高光效高热稳定性蓝色荧光粉Ca2-ySrySiO4:Ce3+,Li+的组成筛选和发光机理

采用高温固相法合成了一系列Ca_(2-x-y)Sr_(y-x)SiO_4∶x Ce~(3+),x Li~+蓝色固溶体荧光粉。XRD结果表明,所合成的固溶体荧光粉均为单一物相。随着Sr~(2+)成分的增加,Ca_(2-y)Sr_y SiO_4物相从单斜晶系β-Ca_2SiO_4向正交晶系α′-Ca_2SiO_4转变,发射光谱逐渐红移。组成为Ca_(1.75)Sr_(0.25)SiO_4时,荧光粉的发射波长最长(454 nm),Stokes位移最大。基质为Ca_(1.1)Sr_(0.9)SiO_4的晶体结构可诱导掺杂离子Ce~(3+)取代SrO_(10)格位、Li~+取代CaO8格位。优化的荧光粉Ca_(1.05)Sr_(0.85)SiO_4∶0.05Ce~(3+),0.05Li~+(CS_(0.85)SO∶CeLi)在375 nm紫外光激发下,发射445 nm的蓝光,内量子效率(IQE)达到91.18%,200℃时发射强度保持室温发光强度的98.70%。根据晶体结构、晶体场分裂和掺杂离子质心位移等理论,讨论了CS_(0.85)SO∶CeLi综合发光效应最佳的内在原因。     

通过能量传递实现Ba5-2x-yTbxNax(PO4)3Cl∶yEu2+荧光粉的光谱调控

通过[Na~+,Tb~(3+)]离子对取代[Ba~(2+),Ba~(2+)]离子对,制备了一系列的Ba_(5-2x-y)Tb_(x )Na_x(PO_4)_3Cl∶y Eu~(2+)荧光粉。通过X射线粉末衍射、扫描电子显微镜、光致激发和发射光谱对其结构、形貌、组成及发光性能进行研究。结果表明:在354 nm激发下,Ba_(3.97)Tb_(0.50)Na_(0.50)(PO_4)_3Cl∶0.03Eu~(2+)样品的发射光谱既包含了Eu~(2+)位于450 nm左右的宽带特征发射,又包含了Tb~(3+)位于490、545、583和622 nm的窄峰特征发射。由于存在Eu~(2+)→Tb~(3+)的能量传递,使得Ba_(3.97)Tb_(0.50)Na_(0.50)(PO_4)_3Cl∶0.03Eu~(2+)中Tb~(3+)的发光强度相对于Ba_(4.00)Tb_(0.50)Na_(0.50)(PO_4)_3Cl中Tb~(3+)的发光强度显著提高。通过改变[Na~+,Tb~(3+)]离子对的浓度,实现了对Ba_(5-2x-y)Tb_(x )Na_x(PO_4)_3Cl∶y Eu~(2+)荧光粉的光谱调控。当x=0.50时,Ba_(4.97-2x)Tb_(x )Na_x(PO_4)_3Cl∶0.03Eu~(2+)中Tb~(3+)的发光强度达到最大。     

Ca9Y(PO4)7:Ce3+,Tb3+纳米荧光粉的制备及发光性能

采用水热法制备出Ca_9Y(PO4)7∶Ce~(3+),Tb~(3+)纳米荧光粉,通过XRD、SEM和荧光光谱等对样品进行了分析,研究在Ca_9Y(PO4)7基质中引入Ce~(3+),Tb~(3+)离子对发光性能的影响规律。研究发现因Tb~(3+)离子自身能量交叉驰豫的存在,使得单掺Tb~(3+)时,通过调节Tb~(3+)离子的浓度可以实现对发光颜色的控制。同时研究了Ce~(3+)-Tb~(3+)之间的能量传递为电多极相互作用的偶极-四极机制,Ce~(3+)-Tb~(3+)之间最大的能量传递效率为55.6%。Ca_9Y(PO4)7∶Ce~(3+),Tb~(3+)的发光颜色可以通过激活离子之间的能量传递和共发射得到可控调节。SEM分析表明荧光粉颗粒尺寸在100 nm左右,分散性好。     

