Li2Sr0.995-xSiO4:0.005Eu2+,xLa3+荧光粉的晶体结构与发光特性

采用高温固相反应法在还原气氛下制备了Li2Sr0.995-x SiO4:0.005Eu2+,xLa3+荧光粉。利用X射线衍射仪、荧光光谱仪和紫外可见分光光度计对样品的晶体结构、激发光谱、发射光谱与荧光衰减寿命以及漫反射光谱进行测试分析。实验结果表明:所制得的样品为单一相的Li2SrSiO4晶体结构化合物。Li2Sr0.995-x SiO4:0.005Eu2+,xLa3+荧光粉的激发光谱均呈现出宽激发带,其中最强的激发峰位于408 nm左右。在此波长激发下可得到峰值位于570 nm左右的宽波段单峰发射光谱,其对应于Eu2+离子4f65d1→4f7电子跃迁。La3+掺杂Li2SrSiO4:Eu2+荧光粉基质产生了晶格缺陷[2La·Sr·V″Sr],其可以吸收光能并将能量传递给发光中心离子Eu2+,进而增强Li2Sr0.995SiO4:0.005Eu2+荧光粉的发光强度。漫反射光谱和荧光衰减寿命测试结果也证实La3+掺杂能够增加Eu2+的激发态吸收能量,延长发光中心Eu2+离子荧光衰减寿命。     

Sr1-x Znx Y2 S4:Er3+,Eu2+荧光粉的合成与发光特性的研究

采用碳酸盐前躯体高温分解法合成了Sr1-xZnxY2S4:Er3+, Sr1-xZnxY2S4:Eu2+和Sr1-xZnxY2S4:Er3+, Eu2+红色荧光粉. XRD图谱表明, Zn2+掺杂量x<0.2 mol 时, 粉末样品为CaFe2O4型正交晶体. Zn2+离子在Sr1-xZnxY2S4:Er3+, Eu2+中的固溶量(x mol)对荧光粉的发射强度影响很大. 随着Zn2+离子掺杂浓度的增加, Sr1-xZnxY2S4:Er3+, Eu2+(SZYSEE)紫外区激发峰(200～413 nm)发生红移, 并与可见光激发带(413～600 nm)形成一个连续的宽带谱, 与紫外和GaN基LED芯片辐射都有良好的匹配性. 当Zn2+掺杂量为0.1 mol时, SZYSEE的发光强度达到最大, 其发光强度比未掺Zn2+的增强10.7倍. Sr0.9Zn0.1Y1.76S4:0.24Er3+, 0.006Eu2+是一种潜在的白光LED用红色荧光粉.     

白光LED用红色荧光粉LixSr1-2xMoO4:Eux3+的制备及发光性质研究

采用高温固相法合成了白光LED用红色荧光材料LixSr1-2xMoO4:Eux3+,对样品分别进行了X射线衍射(XRD)分析、扫描电镜测试(SEM)和荧光光谱的测定.测试结果表明,LixSr1-2xMoO4:Eux3+荧光粉可以被近紫外光(uv)(394 nm)和蓝光(464 nm)有效地激发,且与没有掺杂Li+的荧光粉SrMoO4:Eu3+相比,发光强度得到了明显的增强.同时也讨论Li+和Eu3+的掺杂浓度对发光强度的影响.     

白色荧光粉NaGd（MoO4）2:Dy3+,Eu3+的水热合成及发光性能

采用谷氨酸辅助水热法合成了八面体形NaGd(MoO4)2:Dy3+,Eu3+白色荧光粉.X射线衍射结果表明,合成的样品为四方晶系的NaGd(MoO4)2纯相.扫描电子显微镜照片显示所制备的粒子为八面体形,各边长约为2μm.荧光光谱结果表明,在NaGd(MoO4)2:4%Dy3+,yEu3+(y=0,0.5%,0.6%,0.7%,0.8%,0.9%,1.0%)样品中,随着Eu3+掺入量的增加,Dy3+的发射峰逐渐减弱,而Eu3+的发射峰逐渐增强,说明Dy3+-Eu3+之间存在能量传递.通过色坐标图可知,当Eu3+掺杂量y=0.9%时,荧光粉的色坐标(0.338,0.281)与标准的白光色坐标(0.33,0.33)接近,表明NaGd(MoO4)2:4%Dy3+,0.9%Eu3+是很好的近紫外光激发下的白色荧光粉.     

