水热法制备SrMoO4:Eu3+红色发光材料及其发光性能

以Eu2O3、Sr(NO3)2和(NH4)6Mo7O24.4H2O为原料,采用水热法合成了Eu3+离子掺杂的Sr0.6MoO4∶Eu0.43+红色荧光粉。用X射线衍射(XRD)、场发射扫描电镜(FE-SEM)和荧光光谱(PL)等分析手段研究了荧光粉的结构和光致发光性能。结果表明,制备的荧光粉颗粒分散均匀,形状呈类四方双锥状,粒径在0.5～2μm之间,荧光粉可以被近紫外光(396nm)和蓝光(466nm)有效激发,发射出峰值位于614nm的红光,激发波长与紫外和蓝光LED芯片相匹配。因此,这种荧光粉是一种可能应用在白光LED上的红色荧光粉材料。     

Ca2SiO3Cl2∶Dy3+单一基质白光荧光粉的制备及发光特性

采用溶胶-凝胶法合成了发射白光的Ca2SiO3Cl2∶Dy3+荧光粉。利用XRD分析了荧光粉的晶体结构,其为四方晶系。在350nm近紫外光激发下,荧光粉呈白光发射,有两个主发射峰位分别于482和573nm,分别对应于Dy3+的4F9/2→6H15/2和4F9/2→6H13/2跃迁;监测573nm最强发射峰,激发光谱覆盖200～450nm,主激发峰位于350nm。研究结果表明保温时间的延长有利于发射强度的提高,伴随着Dy3+浓度的增大,发射光谱图中的两个主发射峰先增强后减弱,Dy3+的最佳浓度为2%(摩尔分数)。     

荧光粉Sr3-x-yAl2O6∶xCe3+,yEu2+的制备及其发光特性

采用高温固相反应法制备了Sr3-x-yAl2O6:xCe3+,yEu2+(x=0,y=0;x=0.04,y=0;x=0.04,y=0.02;x=0.04,y=0.04;x=0.04,y=0.06;x=0.04,y=0.08;x=0,y=0.04)荧光粉,研究其相组成与荧光特性,结果表明,样品具有单相Sr3Al2O6晶体结构。在360nm波长的紫外光激发下,Ce3+离子辐射出峰值在434nm附近的宽谱蓝光。通过能量传递作用,Eu2+离子辐射峰值为517nm左右的宽谱绿光。Ce3+和Eu2+的荧光组合获得了色坐标为(0.2611,0.3313)的近白光发射。样品的激发光谱分布在250～400nm的波长范围,这种荧光粉有望在紫外或近紫外激发的白光LED中获得应用。     

稀土多钨酸盐红色荧光粉在白光LED中的应用研究

利用高温固相法合成了Ca9Gd2W4O24:Eu3+和Sr9Gd2W4O24:Eu3+两个系列四钨酸盐体系以及Ca3La2W2O12:Eu3+二钨酸盐体系荧光粉,对比其荧光性能,结果发现此三种多钨酸盐荧光粉在395nm的近紫外和460nm的蓝光区都有较高的激发强度,与现有商业化近紫外光、蓝光LED芯片的发射光谱吻合,可以被这两种LED芯片有效激发,发射色纯度较高的红光,是潜在的紫光和蓝光转换型白光LED用红色荧光粉.Eu3+离子在Ca9Gd2W4O24和Sr9Gd2W4O24两个四钨酸盐体系中没有浓度猝灭效应,而在Ca3La2W2O12二钨酸盐体系中的最佳掺杂浓度为40%.以其中性能优良的Ca9Eu2W4O24、Sr9Eu2W4O24和Ca3La1.2Eu0.8W2O12结合400nm发射的紫光InGaN芯片以及460nm发射的蓝光InGaN芯片制备LED器件,探讨稀土多钨酸盐红色荧光粉在白光LED中实际应用存在的优点和局限性.     

白光LED用双层钙钛矿Sr_3Ti_2O_7:Eu~(3+)荧光粉的制备及其发光性能

采用高温固相法制备双层钙钛矿Sr3Ti2O7:Eu3+系荧光粉。利用X射线衍射(XRD)、扫描电子显微镜(SEM)和荧光光谱,研究了不同煅烧温度对双层钙钛矿Sr3Ti2O7:Eu3+荧光粉的晶体结构、形貌和发光性能的影响。结果表明:荧光粉在煅烧温度为1300℃时为纯双层钙钛矿Sr3Ti2O7相,且其有效激发波长为在395nm和465nm,这与当前近紫外和蓝光LED芯片的输出波长相匹配,激发产生的相应发射波长分别为618nm和626nm。该荧光粉是一种理想的白光LED用红色荧光粉。     