Eu3+掺杂B2O3-CaO发光材料的制备及其发光性能

采用溶胶凝胶法制得高纯的B_2O_3-CaO∶Eu~(3+)荧光粉。用XRD、IR对不同退火温度下所得样品的结构进行表征,结果发现随退火温度的变化,能形成不同结构的硼酸盐基质。通过对以不同结构硼酸盐为基质荧光粉的激发、发射谱图及荧光衰减曲线的分析,探讨了材料的发光性能和发光机理。结果表明,在不同结构硼酸盐基质中,Eu~(3+)都处于无反演对称中心格位,以(5D0→7F2)电偶极跃迁为主,所以材料主要发红光;且900℃退火所得高纯相的CaB2O4基质最有利于发光、对应的荧光衰减时间最长,这都因在此荧光粉中Eu~(3+)更易取代Ca~(2+),并形成相对较多的p-n结和陷阱所致。     

WO3/YF3:Eu3+复合纳米材料的制备与发光性能

采用直接沉淀法制备了WO_3/YF_3∶Eu~(3+)复合纳米材料,并对其结构、组成、形貌和发光性能进行了研究。XRD分析表明:复合纳米材料由纳米粒子WO3和结晶良好的正交晶系的YF3∶Eu~(3+)组成。SEM照片表明:片状WO3颗粒表面沉积了分散性较好、粒径均匀(尺寸为10~50 nm)的YF3∶Eu3纳米颗粒。荧光光谱分析表明:该复合纳米材料具有良好的发光性,以593 nm附近的5D0→7F1磁偶极跃迁为最强发射峰,与纯的YF3∶Eu~(3+)相比WO_3/YF_3∶Eu~(3+)发光强度明显增强,表明具有表面等离子共振效应的WO3纳米粒子对壳层的YF3∶Eu~(3+)起到发光增强作用。     

La_7O_6(BO_3)(PO_4)_2∶Eu~(3+)/Tb~(3+)荧光材料的制备及其光致发光性能

采用优化的高温固相方法制备了稀土离子Eu~(3+)和Tb~(3+)掺杂的La_7O_6(BO_3)(PO_4)_2系荧光材料,并对其物相行为、晶体结构、光致发光性能和热稳定性进行了详细研究。结果表明,La_7O_6(BO_3)(PO_4)_2∶Eu~(3+)材料在紫外光激发下能够发射出红光,发射光谱中最强发射峰位于616 nm处,为5D0→7F2特征能级跃迁,Eu~(3+)的最优掺杂浓度为0.08,对应的CIE坐标为(0.610 2,0.382 3);La_7O_6(BO_3)(PO_4)_2∶Tb~(3+)材料在紫外光激发下能够发射出绿光,发射光谱中最强发射峰位于544 nm处,对应Tb~(3+)的5D4→7F5能级跃迁,Tb~(3+)离子的最优掺杂浓度为0.15,对应的CIE坐标为(0.317 7,0.535 2)。此外,对2种材料的变温光谱分析发现Eu~(3+)和Tb~(3+)掺杂的La_7O_6(BO_3)(PO_4)_2荧光材料均具有良好的热稳定性。     

形貌可控的NaCaGd(WO4)3:Eu3+红色荧光粉的制备及发光性能

采用水热法成功合成了形貌可控的NaCaGd_(1-x)(WO_4)_3∶x Eu~(3+)红色荧光粉。系统地研究了初始溶液pH值、反应温度和Eu3+掺杂浓度对NaCaGd_(1-x)(WO_4)_3∶x Eu~(3+)荧光粉物相结构、微观形貌和发光性能的影响。结果表明,当pH值为9、反应温度为180℃时,可合成单相四方晶系的NaCaGd(WO_4)_3,且颗粒微观形貌呈现分散性好、尺寸较均一的四方盘状纳米晶。在394 nm激发下,荧光粉显现典型的红光发射,其对应于Eu~(3+)的特征4f-4f跃迁。荧光粉发射光谱的强度随着pH值、反应温度及Eu~(3+)掺杂浓度的变化而变化。当pH=9、反应温度为180℃时,NaCaGd_(1-x)(WO_4)_3∶x Eu~(3+)(x=1)获得最佳发光强度。此外,研究了NaCaEu(WO_4)_3荧光粉的热稳定性,结果显示随着温度的升高,荧光粉发光强度逐渐降低。最后,通过理论计算得到荧光粉的色坐标和色纯度分别为(0.658,0.341)和96.1%,接近标准红色CIE坐标(0.673,0.327)。     

