白光用红色荧光粉Gd2SrAl2O7:Eu3+的合成及发光性能研究

用传统的固态反应法合成了新型红色Eu3+掺杂的Gd2SrAl2O7红色荧光粉。通过添加Li2CO3助熔剂,有效地降低了反应温度,获得了纯Gd2SrAl2O7相。用X射线衍射仪分析确认了产物为Gd2SrAl2O7晶相,并用光谱仪测试了光谱性能,发现当Eu3+掺杂浓度为30%时,荧光粉在623 nm处有最强发光,是Y2O3:Eu3+的两倍。(Gd0.7Eu0.3)2SrAl2O7(x=0.650,y=0.349)色度值与美国国家电视标准委员会标准值(x=0.670,y=0.330)接近。     

纳米稀土磷酸盐红色荧光粉的合成及性能

以Gd,Y和Eu的硝酸盐与(NH4)2HPO4为原料,采用室温固相反应合成出前驱体,再经过900℃煅烧2h得到(Gd,Y,Eu)PO4纳米荧光粉,运用TG-DTA、XRD、TEM、固体荧光等技术,研究了荧光粉的形成过程、晶体尺寸、形貌及发光性能.结果表明:荧光粉属于单斜晶系,独居石结构的正磷酸盐,空间群为P21/n,平均粒径为60 nm,分散性好,有较高的热稳定性.在396 nm紫外光激发下,纳米荧光粉发出Eu3+的特征红色荧光,发射主峰在613nm,归属于Eu3+离子的5D0→7F2跃迁,该纳米粉体是一种性能优良的荧光材料.     

核壳型Gd2O3:Eu3+@Y2O3纳米发光材料的制备与发光性能

采用均相沉淀法制备了均匀球形的Gd2O3:Eu3+@Y2O3核壳结构纳米发光材料.XRD结果表明经过800℃焙烧后样品为立方晶系的Gd2O3,并且晶体发育良好,包覆Y2O3之后Gd2O3的衍射峰位置无明显变化,但随着包覆厚度的增加,出现了立方晶系Y2O3的衍射峰.FTIR谱图观测到了Gd-O,Y-O伸缩振动吸收峰,随着包覆厚度的减少吸收峰增强,认为当包覆层的厚度适当时,颗粒表面的悬空键(断键)变少,Gd(Eu,Y)-O键增多所致.SEM表明包覆前后样品为均匀分散的球形结构.XPS分析进一步证明了表面包覆上了Y2O3.荧光光谱表明:纳米Gd2O3:Eu3+表面包覆不同厚度的基质Y2O3后,均观测到Eu3+离子的特征红光发射,当包覆厚度R=4:1时的发光强度比未包覆的Gd2O3:Eu3+增强,认为核-壳型样品降低了纳米Gd2O3:Eu3+的表面效应给发光强度带来的负面影响.     

碳酸盐共沉淀法合成Lu2O3∶Er3+纳米粉体及性能表征

分别以硫酸铵、聚丙烯酰胺和聚乙二醇为分散剂,采用碳酸盐共沉淀法合成了Er3+掺杂Lu2O3纳米粉体。应用FTIR、TG-DSC、XRD、SEM等测试方法研究了前驱沉淀物的热分解过程,以及不同类型分散剂对Lu2O3∶Er3+纳米粉体晶粒尺寸和分散性的影响。结果表明,以(NH4)2SO4和PAM为分散剂时,前驱体经1 000℃煅烧2 h所得粉体为粒径在50~70 nm之间的球形颗粒,粉体分散性较好。此外,探讨了在980 nm激光激发下Lu2O3∶Er3+粉体的上转换发光性能。     

氨水共沉淀法制备Nd∶Y2O3透明陶瓷纳米粉体

以Y2O3粗粉、Nd2O3、硝酸和氨水为原料,通过共沉淀法制备了Nd:Y2O3透明陶瓷纳米粉体,利用热重/差热分析(TG/DTA)、红外光谱(FTIR)、粉末X射线衍射(XRD)、透射电镜(TEM)以及能谱分析(EDS)等方法对合成的Nd:Y2O3纳米粉体进行了表征.结果表明,在前驱物中添加适量SO42-离子能减轻煅烧得到的Nd:Y2O3纳米粉体粒子的团聚,使Nd:Y2O3纳米粒子的粒度均匀并呈球形分布.在600～1000℃煅烧3 h所得粉体粒子的粒径在20～40 nm之间,具有较好的分散性.     