红色荧光粉Ca3Y2Si3O12∶Pr3+的制备及发光特性

通过高温固相方法合成了红色荧光粉Ca3Y2Si3O12∶Pr3+,研究了Pr3+掺杂浓度及助熔剂对荧光粉发光性能的影响。结果显示,所合成的荧光粉的主晶相为Ca3Y2Si3O12。通过分析荧光光谱,发现Ca3Y2Si3O12∶Pr3+硅酸盐荧光粉的有效激发范围可以在430~490nm范围内,并发射红光。在445nm激发下,样品发射光谱中的主发射峰分别位于610nm(3P0→3 H6)和644nm(3P0→3F2),其中610nm处峰值最大。通过改变Pr3+掺杂浓度,发现荧光粉发光强度先增大后减小,最佳Pr3+掺杂量x(Pr3+)为2.0%,超过最佳掺杂浓度表现为由离子间的相互作用导致的浓度淬灭。该荧光粉色温为2261℃。通过观察助熔剂的助熔效果,发现最佳的助熔剂H3BO3添加量为2.0%。     

Ca_(1.7)Mg_(0.3)SiO_4:Dy~(3+)白光LED荧光粉的合成与性能研究

采用溶胶-凝胶法制备了Ca1.7Mg0.3SiO4:Dy3+白光LED荧光粉,通过正交试验分析了不同Dy3+掺杂浓度、合成温度以及保温时间等因素对Ca1.7Mg0.3SiO4:Dy3+荧光粉性能的影响,确定Ca1.7Mg0.3SiO4:Dy3+白光LED荧光粉最佳合成工艺条件。通过对所合成荧光粉的物相、粉体颗粒形貌表征,以及激发和发射光谱测试,焙烧温度为1300℃、保温时间3.5h条件下合成得到的Ca1.7Mg0.3SiO4:0.058Dy3+荧光粉,粉体粒径为1~2μm,无杂质相,在351nm近紫外光波激发下检测到发射光谱波长在482.0nm和577.0nm处分别有较尖锐的发射峰,其色坐标处于近白光区。     

蓝光发射荧光粉Ba3P4O13∶Eu2+的发光特性及热稳定性

采用固相法在相对较低的温度(~840℃)下合成了一种可被紫外光激发的蓝光发射荧光粉α-Ba_(3-x)P_4O_(13)∶xEu~(2+),详细研究了其物相、发光特性与荧光热稳定性。在360nm紫外光的激发下,样品的发射光谱由峰位处于~439nm的不对称宽带组成。通过激发与发射光谱、荧光寿命测试及结构分析证实该不对称宽峰是由于Eu~(2+)在Ba_3P_4O_(13)中同时占据多个不同的格位所致。此外,Eu~(2+)在α-Ba_3P_4O_(13)中的最佳掺杂浓度约为x=0.06,其荧光猝灭机理为电偶极矩-电偶极矩相互作用。与商用绿色荧光粉(Ba,Sr)_2SiO_4∶Eu~(2+)相比,该荧光粉具有更好的热稳定性。α-Ba_3P_4O_(13)∶Eu~(2+)荧光粉有望在紫外激发的白光LED领域得到应用。     

白光LED用白光荧光粉Gd_2MoB_2O_9:Eu~(3+),Tb~(3+)的制备及其发光性能研究

采用高温固相法首次合成了由Eu3+和Tb3+共激活的Gd2MoB2O9白色荧光粉,并对其发光性质进行研究。该荧光粉在近紫外光(375nm)激发下发出较强的白色荧光(常温),光谱测试显示Gd2MoB2O9∶Eu3+,Tb3+的发射光谱中存在3个发射峰,分别位于486,543和613nm处,能够合成较理想的白光;激发光谱在250~400nm处均有较强的吸收,能与紫外LED很好地匹配,适用于白光LED。     

白光LED用KNaCa2（PO4）2∶Dy3+材料的制备与发光特性研究

采用高温固相法制备了KNaCa2(PO4)2∶Dy3+发光材料并对其发光特性进行了研究。光谱显示,KNaCa2(PO4)2∶Dy3+激发谱为300～500nm范围内的一系列锐谱,可被InGaN管芯和蓝光有效激发。尤其在385nm紫外光激发下,样品呈现较强白光发射,主发射峰位于485和577nm,对应Dy3+的4F9/2-6 H15/2、4F9/2-6 H13/2跃迁,形成"黄+蓝"单一基质白光。研究了Dy3+掺杂浓度对KNaCa2(PO4)2∶Dy3+发光性能的影响,随Dy3+浓度增加,发光强度先增大后减小,最佳掺杂浓度为0.04mol,Y/B值在较小范围内先增大后减小。根据Dexter理论分析其浓度猝灭机理为电偶极-电偶极相互作用。测量并标定了Dy3+不同浓度下样品的色坐标均呈现白光发射。研究表明,KNaCa2(PO4)2∶Dy3+材料是一种适合紫外-近紫外-蓝光激发的单一基质白光荧光粉。     

VLE data for CO2-CF2Cl2, N2-CO2, N2-CF2Cl2 and N2-CO2-CF2Cl

Knowledge about vapour-liquid (VLE) is required as a basis of reliable calculations for separation processes. Correlations available for the prediction of T, p, x, y data are less accurate for mixtures at high pressures and mixtures containing supercritical components. The results of VLE experiments are reported and compared with data calculated with equations of state.     