Cr3+在不同基质Y3Ga5O12或Ga2O3中的荧光特性

以Ga_2O_3、Y_2O_3、Cr(NO_3)_3·9H_2O为原料,柠檬酸为配位剂,通过溶胶-凝胶高温固相合成法制备出Ga_(2-2x)O_3∶2xCr~(3+)(Ga_2O_3∶xCr)与Y_3Ga_(5-5x)O_(12)∶5xCr~(3+)(YGG∶xCr)2种多晶粉体(x=0.01,0.03,0.05,0.07)。并采用X射线衍射(XRD)、红外光谱(IR)、扫描电镜(SEM)、荧光光谱(PL)对样品的结构、组成、形貌和荧光性能进行测试分析。XRD和IR分析结果显示在900℃煅烧后Ga_2O_3∶xCr和YGG∶xCr两种样品均成相。SEM照片显示Ga_2O_3∶xCr样品形貌为柱形多面体,YGG∶xCr为短棒状。PL结果显示Cr~(3+)在Ga_2O_3和YGG两种基质中的最强荧光发射峰分别位于742和740 nm,均属于Cr~(3+)的~2E-~4A_2跃迁,对比发现Cr~(3+)在YGG基质中的荧光发射强度更强,在远红光区的荧光性能更好,能满足温室照明中植物光合作用的需求。     

Dy3+，Eu3+共掺的LiGd(MoO4)2单一相荧光粉的合成、发光及能量传递

采用溶胶-凝胶法制备了LiGd(MoO_4)_2∶Dy~(3+),Eu~(3+)系列荧光粉。用X射线衍射仪(XRD)、场发射扫描电镜(FESEM)、荧光光谱仪等对所得样品的结构、形貌和发光性能进行了表征,并研究了其能量传递机理。结果表明:白钨矿结构的Li Gd(Mo O_4)_2∶Dy~(3+),Eu~(3+)荧光粉的形貌为不规则颗粒,其粒径为1.8μm。在354 nm近紫外光激发下,该荧光粉显示出Dy~(3+)的特征黄、蓝光发射和Eu~(3+)的特征红光发射。计算Dy~(3+)和Eu~(3+)的临界距离为1.383 nm,Dy~(3+)→Eu~(3+)之间能量传递机理为偶极-四极相互作用。通过调节Dy~(3+)、Eu~(3+)的掺杂浓度,荧光粉可实现暖白光发射。此外,详细研究了稀土离子(Dy~(3+),Eu~(3+))的掺杂浓度与荧光粉的色温值之间的关系。     

Ba_3Y(PO_4)_3∶Dy~(3+),Eu~(3+)单基质白光荧光粉的制备与发光性能

为了探究在Dy~(3+)掺杂Ba_3Y(PO_4)_3荧光粉中共掺Eu~(3+)离子对其发光性能的影响,我们采用传统高温固相法制备了一系列Dy~(3+)、Eu~(3+)单掺杂和共掺杂Ba_3Y(PO_4)_3荧光粉。通过X射线衍射(XRD)、荧光发射光谱和荧光衰减曲线对样品进行了表征。结果表明,所制备的荧光粉呈闪铋矿立方相。在近紫外光激发下,Ba_3Y(PO_4)_3∶Dy~(3+)发射光谱在487和578 nm处有两个窄带发射峰,呈冷白光发射;Ba_3Y(PO_4)_3∶Eu~(3+)发射光谱的窄带发射位于594和616 nm处,呈发橙红光。在Ba_3Y(PO_4)_3∶Dy~(3+),Eu~(3+)中,由于Eu~(3+)离子补偿Dy~(3+)冷白光发射所缺的红色组分,从而实现了色纯度高、色温适中的暖白光发射。进一步探索了Ba_3Y(PO_4)_3∶Dy~(3+),Eu~(3+)荧光粉发光机理。所制备的Ba_3Y(PO_4)_3∶Dy~(3+),Eu~(3+)单基质白光荧光粉在白光近紫外激发白光二极管(UVWLED)领域具有潜在应用价值。     