NaF助熔剂对Sr2MgSi2O7:Eu2+,Zr4+荧光粉结构及发光性能影响

在还原性气氛下采用高温固相法合成了适合近紫外(λex=375 nm)激发的光致发光蓝色荧光粉Sr2MgSi2O7:Eu2+,Zr4+,研究了NaF助熔剂对Sr2MgSi2O7:Eu2+,Zr4+荧光粉晶体结构、颗粒形貌及发光性能影响。结果表明:适量的NaF助熔剂有利于样品的晶化,所获得样品的颗粒形貌更加规整,能有效降低中间粒径(D50)并控制粒径分布;只含中间颗粒(D50)样品的发光强度高于含全颗粒样品的发光强度;NaF助熔剂最佳添加含量为6%(质量分数),可使样品的发光强度提高446%;掺杂适量的Zr4+有利于样品的发光强度的提高,最后探索NaF助熔剂及掺杂Zr4+离子提高发光性能的机制。     

钨钼酸盐荧光粉基质组成及其退火过程对荧光性能的影响

采用高温固相法合成了一系列Eu3+掺杂的钨钼酸盐红色荧光粉CaxSr0.88-x(WO4)y(MoO4)1-y:0.08Eu3+。对其晶体结构和荧光性能进行了X射线衍射(XRD)、荧光光谱(PL)的表征,研究了不同Sr/Ca和WO4/MoO4比例对荧光粉光谱性能的影响,初步研究了不同退火过程对其发光性能的影响。所合成的Ca0.70Sr0.18(MoO4)0.5(WO4)0.5:0.08Eu3+荧光粉发光强度较好,可以被近紫外光(395 nm)和蓝光(465nm)有效激发,发射峰位于616 nm(Eu3+的5 D0→7 F2跃迁)。     

(Ca1-x-yLuy)MoO4∶xEu3+红色荧光粉的化学共沉淀合成与光致发光

使用NH4HCO3-NH3.H2O混合沉淀剂,采用化学共沉淀法合成(Ca1-x-yLuy)MoO4:xEu3+红色荧光粉,通过XRD、EDS、荧光光谱和CIE色度图研究该荧光粉的晶体结构、成分组成及发光性能。结果表明,实验按照理论化学计量比成功合成了(Ca1-x-yLuy)MoO4:xEu3+红色荧光粉,该荧光粉为CaMoO4白钨矿结构;(Ca1-x-yLuy)MoO4:xEu3+具有7F0→5L6(394 nm)和7F0→5D2(465 nm)的强电子吸收,且在613 nm处可发射高强度红光,其色坐标为(0.666 5,0.332 9),明显优于传统的Y2O2S:Eu3+红色荧光粉;此外,当Lu含量为30mol%时,荧光粉发光强度最佳。     

Eu~(2+),Mn~(2+)共激活碱土镁硅酸盐基红色荧光粉的发光性能

制备了以R3MgSi2O8(R=Ba,Sr,Ca)为基,Eu2+,Mn2+共激活的红色荧光粉并研究了其荧光性质。分别以Ba3MgSi2O8,Sr3MgSi2O8,Ca3MgSi2O8为基质时,由于晶体场环境不同,发光强度、发射峰产生相应变化。研究了以(Ba,Sr)3MgSi2O8为基的荧光粉中Ba,Sr相对量,及Eu2+,Mn2+浓度对发光性质的影响并探讨了Eu2+,Mn2+在基质中所处格位;结果表明,红光是由基质中处于九配位的Eu2+将能量传递给八面体六配位的Mn2+,而由Mn2+所发射的。     

电荷补偿对红色LED用荧光粉体的荧光性能改进

通过高温动态球磨固相法, 采用三种电荷补偿方式: (a) 3Ca2+/Sr2+→2Eu3+/Gd3++空穴; (b) 2Ca2+/Sr2+→2Eu3+/Gd3++M+(M+=Li+, Na+, K+中的一种或多种离子); (c) Ca2+/Sr2+→2Eu3+/Gd3++X-(X-=F-, Cl-, Br-, I-), 制备了红色发光二极管(LED)荧光粉体Ca0.54Sr0.16-δEu0.08Gd0.12(MoO4)0.2(WO4)0.8(δ=0-0.16). 研究表明, 方法(b)是一种较优的电荷补偿方式. 利用此荧光粉和390-405 nm发射LED芯制备了红色LED, 当正向驱动电流为20 mA时, 色坐标为x=0.66, y=0.33; 色纯度100%; 光强达6200 cd·m2; 发光效率约为95 lm·W-1. 器件的色坐标和显色指数等参数随正向驱动电流的变化起伏很小, 颜色稳定. 该红光荧光粉在新一代白色LED照明领域具有广阔应用前景.     