Preparation of ZrO2-CeO2 and HfO2-CeO2 nanopowders

We prepared weakly agglomerated powders of ZrO₂-CeO₂ and HfO₂-CeO₂ solid solutions 5–8 nm in particle size, consisting of monoclinic and tetragonal phases. After heat treatment at 1200°C, the crystallite size was 30 and 14 nm, respectively. We also examined the effect of precipitate freeze drying on the crystallization of hafnia-based solid solutions containing up to 20 mol % CeO₂.     

Thermal diffusion in binary mixtures H2-CCl2F2 and H2-CHClF2

Thermal diffusion coefficients were measured in two gaseous mixtures, in which one component was close to the critical temperature, in the pressure range (19.6–127.4)·10⁴ N/m² and at a freon concentration of 0.25–0.8.     

Comparison of the Electronic Structures of La2CuO4, Sr2CuO2Cl2, and Sr2CuO2F2

First-principles cluster calculations are reported of the local electronic structure of the three compounds: La₂CuO₄, Sr₂CuO₂Cl₂, and Sr₂CuO₂F₂. The copper ${\text{3d}}_{x^2 - y^2 } $ and the planar oxygen 2p _σ atomic orbitals exhibit a similar degree of covalency. The out-of-plane orbitals, however, are quite different with the ${\text{3}}d_{3z^2 - r^2 } $ atomic orbital lowered significantly in energy for chlorine and fluorine apical positions.     

Radial GRIN glasses in Li2O-Na2O-Al2O3-TiO2-SiO2 systems

A series of GRIN glass rods have been developed in Li2O-Na2O-Al2O3-TiO2-SiO2 systems. Negative radial refractive index profiles were generated by exchanging Na+ for Li+ ions in these glass rods. It has been observed that TiO2 plays a vital role in increase in the profile depth and maximum change in the refractive index because of its ambivalent nature. Change in the refractive index can be further increased by increasing the concentration of exchanging cation in the base glass.     

Elastic and Electronic Properties of Superconducting CaPd 2 As 2 and SrPd 2 As 2 vs. Non-superconducting BaPd 2 As 2

The first-principles calculations were performed to predict the elastic and electronic properties of the superconducting ThCr₂Si₂-type phases CaPd₂As₂ and SrPd₂As₂ in comparison with the non-superconducting CeMg₂Si₂-type phase BaPd₂As₂. Besides, the same properties were compared for CeMg₂Si₂- and ThCr₂Si₂-type polymorphs of BaPd₂As₂. We found that all these phases are mechanically stable and belong to soft materials with low hardness. The near-Fermi region is formed by the valence states of the blocks [Pd₂As₂] with decisive contributions of Pd 4d states. The values of N(E _F) increase in the sequence: CaPd₂As₂ < SrPd₂As₂ < BaPd₂As₂, i.e. in the reverse sequence relative to the transition temperatures T _C. Thus, the change in T _C cannot be explained by the electronic factor, i.e. by the simple correlation T _C～N(E _F). Most likely the decrease in T _C in the sequence CaPd₂As₂ → SrPd₂As₂ and the absence of a superconducting transition in BaPd₂As₂ are related to the structural factors and the peculiarities of the electron–phonon coupling mechanism.     

Si_2N_2O-Al_2O_3-La_2O_3和Si_2N_2O-Al_2O_3-CaO系统的亚固相关系

本文给出了 Si_2N_2O-Al_2O_3-La_2O_3和 Si_2N_2O-Al_2O_3-CaO 系统的亚固相图。实验结果表明:在 Si_2N_2O-Al_2O_3-CaO 系统中有一个未知结构的新化合物 CaO·Si_2N_2O,在3CaO·Si_2N_2O 和3CaO·Al_2O_3两化合物之间形成连续立方固溶体。而 Si_2N_2O-Al_2O_3-La_2O_3系统中则没有发现新化合物。在两个系统的富 Si_2N_2O区,过量的 Si_2N_2O 与 La_2O_3和 CaO 分别反应形成 Si_3N_4与 La_(10)[SiO_4]_(?)N_2(H-相)(和 CaSiO_3。所研究的这两个三元系统中,分别形成了如下几个四元相容性区。在 Si_2N_2O-Al_2O_3-La_2O_3系统内有:H-Si_3N_4-La_2O_3·Si_2N_2O-La_2O_3·Al_2O_3;H-Si_3N_4-La_2O_3·Al_2O_3-La_2O_3·11 Al_2O_3;H-Si_3N_4-La_2O_3·11 Al_2O_3-Al_2O_3;H-Si_3N_4-Al_2O_3-O′s.s;H-Si_3N_4-O′s.s-Si_2N_2O在 Si_2N_2O-Al_2O_3-CaO 系统内有:Si_3N_4-CaSiO_3-CaO·Si_2N_2O-3CaO·Al_2O_3;Si_3N_3-CaSiO_3-3CaO·Al_2O_3-2CaO·Al_2O_3·SiO_(?);Si_(?)N_(?)-CaSiO_3-2CaO·Al_2O_3·SiO_2-Al_2O_3;Si_3N_4-CaSiO_3-Al_2O_(?)-O′s.s;Si_3N_4-CaSiO_3-O′s.s-Si_(?)N_(?)O