codes used for pionic X-ray calculations use formulae for nuclear absorption widths derived from perturbation theory using hydrogenic wavefunctions. Comparison with exact calculations shows that these formulae are very accurate for orbitals with l 2 but large errors can arise for l = 0, 1. An improved formula for s and p states is derived.     

K-shell photoionization of boron-like carbon ions： analysis of ls-2p resonances

Close-coupling calculations based on an R-matrix formalism are performed for the 1s--2p resonance photoionizations from the low-lying states of boron-like carbon ions. The resonance energies, widths and oscillator strengths of 1s-2p core excitations are determined by analysing the calculated photoionization cross sections. Our calculations are in reasonable agreement with the experimental and theoretical results presented by other authors. The present numerical values may help to analyse the astrophysical and laboratory plasmas.     

Electron impact excitation coefficients for laboratory and astrophysical plasmas

Electron impact excitation rate coefficients have been obtained for a number of transitions in highly ionized ions of interest to astrophysical and laboratory plasmas. The calculations were done using the method of distorted waves. Results are presented for various transitions in highly ionized Ne, Na, Al, Si, A, Ca, Ni and Fe.     

稠密、冷铝等离子体的辐射不透明度研究

使用细致谱项模型、联合组态相互作用方法和R 矩阵方法计算了处于局域热动平衡条件下的稠密、冷铝等离子体的辐射不透明度 .组态相互作用方法用于获得束缚 束缚吸收截面所需要的偶极跃迁振子强度 ,R矩阵方法用于获得光电离截面 .对于温度在 6— 12eV、密度为 0 .36mg/cm3 的铝等离子体 ,计算得到的吸收系数在波长为 0 .35 1,0 .5 2 7和 1.0 5 4 μm处与实验结果符合较好 ,而温度在 3— 6eV时 ,理论计算比实验结果大. The radiative opacity has been investigated by using detailed term accounting approximation for dense, cold aluminum plasmas under local thermodynamic equilibrium. The configuration interaction scheme has been used to obtain the relevant atomic parameters for bound-bound absorption, such as excitation energies and oscillator strengths. R-matrix method has been used to obtain the photoionization cross sections. For aluminum plasmas of density 0.36 mg/cm 3, temperature of 6-12 eV, the...     

Interband absorption and exciton binding energy in an inverse parabolic quantum well under the magnetic field

We have investigated the effects of the magnetic field which is applied perpendicular to the growth direction of the well on the interband absorption and on the binding energy of the excitons in an GaAs/Ga1−xAlxAs inverse parabolic quantum well (IPQW) with different widths as well as different Al concentrations at the well center. The calculations were performed within the effective mass approximation, using a variational method. We observe that IPQW structure turns into parabolic quantum well with the inversion effect of the magnetic field and the effective band gap of the system can be modified by changing Al concentration at the well center, the strength of the magnetic field and well dimensions. This case directly influences the nature of electronic and optical properties in this structure.     

Electronic structure,phase stability,and vibrational properties of Ir-based intermetallic compound IrX (X=Al,Sc, and Ga)

The phase stability and mechanical properties of B2 type IrX (X=Al, Sc and Ga) compounds are investigated. Self-consistenttotal-energy calculations in the framework of density functional theory using the Generalized Gradient Approximation (GGA) to determine the equations of state and the elastic constants of IrX (X=Al, Sc, and Ga) in the B2 phase have been performed. The calculations predicted the equilibrium lattice constants, which are about 1% greater than experiments for IrAl, 1.81% for IrGa, and 0.71% for IrSc compound. IrAl is shown to be the least compressible, and it is followed by IrGa and the IrSc compound. The phase stability of the studied compounds is checked. The brittleness and ductility properties of IrX (X=Al, Sc, and Ga) are determined by Poisson's ratio σ criterion and Pugh's criterion. IrGa compound is a ductile material; however, IrAl and IrSc show brittleness. The band structure and density of states (DOS), and phonon dispersion curves have been obtained and analyzed. The position of the Fermi level and the contribution of d electrons to the density of states near E_F is studied and discussed in detail. We also used the phonon density of states and quasiharmonic approximation to calculate and predict some thermodynamic properties such as constant-volume specific heat capacity of the B2 phase of IrX (X=Al, Sc and Ga) compounds.