Cr2(WO4)3和Cr2(MoO4)3的负热膨胀特性研究

用液相反应-前驱物烧结法制备了Cr₂(WO₄)₃和Cr₂(MoO₄)₃粉体。298～1 073 K的原位粉末X射线衍射数据表明Cr₂(WO₄)₃和Cr₂(MoO₄)₃的晶胞体积随温度的升高而增大, 本征线热膨胀系数分别为(1.274±0.003)×10^-6 K^-1和(1.612±0.003)×10^-6 K^-1。用热膨胀仪研究了Cr₂(WO₄)₃和Cr₂(MoO₄)₃在静态空气中298～1 073 K范围内热膨胀行为，即开始表现为正热膨胀，随后在相转变点达到最大值，最后表现为负热膨胀，其负热膨胀系数分别为(-7.033±0.014)×10^-6 K^-1和(-9.282±0.019)×10^-6 K^-1。     

Non-centrosymmetric Ba3Ti3O6(BO3)2

The compound previously reported as Ba₂Ti₂B₂O₉ has been reformulated as Ba₃Ti₃B₂O₁₂, or Ba₃Ti₃O₆(BO₃)₂, a new barium titanium oxoborate. Small single crystals have been recovered from a melt with a composition of BaTiO₃:BaTiB₂O₆ (molar ratio) cooled between 1100°C and 850°C. The crystal structure has been determined by X-ray diffraction: hexagonal system, non-centrosymmetric space group, a=8.7377(11) Å, c=3.9147(8) Å, Z=1, wR(F²)=0.039 for 504 unique reflections. Ba₃Ti₃O₆(BO₃)₂ is isostructural with K₃Ta₃O₆(BO₃)₂. Preliminary measurements of nonlinear optical properties on microcrystalline samples show that the second harmonic generation efficiency of Ba₃Ti₃O₆(BO₃)₂ is equal to 95% of that of LiNbO₃.     

可见光响应的Co3(PO4)2/Ag3PO4纳米复合光催化剂的制备及表征

采用简单的化学偏聚法合成出Ag₃PO₄纳米颗粒、磷酸钴（Co₃（PO₄）₂,CoP）纳米片以及它们两者的纳米复合结构（CoP/Ag₃PO₄）,同时还比较了它们的可见光催化活性. 采用场发射扫描电镜（FESEM）、X 射线衍射（XRD）、紫外-可见（UV-Vis）吸收光谱以及光致发光谱等手段对其形貌、结构、光学以及可见光催化性能等进行表征. 结果表明,CoP/Ag₃PO₄复合纳米结构的可见光降解甲基橙（MO）的速率和循环稳定性均明显优于其它两种物质. 这表明CoP应该起着共催化剂的作用,它能够抑制光生电子与空穴之间的复合,并且提供大量高活性的光生空穴. 此外,我们还发现CoP/Ag₃PO₄降解另一种阳离子型染料——罗丹明B（RhB）的能力则远不如纯Ag₃PO₄,这可能是与光催化剂的表面性质发生改变有关,造成更低的RhB吸附能力. 本文提供了一种廉价制备高效可见光催化剂的新方法.     

Eu0.5RE0.5Fe0.5Mn0.5O3的57Fe Msosbauer谱研究

利用固相反应合成了Eu0.5RE0.5Fe0.5Mn0.5O3(RE=La,Pr,Nd,Sm,Eu,Gd,Tb,Dy,Ho,Er,Tm,Yb,Y)等化合物。测量了其XRD谱及57FeMssbauer谱。实验发现,随着RE原子序数的增加,样品的晶胞体积减小,Fe在化合物中处于Fe3+的高自旋状态,57Fe的四极裂矩与样品的畸变参数D成线性关系。     