Dy3+,Eu3+双掺单基质Ca9Y(PO4)7白色荧光粉的合成与发光性能

以具有多种格位的Ca9Y(PO4)7作为基质, 以Dy3+和Eu3+作为共激活剂, 利用高温固相法合成了一种单基质白光荧光粉. X射线衍射证实样品属于三方晶系菱面体结构, Dy3+和Eu3+在Ca9Y(PO4)7晶体中占据了Y3+ 的格位. 样品在365 nm紫外线激发下, 荧光光谱同时出现了Dy3+和Eu3+的特征发射, 且发光强度以及色度坐标随着Dy3+和Eu3+掺杂比率的变化而有规律变化, 所有样品的发射均处于白光区域. 利用近紫外芯片作为激发源, 单一基质白色荧光粉Ca9Y1-x-y(PO4)7: xDy3+, yEu3+可应用于白光发光二极管等领域.     

Liquid-liquid equilibria of (cyclohexane + acetonitrile + methylcyclohexane + toluene) and of {(acetonitrile + methylcyclohexane) + benzene or + toluene or + cyclohexane or + chlorobenzene} at 298.15 K

Tie-line results at 298.15 K and atmospheric pressure are reported for (cyclohexane + acetonitrile + methylcyclohexane + toluene) and for {(acetonitrile + methylcyclohexane) + benzene or + toluene or + cyclohexane or + chlorobenzene). The extended UNIQUAC and UNIQUAC equations are used to correlate binary vapour-liquid equilibria and mutual solubilities for 10 mixtures constituting the ternary mixtures and to predict the ternary and quaternary liquid-liquid equilibria by use of only binary parameters.     

A photoionization study of the charge transfer reactions: Xe+ + O2 → O+2 + Xe and O+2 + Xe → Xe+ + O2

Photoionization mass spectrometer techniques have been employed to study the charge transfer reactions: Xe⁺ + O₂ → O⁺₂ + Xe and O⁺₂ + Xe → Xe⁺ + O₂. The results show the reaction of Xe⁺(²P_{$\text{3}\text{2}$}) ions with O₂ molecules is much more efficient than the reaction of Xe⁺(²P_{$\text{1}\text{2}$}) ions with O₂ molecules. The charge transfer reaction of O⁺₂ ions with Xe atoms was detected for O⁺₂ ions in the a ⁴Π_u state.     

Liquid–Liquid Equilibria of Linalool + Ethanol + Water, Water + Ethanol + Limonene, and Limonene + Linalool + Water Systems

The present work was undertaken to determine liquid–liquid equilibria for ternary systems involved in the citrus essential oil terpeneless using dilute alcohol. Tie-line data have been determined for the linalool + ethanol + water, water + ethanol + limonene, and limonene + linalool + water ternary systems at 298.15 K. The experimental data were satisfactorily correlated using the UNIQUAC and NRTL equations, and the obtained binary interaction parameters are reported. The UNIFAC group-contribution method did not allow adequate predictions of liquid–liquid equilibria involved in this study.     

Kinetics of the reactions Br + NO2 + M and I + NO2+ M

The reactions Br + NO₂ + M → BrNO₂ + M (1) and I + NO₂ + M → INO₂ + M (2) have been studied at low pressure (0.6-2.2 torr) at room temperature and with helium as the third body by the discharge-flow technique with EPR and mass spectrometric analysis of the species. The following third order rate constants were found k₁₍₀₎ = (3.7 ± 0.7) × 10^?31 and k₂₍₀₎ = (0.95 ± 0.35) × 10^?31 (units are cm⁶ molecule^?2 s^?1). The secondary reactions X + XNO₂ → X₂ + NO₂ (X = Br, I) have been studied by mass spectrometry and their rate constants have been estimated from product analysis and computer modeling.     

Ni+Pd+Ga and Ni+Pd+in liquid alloys: Enthalpies of formation

In order to fill the evident gap in the thermodynamic data of nickel-palladium-gallium and nickel-palladium-indium ternary alloys, the enthalpies of formation of these systems in the liquid state have been determined. This was achieved by means of a very high temperature calorimeter (T<1800 K), using the direct drop method, and based on analogous measurements of the respective binary alloys previously published. Complete automation of the calorimeter led to a good precision even at the highest temperatures. The enthalpies of formation of the ternary liquid alloys were measured between 1400 and 1600 K on the whole composition range. As in the limiting binary systems, enthalpies of formation are negative and non temperature dependent at any composition.