Gd3Ga5O12∶Eu3+发光纳米晶的燃烧合成及性质

以尿素为燃烧剂,乙二醇为分散剂采用燃烧法制备了Gd3Ga5O12∶Eu3+纳米晶。利用X射线衍射、电镜和荧光光谱对前驱体和热处理后样品的结构、形貌和发光性能进行了表征。XRD结果表明:700℃热处理2 h即可获得立方结构Gd3Ga5O12∶Eu3+纳米晶。根据Scherrer公式估算经700℃和900℃热处理2 h获得的纳米晶的一次性粒径分别为28 nm和42 nm。发射光谱和激发光谱的结果表明:特征发射峰来自于5D0-7FJ跃迁,而来自于Eu3+的5D0→7F1的磁偶极跃迁发射最强;宽激发带主要来自于Eu-O电荷迁移带和Gd3Ga5O12基质吸收。发射强度和激发强度随热处理温度的提高而增强。     

高温固相法合成R_(2-x)(MoO_4)_3∶xEu~(3+)(R=Y,Gd)红色荧光粉的研究

采用高温固相法合成R2-x(MoO4)3∶xEu3+(R=Y,Gd)系列红色荧光粉.研究了煅烧温度、助熔剂的含量和Eu3+的掺杂量对样品发光性能的影响,并对样品的物相组成、激发和发射光谱进行分析.结果表明,样品Gd0.6(MoO4)3∶1.4Eu3+在800℃左右煅烧时呈单斜晶结构,当煅烧温度提高到950℃左右,呈正交斜晶结构;样品Y0.2(MoO4)3∶1.8Eu3+在800℃左右煅烧时已经完全形成了正交结构,当煅烧温度升高到1000℃左右时,其正交结构得到保持,没有发生相变.其中,助熔剂NH4Cl的含量占样品总量的3%,煅烧温度为1000℃,保温3h得到的样品Gd0.6(MoO4)3∶1.4Eu3+和Y0.2(MoO4)3∶1.8Eu3+的发光性能达到最佳.另外,由激发和发射光谱分析表明,该荧光粉可以被近紫外光(395nm)和蓝光(465nm)有效激发,发射峰值位于612nm的红光,对应于Eu3+离子的5 D0→7 F2跃迁,是一种可应用在紫外光和蓝光芯片激发产生白光LED的红色荧光粉.     

(Y,Gd)BO_3∶Eu的真空紫外光谱特性

近年来由于等离子体平板显示 (PDP)技术的需要 ,对真空紫外 (VUV)光激发的荧光粉的研究成为发光材料领域中的一个新方向 [1～ 3] .由于技术和实验仪器等方面的原因 [4 ] ,以往人们对稀土发光材料VUV区的研究很少 ,缺乏对其光谱和能级的完整认识 .另外 ,稀土离子 Gd3+在荧光粉的能量传递中具有特殊作用 ,一些含 Gd3+的发光材料在 VUV区发光效率很高 ,例如 ,(Y,Gd) BO3∶ Eu在 VUV区的发光效率比 YBO3∶ Eu提高了 2 0 % ,比 Y2 O3∶ Eu提高了 1 .8倍 ,与其它红粉相比更具有实际应用价值 [4 ,5] .但目前对于 (Y,Gd) BO3∶ Eu的研…     

白光LED用(Y_xGd_(1-x))(P,W)O_4:Eu红色荧光粉的发光性能研究

采用高温固相方法合成了(YxGd1-x)(P0.5W0.5)O4:Eu0.15粉末状发光材料,经X衍射分析结构发现,当Y3+/Gd3+≤3∶7时,样品主要由Gd2WO6相和Gd PO4相组成,当Y3+/Gd3+接近或等于1∶1时,合成的样品由Gd2WO6相、Gd PO4相和Gd0.5Y0.5PO4相三相组成,当Y3+/Gd3+≥7∶3时,合成的样品由Gd2WO6相与Gd0.5Y0.5PO4相组成。研究了样品在蓝光激发下的光谱性质,讨论了Y3+/Gd3+的掺杂对材料发光性能的影响,发现当Y3+/Gd3+=7∶3时,样品发光强度最高。在蓝光激发下,样品的发射光谱主峰在611.5 nm,对应于Eu3+的5D0→7F2电偶极跃迁。在添加助熔剂试验中发现,粉体中加入NH4NO3做助熔剂效果最好,其最佳掺入浓度为3%(质量分数)。     

Gd2O3∶Eu3+纳米棒的制备与发光性能

在表面活性剂辅助的水热条件下合成出尺寸均一的Gd2O3∶Eu3+纳米棒, 对其结构和荧光性质进行了表征, 并对其生长机理进行了初步讨论. XRD结果表明, 水热前驱体样品为六方晶相的Gd(OH)3, 经过灼烧之后样品为立方相的Gd2O3. TEM照片表明, 所得样品为直径60 nm、长度约600 nm的纳米棒. 荧光光谱表明, 在波长为254 nm 的紫外光激发下, Gd2O3∶Eu3+纳米棒产生了不同于前驱体的特征红光发射, 对应于Eu3+ 的5D0-7F2跃迁, 表明Gd2O3是红色发光材料的良好基质.     

