A Novel Synthesis of Alkaline Earth Silicate Phosphor Sr3MgSi2O8： Eu^2＋, Dy^3＋

A novel method for synthesizing long afterglow silicate phosphor Sr3MgSi2O8：Eu^2＋,Dy^3＋using TEOS and inorganic powders as reactants was reported. Acetic acid as a catalyzer controlled the hydrolysis of TEOS by adjusting pH value of the system. The morphologies of precursor were characterized by transmission electron microscope （TEM）. The structure and optical properties of the phosphor powders were systematically investigated by means of X-ray diffraction and spectrofluorometry. TEM images have reflected the core-shell structure and quasi-spherical morphology of the precursor particles. It was found that the single-phase Sr3MgSi2O8 crystalline structures were obtained at 1050 and 1250 ℃ for the samples prepared with the nano-coating method and the solid state reaction, respectively. The emission intensities of the phosphors prepared by the present method were higher than those by the conventional process. Also, the afterglow characteristic was better than that prepared by solid-state reaction in the comparable condition.     

Lidar-observed temperature structures and gravity-wave perturbations of the mesopause region in the springs of 1990–1992 over Fort Collins,CO

The Na temperature lidar data taken during the nine nights in springs 1990 and 1991 at Fort Collins, CO, have been re-analyzed by a refined procedure, which takes into account the effects of (i) the more accurately determined lidar operational frequencies, (ii) the proper inclusion of extinction in the Na layer and (iii) additional temporal and spatial smoothing. Depending on altitudes, the new lidar frequencies and the effect of Na extinction combined to lower the calculated temperature values by 2–8 K. Although the occasionally noted large rapid change (in 15 min) in the centroid temperature is reduced from 40 K to 20 K due to the added smoothing first employed by Bills and Gardner, the general conclusion presented in the recently published paper [1] remains valid. In this paper, we also present the analysis of new data (a total of 17 nights) taken during spring 1992 which further substantiates the fact that the averaged mesopause in spring rises from a lower altitude before midnight to a higher altitude after midnight. In addition, parameters depicting atmospheric gravity-wave perturbations have been derived from the measured temperature profiles. Using the data collected in 26 spring nights, we have determined the averaged relative density (temperature) perturbation, Brunt Vaisala period and Richardson number to be, respectively, 5.1±1.1%, 5.1±0.3 min, and 1.8±1.0.     

Quantum anticentrifugal force for wormhole geometry

We show the existence of an anticentrifugal force in a wormhole geometry in R³. This counterintuitive force was shown to exist in a flat R² space. The role the geometry plays in the appearance of this force is discussed.     

Tunnelling Effect and Hawking Radiation from a Vaidya Black Hole

We extend Parikh＇s study to the non-stationary black hole. As an example of the non-stationary black hole, we investigate the tunnelling effect and Hawking radiation from a Vaidya black hole whose Bondi mass is identical to its mass parameter. The Hawking radiation is considered as a tunnelling process across the event horizon and we calculate the tunnelling probability. It is found that the is the function of Bondi mass re（υ）. result is different from Parikh＇s study because dr H/dυ     

Gd2ZnTiO6∶Dy3+, Eu3+单基质白光荧光粉的制备与发光性能

采用溶胶-凝胶法制备出Dy³⁺, Eu³⁺共掺杂Gd₂ZnTiO₆白光荧光粉. 通过X射线衍射(XRD)、 扫描电子显微镜(SEM)、 光致发光(PL)光谱对荧光粉的物相、 形貌及荧光性质进行了表征. 结果表明, 所制备的样品均为双钙钛矿结构, 属于单斜晶系(空间群: P2₁/n), 形貌为2~5 μm无规则形状的颗粒. 在392 nm近紫外光的激发下, Gd₂ZnTiO₆∶Dy³⁺,Eu³⁺荧光粉展现出Dy³⁺的蓝光、 黄光发射以及Eu³⁺的特征红光发射. 此外, 通过调节Dy³⁺和Eu³⁺的掺杂浓度, 可实现低色温的暖白光发射. 基于样品优异的荧光性能, 该荧光粉在近紫外激发白光LED中具有一定的开发潜力.     