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Zusammenfassung Um die Lücke hinsichtlich thermodynamischer Daten von Nickel-Palladium-Gallium und Nickel-Palladium-Indium Legierungen zu füllen, wurden die Bildungsenthalpien dieser ternÄren Systeme im flüssigen Zustand bestimmt. Dies erfolgte mittels eines Kalorimeters für sehr hohe Temperaturen (T<1800 K), unter Verwendung der direkten Einwurfmethode auf der Basis früher veröffentlichter Messungen an den entsprechenden binÄren Systemen. Die Bildungsenthalpien der flüssigen ternÄren Legierungen wurden zwischen 1400 und 1600 K über den gesamten Zusammensetzungsbereich bestimmt. VollstÄndige Automation des Kalorimeters bewirkte hohe PrÄzision selbst bei den höchsten Temperaturen. Wie in den begrenzenden binÄren Systemen sind die Bildungsenthalpien negativ und bei allen Zusammensetzungen nicht temperaturabhÄngig.

     

Preparation, characterization and ESR studies of bulk and nano sized pyrochlore La2-xGdxZr2O7 (x=0.025, 0.05, 0.075 and 0.1)

Bulk and nano sized pyrochlore of composition La(2-x)Gd(x)Zr(2)O(7) (x=0.025, 0.05, 0.075 and 0.1) have been prepared by sol-gel method. They are characterized by powder X-ray diffraction and infrared spectroscopy. The sintering temperature influences the particle size of the sample. The room temperature powder ESR of La(1.95)Gd(0.05)Zr(2)O(7) gave characteristic "U" spectrum. The influence of particle size on the ESR of Gd(3+) is investigated. Possible reason for the disappearance of "U" spectrum with increase in the particle size is given.     

钠型斜发沸石在K^＋-Na^＋-NH4^＋和K^＋-Na^＋-Ca^2＋水溶液体系中的离子交换平衡

研究了K -Na -NH4 和K -Na -Ca2 水溶液体系与钠型斜发沸石的离子交换平衡。分别测定出以上两个体系在25℃、50℃和75℃下的离子交换平衡数据,利用平面三角图绘制表达出三元离子交换平衡等温线,并计算出沸石对体系中离子的分离因数。结果表明,在K -Na -NH4 溶液体系中,K 的分离因数在3以上,NH4 的分离因数在1~3之间,Na 的分离因数小于1,斜发沸石的离子交换选择顺序是K >NH4 >Na ,且低温有利于K 的交换,高温时NH4 的交换能力增强;在K -Na -Ca2 溶液体系中,K 的分离因数大于8,Na 的分离因数在1左右,Ca2 分离因数小于1,沸石的离子交换选择顺序是K >Na >Ca2 ,其中Ca2 属于部分交换,Ca2 对沸石对K 的交换选择性影响不大,且低温有利于沸石对K 的交换。     

Tricritical phenomena in quasi-ternary mixtures of water + n-decane + n-undecane + tert-butanol

Coexistence curves for the quasi-ternary system of water + n-decane + n-undecane + tert-butanol have been determined by measurements of the refractive index in three coexisting liquid phases. The binary mixtures of n-decane + n-undecane constructed the quasi-pure components in which the mass fraction beta of n-decane controls the approach to the tricritical point. The coexistence curves can be fitted to Scott's extended theory and can be extrapolated to a tricritical point at (44.1 +/- 0.3) degrees C and beta = 0.77 +/- 0.02 corresponding to an average n-alkane-carbon number of 10.19 +/- 0.02. The nonclassical critical amplitude ratio has been confirmed to be 4-5% smaller than the classical value, which is consistent with Fisher's prediction.     

Thermochemistry of HCOS+ and HCS2+

Heats of formation for HCOS⁺ and HCS₂⁺, obtained from high-quality ab initio calculations, have been used to determine the thermochemistry of several reactions which may form these ions in interstellar clouds or mass spectrometer experiments. Radiative association of HCO⁺ or HCS⁺ with either O or S may be important in interstellar clouds, whereas proton transfer from H₃⁺ or HCO⁺ to CS₂ or COS may be a means of synthesizing these ions by mass spectrometry. In the latter case, the relevant heats of formation are: HCS₂⁺(¹A₁) 1042 kJ mol^?1 and HCOS⁺ (¹A′) 996 kJ mol^?1.