不可分辨跃迁阵模型下类镍金离子M带谱的理论计算

 用不可分辨跃迁阵模型(UTA model)计算类镍金(Au ⁵¹⁺)谱中8个跃迁阵的特征参数: 平均波数(kav)、半宽度(FWHM)、总强度(W)和谱线数(L)。利用高斯分布线型,根据各个阵的总强度进行叠加,得到了在总体上与实验相一致的结果,使得在实验中对金M带谱进行时间或空间的高分辨率测量成为可能。     

非预解形式线性微分方程的解

通过几个实例给出解非预解形式线性微分方程的一般方法,并讨论了预解形式的线性微分方程与非预解形式的线性微分方程解集的差别.     

稠油中饱和烃复杂混合物成分解析及其意义

利用两根极性不同的毛细柱,在全二维气相色谱上分析辽河油田遭受严重生物降解形成的稠油饱和烃组分,可以将传统色谱分析时形成的“基线鼓包”即不可分辨的复杂混合物（Unresolved Complex Mixtures）分开．根据饱和烃全二维气相色谱谱图的族分离特点和瓦片效应,结合飞行时间质谱提供的质谱信息初步解析不可分辨的复杂混合物主要成分．发现常规色谱分析时形成的所谓“基线鼓包”是由成千上万、含量相对较低的不同取代基的环状化合物组成,这些化合物在一维色谱上以分子量递增的顺序排列,在二维色谱上以极性的差异或者环的多少排列．C24之前的第一组不可分辨的复杂混合物主要由环己烷为基本单元的单环、双环和三环烷烃类化合物组成,信噪比在100以上的化合物数量约为饱和烃总数量的75％,质量分数是饱和烃总量的80％以上,是饱和烃的主要组成部分．C24之后出现的第二组不可分辨的复杂混合物主要由四个环或者五个环为基本单元的化合物组成,信噪比在100以上的化合物数量约为饱和烃总数量的17％,质量分数是饱和烃总量的0．5％．对稠油中这些不可分辨的复杂混合物的解析有助于对其成因机理的认识和高效开采方案的制定．     

Stochastic modeling of unresolved scales in complex systems

Model uncertainties or simulation uncertainties occur in mathematical modeling of multiscale complex systems, since some mechanisms or scales are not represented (i.e., ‘unresolved’) due to a lack in our understanding of these mechanisms or limitations in computational power. The impact of these unresolved scales on the resolved scales needs to be parameterized or taken into account. A stochastic scheme is devised to take the effects of unresolved scales into account, in the context of solving nonlinear partial differential equations. An example is presented to demonstrate this strategy. Dedicated to Professor Peter E. Kloeden on the occasion of his 60th birthday     

Suppression of Stokes heating processes and improved optomechanical cooling with frequency modulation

Ground-state cooling of mesoscopic mechanical objects is still a major challenge in the unresolved-sideband regime. We present a frequency modulation (FM) scheme to achieve cooling of the mechanical resonator to its ground-state in a double-cavity optomechanical system containing a mechanical resonator. The mean phonon number is determined by numerically solving a set of differential equations derived from the quantum master equations. Due to efficient suppression of Stokes heating processes in the presence of FM, the ground-state cooling, indicated by numerical calculations, is significantly achievable, regardless of whether in the resolved-sideband regime or the unresolved-sideband regime. Furthermore, by choosing parameters reasonably, the improvement of the quantum cooling limit is found to be capable of being positively correlated with the modulation frequency. This method provides new insight into quantum manipulation and creates more possibilities for applications of quantum devices.     

Au激光等离子体0.3~0.4nm范围X射线发射谱模拟

 应用自旋-轨道劈裂不可分辨跃迁组理论对高离化Au元素激光等离子体0.3~0.4nm范围的X射线发射谱进行了分析和解释。采用单温局域热动平衡近似,对实验谱进行理论模拟,并根据不可分辨跃迁组强度比得到等离子体电子温度。     

强组态相互作用对Sn离子谱线分布的影响

本文利用多组态Dirac-Fock(MCDF)方法,计算了Sn离子在不同离化度下（从SnVI到SnXIII）所产生的4p64dn-14f+4p64dn-15p+4p54dn+1 - 4p64dn的跃迁光谱,给出了组态平均能量随电离度的变化规律和理论预言的辐射光谱,并分析了组态相互作用对其的影响。     

Measurement of 232Th (n,γ) cross section at the CSNS Back-n facility in the unresolved resonance region from 4 keV to 100 keV

The neutron capture cross section of ²³²Th was measured at the neutron time-of-flight facility Back-n of China Spallation Neutron Source (CSNS) for the first time. The measurement was performed with 4 hydrogen-free deuterated benzene C₆D₆ liquid scintillation detectors, in the ES#2 experiment station on the beam line, at a distance of about 76 m from the neutron-production assembly. The total energy detection principle in combination with the pulse height weighting technique (PHWT) was applied to analyze the measured data. Results of the ²³²Th (n,γ) reaction cross section in the unresolved resonance region from 4 keV to 100 keV were obtained, which shows a good agreement with the existing experimental data from EXFOR, as well as with the evaluated data from the ENDF/B-VIII.0 and CENDL-3.1. In addition, the excitation function of ²³²Th (n,γ)²³³Th reaction in the unresolved resonance region was theoretically calculated by using the code TALYS-1.95. By fitting the experimental cross section and theoretical data, the average parameters in the unresolved resonance region were extracted. The datasets are openly available at http://dx.doi.org/10.11922/sciencedb.j00113.00015.     

Fe离子M壳层不可分辨跃迁系不透明度研究

在活动星系核吸收光谱中存在着一种重要的吸收特征——铁元素的M 壳层不可分辨跃迁系吸收谱, 认识这种特征对于活动星系核区的物理性质的研究具有重要的意义. 利用细致谱线模型, 对实验室中获得的吸收谱进行了理论计算和分析, 较好地重现了实验结果中主要的吸收结构, 同时计算了温度为10-50 eV的预测吸收谱,用于活动星系核光谱的研究.     

基于跃迁系不可分辨方法的辐射不透明度

描述了基于跃迁系不可分辨(UTA)辐射不透明度的计算方法,给出了锗(Ge)和铝(Al)的计算结果,并同实验测量结果作了比较。