g-C3N4/Bi2O2CO32D纳米片复合材料的制备及可见光催化性能研究

采用自组装和化学沉淀法分别制得两种可见光驱动复合材料石墨相氮化碳/碳酸氧铋(g-C_3N_4/Bi_2O_2CO_3).采用X射线衍射光谱(XRD),紫外可见光谱、扫描电镜(SEM)、N_2吸附、电化学阻抗谱(EIS)和X射线光电子能谱(XPS)等分析手段对制备的催化剂进行了表征.结果表明,制备方法对纳米复合材料的晶相、形态及光学性能没有影响,但是影响g-C_3N_4和Bi_2O_2CO_3之间的相互作用力,导致光生电子-空穴对的分离速率存在显著差异.以可见光驱动苯酚和罗丹明B的降解实验为探针反应检测催化剂的光催化性能.实验结果表明自组装法得到的异质结催化剂中相互作用力更强,催化效果最高.O_2-是罗丹明B降解反应的主要活性物种,染料的光敏化、Bi_2O_2CO_3与g-C_3N_4综合效应,导致光生载流子电荷分离效率更高.     

Vibrational spectra of the peroxotantalates (NH4)3[Ta(O2)4], K3[Ta(O2)4], Rb3[Ta(O2)4] and Cs3[Ta(O2)4] and the crystal structure of Rb3[Ta(O2)4]

The compounds (NH₄)₃[Ta(O₂)₄], K₃[Ta(O₂)₄], Rb₃[Ta(O₂)₄] and Cs₃[Ta(O₂)₄] have been prepared and investigated by X-ray powder methods as well as Raman- and IR-spectroscopy. In the case of Rb₃[Ta(O₂)₄] the structure has been solved from single crystal data. It is shown that all these compounds are isotypic and crystallize in the K₃[Cr(O₂)₄] type (SG , No. 121). The infrared- and Raman spectra (recorded on powdered samples) are discussed with respect to the internal vibrations of the peroxo-group and the dodecahedral [Ta(O₂)₄]³⁻ ion. Symmetry coordinates for the [Ta(O₂)₄]³⁻ ion are given from which the vibrational modes of the O-O stretching vibrations of the O₂²⁻ groups, the Ta-O stretching vibrations and the Ta-O bending vibrations are deduced.     

Synthesis, crystal structure, infrared and Raman spectra of Sr4Cu3(AsO4)2(AsO3OH)4·3H2O and Ba2Cu4(AsO4)2(AsO3OH)3

The two new compounds, Sr₄Cu₃(AsO₄)₂(AsO₃OH)₄·3H₂O (1) and Ba₂Cu₄(AsO₄)₂(AsO₃OH)₃(2), were synthesized under hydrothermal conditions. They represent previously unknown structure types and are the first compounds synthesized in the systems SrO/BaO-CuO-As₂O₅-H₂O. Their crystal structures were determined by single-crystal X-ray diffraction [space group C2/c, a=18.536(4) Å, b=5.179(1) Å, c=24.898(5) Å, β=93.67(3)°, V=2344.0(8) Å³, Z=4 for 1; space group P4₂/n, a=7.775(1) Å, c=13.698(3) Å, V=828.1(2) Å³, Z=2 for 2]. The crystal structure of 1 is related to a group of compounds formed by Cu²⁺-(XO₄)³⁻ layers (X=P⁵⁺, As⁵⁺) linked by M cations (M=alkali, alkaline earth, Pb²⁺, or Ag⁺) and partly by hydrogen bonds. In 1, worth mentioning is the very short hydrogen bond length, D···A=2.477(3) Å. It is one of the examples of extremely short hydrogen bonds, where the donor and acceptor are crystallographically different. Compound 2 represents a layered structure consisting of Cu₂O₈ centrosymmetric dimers crosslinked by As1φ₄ tetrahedra, where φ is O or OH, which are interconnected by Ba, As2 and hydrogen bonds to form a three-dimensional network. The layers are formed by Cu₂O₈ centrosymmetric dimers of CuO₅ edge-sharing polyhedra, crosslinked by As1O₄ tetrahedra. Vibrational spectra (FTIR and Raman) of both compounds are described. The spectroscopic manifestation of the very short hydrogen bond in 1, and ABC-like spectra in 2 were discussed.     