Tb0.3Dy0.7Fe2合金的本构参数辨识方法研究

建立了一种简便的、适用于磁畴模型应用的Tb0.3Dy0.7Fe2合金本构参数辨识方法.针对Tb0.3Dy0.7Fe2合金磁畴模型中本构参数不明确且直接实验测试困难的问题,提出了一种数值计算与实验测试相结合的参数辨识方法.采用坐标变换与绘制自由能等势曲线相结合的方法,简化了载荷作用下Tb0.3Dy0.7Fe2合金内磁畴角度偏转的数值计算,研究了合金磁畴角度偏转模型的参数依赖性.在此基础上,结合简单的实验测试,建立了Tb0.3Dy0.7Fe2合金各向异性常数K1和K2、能量分布因子ω、晶轴取向分布的辨识及修正方法.该方法能够简单、快速地完成Tb0.3Dy0.7Fe2合金磁畴模型中本构参数的辨识,对完善磁致伸缩材料磁畴偏转的数值计算模型非常有意义.理论分析可为类磁致伸缩材料磁机耦合模型的建立、完善,以及材料本构参数的辨识、获取提供参考.     

Spin‐Hamiltonian parameters for Dy3+ ion at the trigonal 12‐fold coordinated La3+ site of La2Mg3(NO3)12·24H2O

The spin‐Hamiltonian parameters (g factors g_‖, g_⊥ and hyperfine structure constants ¹⁶¹A_‖, ¹⁶¹A_⊥, ¹⁶³A_‖, ¹⁶³A_⊥) for ¹⁶¹Dy³⁺ and ¹⁶¹Dy³⁺ isotopes in the trigonal 12‐fold coordinated La³⁺ site of La₂Mg₃(NO₃)₁₂·24H₂O crystal are calculated from a diagonalization (of energy matrix) method. In the method, the Zeeman and hyperfine interaction terms are added to the conventional Hamiltonian used in the studies of crystal‐field energy levels, and a 66×66 energy matrix concerning the ground multiplet ⁶H_15/2 and the first to fifth excited multiplets ⁶H_13/2, ⁶H_11/2, ⁶H_9/2, ⁶H_7/2 and ⁶H_5/2 are applied. The calculated results are discussed. (© 2010 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

Sub-coercive field dynamic hysteresis in morphotropic phase boundary composition of Pb(Zr1/2Ti1/2)O3-Pb(Zn1/3Nb2/3)O3 ceramic and its scaling behavior

Sub-coercive field dynamic ferroelectric hysteresis of a morphotropic phase boundary composition of the PZT-PZN ceramic was investigated under influence of the compressive stress. The scaling relation of hysteresis area 〈A〉 against frequency f, field amplitude E₀, and stress σ took a form of , which is not different significantly to that of other PZT-PZN compositions with pure tetragonal or rhombohedral structure, as well as to that of soft and hard PZT bulk ceramics. This study suggested that the domain structures, not ceramic compositions, played a key role in controlling dynamic hysteresis behavior of ferroelectric materials.     

Dy~(3+)掺杂Ge-Ga-Se-KBr硫卤玻璃近红外和中红外发光特性研究

用熔融淬冷法制备了系列掺杂浓度的Dy3+∶Ge-Ga-Se-KBr硫卤玻璃样品,测试了样品的折射率、吸收光谱、近红外及中红外荧光谱。应用Judd-Ofelt理论计算了Dy3+离子的强度参数(Ωi,i=2,4,6)、自发辐射跃迁几率(A)、荧光分支比(β)和辐射寿命(τrad)等光谱参数。研究了810 nm激光泵浦下样品中红外荧光特性与掺杂浓度之间的关系,利用McCumber(MC)和Futchbauer-Ladenburg(FL)理论分别计算了常温Dy3+:6F5/2→6H9/2(2.17μm),6F11/2(6H9/2)→6H13/2(2.47)和6H13/2→6H15/2(2.86μm)中红外荧光的受激发射截面。     

纳米SrAl2O4:Eu2+,Dy3+长余辉发光材料的制备与性能

采用水热-均匀共沉淀法制备了纳米SrAl2O4:Eu2+,Dy3+长余辉发光材料.通过XRD、TEM、荧光光谱、热释光谱对其结构和性能进行分析.XRD结果表明所制备的SrAl2O4:Eu2+Dy3+纳米发光材料为单相,属单斜晶系.TEM测试表明纳米SrAl2O4:Eu2+,Dy3+发光材料为规则的球状粒子,粒径为50～80 nm,且分散性良好.激发和发射光谱测试表明,样品的激发光谱是峰值在356 nm 的连续宽带谱,发射光谱是峰值位于512 nm的宽带谱,与SrAl2O4:Eu2+,Dy3+粗晶材料相比,激发和发射光谱都出现了"蓝移"现象.样品的热释光峰值位于358 K,适合于产生长余辉.