Synthesis of some derivatives of 3-amino-3-desoxyerythrose and 3-amino-3-desoxy-D-3-erythrose

The synthesis of derivatives of 3-amino-3-deoxy-L-erythrose by LAH or LAD reduction of the oxime of 1,2-O-isopropylidene α-L -glycero-tetros-3-ulofuranose is described.     

Synthesis of γγγ-trifluorocarbonyl compounds

γγγ-Trifluorocarbonyl compounds are easily obtained in a good yield by introduction of the 1,1,1-trifluoroethyl moiety (CF₃-CH₂-) on the -methylene group of a ketone.     

Vibrational spectra of CH3GeH3 and CD3GeH3

Infrared gas phase spectra of CH₃GeH₃ and CD₃GeH₃ have been investigated at a resolution of 0.06 cm⁻¹ and Raman spectra obtained in the liquid phase at low resolution. Several reassignments of the fundamental frequencies are proposed. Q-branch maxima from the five naturally occurring Ge isotopes have been resolved in several of the fundamental vibrations and new values obtained of rotational and Coriolis coupling constants for ν₇, ν₈, ν₁₀ and ν₁₂ of CH₃GeH₃ and ν₇, ν₈, ν₉, ν₁₀ and ν₁₂ of CD₃GeH₃. Germanium isotopic frequency shifts on ν_GeC are also reported.     

Freezing the polarization of CH3NH3PbI3 and CH3NH3PbI3-xClx perovskite films

Thin films of methylammonium lead halides, CH₃NH₃PbI₃ and CH₃NH₃PbI_3-xCl_x, were deposited onto symmetrical microstructured electrode arrays of gold or platinum on Si/SiO₂ wafers. Polarization studies were carried out on perovskite films under vacuum in the dark. For poling, a constant voltage was applied to the samples while the temperature was cycled between 295 K and 4 K. The measured current densities depending on the temperature showed distinct characteristics relating strongly to the crystal phase and the dielectric properties of the perovskite films. Voltage sweeps were carried out at different scan rates at specific temperature intervals after poling. The polarization of the films due to the migration of iodide vacancies in direction of the blocking perovskite/metal interface was frozen almost up to room temperature. Charge carriers were only able to cross the blocking barrier and contribute to the current where the ions have accumulated during poling. All J-V curves showed hysteresis: inverted and regular hysteresis at room temperature and below, respectively. Inverted hysteresis originates from the slow accumulation of ions at the blocking barrier, while regular hysteresis arises from a distortion in the adjacent crystals which will be discussed.     

钙钛矿CH3NH3PbI3晶体的电化学

电化学方波伏安及循环伏安测量表明,钙钛矿CH₃NH₃PbI₃晶体在有机电解质中的氧化还原过程伴随着化学降解。该化学降解源于CH₃NH₃PbI₃晶体中铅离子的还原以及碘离子的氧化。通过电化学伏安法可以测定晶体的能带。     

Non-Isothermal Kinetics of the Decomposition Reaction of Cluster [Ag3WS3Br]（PPh3）3 and [Cu3WS3Br]（PPh3）3

The thermal behaviors of clusters [Ag3WS3Br](PPh3)3 and [Cu3WS3Br](PPh3)3 (PPh3=triphenyl phosphine) in a nitrogen atmosphere were studied under the non-isothermal conditions by simultaneous TG-DTG-DSC and EDS techniques. The results showed that the evolution of PPh3 generally proceeded before the release of the other moiety in one or two step-mode. The mechanisms, the kinetic and the thermodynamic parameters for decomposition of PPh3 of both clusters were determined and calculated by jointly using several methods, which showed that its evolution was controlled by Avrami-Erofeev equation. The results also showed that there was no new stable phase composed of W-Ag(Cu)-S-Br after release of organic moiety PPh3 and that CVD method was not applicable to their further processing.     

Addition of NH3 to Al3O3-

Recent computational studies on the addition of ammonia (NH3) to the Al3O3- cluster anion [A. Guevara-Garcia, A. Martinez, and J. V. Ortiz, J. Chem. Phys. 122, 214309 (2005)] have motivated experimental and additional computational studies, reported here. Al3O3- is observed to react with a single NH3 molecule to form the Al3O3NH3- ion in mass spectrometric studies. This is in contrast to similarly performed studies with water, in which the Al3O5H4- product was highly favored. However, the anion PE spectrum of the ammoniated species is very similar to that of Al3O4H2-. The adiabatic electron affinity of Al3O3NH3 is determined to be 2.35(5) eV. Based on comparison between the spectra and calculated electron affinities, it appears that NH3 adds dissociatively to Al3O3-, suggesting that the time for the Al3O3-NH3 complex to either overcome or tunnel through the barrier to proton transfer (which is higher for NH3 than for water) is short relative to the time for collisional cooling in the experiment.