A Structural Investigation of La2(GeO4)O and Alkaline-Earth-Doped La9.33(GeO4)6O2

The structures of the oxyorthogermanate La₂(GeO₄)O and the apatite-structured La_9.33(GeO₄)₆O₂ have been refined from powder neutron diffraction data. La₂(GeO₄)O crystallizes in a monoclinic unit cell (P2₁/c) and is cation stoichiometric in contrast to previous reports. La_9.33(GeO₄)₆O₂ crystallizes in a hexagonal unit cell (P6₃/m) and the powder diffraction data show anisotropic peak broadening that is observed in electron diffraction patterns as incommensurate diffuse spots at hkq reciprocal planes (with q=1.6-1.7) and can be attributed to a correlated disorder in the “apatite channels”. This compound was doped up to a nominal composition close to M₂La₈(GeO₄)₆O₂ with M=Ca, Sr, Ba. The dopant ions preferentially occupy the 4f sites as the number of La vacancies decreases. The measured ionic conductivity of La_9.33(GeO₄)₆O₂ is about 3 orders of magnitude larger than for La₂(GeO₄)O at high temperatures and decreases with increasing dopant content from the highest value of about 0.16 S cm⁻¹ at 1160 K.     

Sol-gel synthesis of K3InF6 and structural characterization of K2InC10O10H6F9, K3InC12O14H4F18 and K3InC12O12F18

K₃InF₆ is synthesized by a sol-gel route starting from indium and potassium acetates dissolved in isopropanol in the stoichiometry 1:3, with trifluoroacetic acid as fluorinating agent. The crystal structures of the organic precursors were solved by X-ray diffraction methods on single crystals. Three organic compounds were isolated and identified: K₂InC₁₀O₁₀H₆F₉, K₃InC₁₂O₁₄H₄F₁₈ and K₃InC₁₂O₁₂F₁₈. The first one, deficient in potassium in comparison with the initial stoichiometry, is unstable. In its crystal structure, acetate as well as trifluoroacetate anions are coordinated to the indium atom. The two other precursors are obtained, respectively, by quick and slow evaporation of the solution. They correspond to the final organic compounds, which give K₃InF₆ by decomposition at high temperature. The crystal structure of K₃InC₁₂O₁₄H₄F₁₈ is characterized by complex anions [In(CF₃COO)₄(OH_x)₂]^(5−2x)− and isolated [CF₃COOH_2−x]^(x−1)− molecules with x=2 or 1, surrounded by K⁺ cations. The crystal structure of K₃InC₁₂O₁₂F₁₈ is only constituted by complex anions [In(CF₃COO)₆]³⁻ and K⁺ cations. For all these compounds, potassium cations ensure only the electroneutrality of the structure. IR spectra of K₂InC₁₀O₁₀H₆F₉ and K₃InC₁₂O₁₂F₁₈ were also performed at room temperature on pulverized crystals.     

Ni-P-Zn3(PO4)2(ZnSnO3、ZnSiO3)纳米复合化学镀层性质和组成的研究

研究了温度、时间、浓度等对Ａ３钢片上Ｎi-P-Zn3(PO4)2、Ni-P-ZnSnO3和Ｎi-P-ZiSiO3纳米复合合化学镀层外貌的影响,用扫描电子显微镜（ＳＥＭ）观察外貌、称重法测定厚度;通过１０％ＮaCl溶液、１％Ｈ２Ｓ气体加速腐蚀试验,１０％ＣuSO4溶液点滴试验等多种手段测定其耐腐蚀性能,用Ｘ－射线光电子谱（ＸＰＳ）及俄歇电子能谱（ＳＥＳ）测定其价态组成,结果表明：在最佳施镀条件下,可得光亮、致密、耐腐蚀性强于Ａ３钢、磷化膜及Ｎi-P镀层的纳米复合化学镀层,镀层的原子百分组成约为（％）：Ｎi-P-Zn3(PO4)2:Ni70.00,P12.47,Zn3(PO4)213.93,C3.6;Ni-P-ZnSnO3;Ni77.56,P10.00,ZnSnO39.84,C2.6;Ni-P-NiSiO3,Ni83.00,P10.96,ZnSi5.15,C0.89.