燃烧法合成Ln2O2 S:RE3+(Ln=Gd,La;RE=Eu,Tb) X射线荧光粉及发光性能

采用燃烧合成法,以稀土硝酸盐和二硫代乙二酰胺为反应物,通过控制两者的摩尔比例,在点燃温度为300—350℃时,制备了掺杂不同浓度稀土激活剂离子的硫氧化物X射线荧光粉。分别以X射线衍射(XRD)、扫描电子显微镜(SEM)、光致发光(PL)光谱及X射线激发的发光(XEL)光谱对样品进行了表征。XRD分析表明,当热处理温度低于500℃时,可得到单一相的硫氧化物X射线荧光粉,这就避免了高温烧结的缺点;而当烧结温度较高时,开始有硫酸氧化物出现。从SEM图像中可以看到荧光粉粉末具有疏松和多孔连续的三维的网络块状结构,但其初级粒子尺寸较小,均小于50nm,这在一定程度上,可以提高成像系统的空间分辨率。PL光谱分析表明,所制备的荧光粉样品分别呈现出Eu^3 ,Tb^3 离子的特征发射。XEL光谱结果表明,尽管它与光致发光的激发原理不一样,但同样呈现出Eu^3 ,TB^3 离子的特征发射;这些样品本身对X射线的吸收系数及掺杂浓度不一样,因此它们的光发射效率也有所差别。     

PIV Measurements and Mechanisms of Adjacent Synthetic Jets Interactions

Interactions of adjacent synthetic jet actuators with varying relative amplitude and the relative phase of driving voltage are measured using a particle image velocimetry （PIV）. Varying relative amplitude or relative phase of driving voltage of the adjacent actuators vectors the direction of the ensuing merged jet of the adjacent synthetic jets. The vectoring mechanism of the adjacent vortex pairs, attract-impact causing deflection （AICD）, is provided to explain why the merged jet is generally vectored to the side of the phase-leading synthetic jet or the synthetic jet with higher driving voltage.     

有势力和规范对称性

介绍了有势力的一般性质,针对一般非惯性系中的惯性力引入其矢势和标势,并分析了其中的规范对称性与电磁学的形式类比.     

Effect of Strong Magnetic Field on Gamow-Teller Transition Electron Capture of Iron Group Nuclei at Crusts of Neutron Stars

The electron capture of Gamow--Teller transition on iron group nuclei is investigated in a strong magnetic. field at the crusts of neutron stars. The results show that the magnetic field has only a slight effect on the electron capture rates with the range of the magnetic fields （10^9 - 10^13 G） on surfaces of most neutron stars, whereas for some magnetars whose range of the magnetic field is 10^13 - 10^18 G, the electron capture rates of most iron group nuclei would be debased greatly and may be even decreased overrun 3 orders of magnitude by the strong magnetic field.     

Approximate wφ - Ωφ Relations in Quintessence Models

Quintessence field is a widely-studied candidate of dark energy. There is ＂tracker solution＂ in quintessence models, in which evolution of the field φ at present times is not sensitive to its initial conditions. When the energy density of dark energy is negleetable （Ωφ 〈〈 1）, evolution of the tracker solution can be well analysed from ＂tracker equation＂. In this paper, we try to study evolution of the quintessence field from ＂full tracker equation＂, which is valid for all spans of Ωφ. We get stable fixed points of we and wφ （noted as wφ and Ωφ） from the ＂full tracker equation＂, i.e., we and ωφ will always approach ωφ and Ωφ respectively. Since wφ and Ωφ are analytic functions of φ, analytic relation of φ can be obtained, which is a good approximation for the we φ relation and can be obtained for the most type of quintessence potentials. By using this approximation, we find that inequalities ωφ 〈 we and 〈ωφ are statisfied if the we （or ωφ） decreases with time. In this way, the potentiai U（φ） can be constrained directly from observations, by no need of solving the equations of motion numerically.     

Differential Representations of SO（4） Dynamical Group

In this paper we present systematic differential representations for the dynamical group SO（4）. These representations include the left and the right differential representations and the left and the right adjoint differential representations in both the group parameter space and its coset spaces. They are the generalization of the differential representations of the SO（3） rotation group in the Euler angles. These representations may find their applications in the study of the physical systems with SO（4） dynamical symmetry.     

Phenomenology of Friedberg-Lee Texture in Left-Right Symmetric Model

We consider that the Higgs triplet Yukawa coupling takes the Friedberg-Lee texture, and the Higgs doublet Yukawa coupling simply identifies with the diagonal Yutawa coupling of charged lepton in the context of left-right symmetric model. In this scenario, the phenomenology, including effective neutrino masses, mixings, and thermal flavor-dependent leptogenesis and lepton flavor violation decays are studied. We investigate the combined constrain of the parameters in this scenario and test its consistency with present data.     

Neutrino energy loss by electron capture in magnetic field at the crusts of neutron stars

Based on the p-f shell model,the effect of strong magnetic field on neutrino energy loss rates by electron capture is investigated.The calculations show that the magnetic field has only a slight effect on the neutrino energy loss rates in the range of 108-1013 G on the surfaces of most neutron stars.But for some magnetars,the range of the magnetic field is 1013-1018 G,and the neutrino energy loss rates are greatly reduced,even by more than four orders of magnitude due to the strong magnetic field.     

具有前置公用工程的换热器网络的通用解法

本文在罗行等人提出的分级超结构换热器网络的通用解的基础上,提出一种将热冷公用工程放置于换热器网络每一级的冷热流体之前的带分流的分级超结构换热器网络数学模型,并根据这种新型的模型推导出换热器网络的出口温度和每一级流股节点的温度的计算公式,从而增强了分级超结构换热器网络模型的适用性.最后用实例证明所提出的数学模型的正确性.