纳米CaCO3的改性、表面结构与流变行为研究

采用铝锆偶联剂和棕榈酸改性纳米CaCO₃ 粉体. 借助 XRD, FTIR, 接触角及流变学等测试方法对纳米CaCO₃ 的表面结构进行表征. XRD 分析表明: 改性纳米 CaCO₃保持原样品完整的体相结构, 为方解石型纳米微晶. FTIR 分析证明: 表面改性剂与纳米 CaCO₃ 表面是以化学键合和物理吸附方式相结合, 粒子表面存在羧基等有机官能团的红外吸收特征. 通过测定苯和水在改性纳米CaCO₃粉末压片上的接触角, 计算了改性纳米 CaCO₃的表面能和极性分量, 并与未改性纳米CaCO₃ 进行比较. 结果表明, 经表面改性, 纳米 CaCO₃ 的表面能和极性分量明显降低, 其在有机溶液中的吸附功增大, 界面张力大大降低; 经棕榈酸改性的纳米 CaCO₃ 表现出较好的亲油疏水性, 而铝锆偶联剂改性的纳米 CaCO₃ 同时具有亲水性和亲油性. 以液体石蜡为溶剂, 研究了表面改性对纳米CaCO₃悬浮液流变行为的影响. 实验发现: 经过表面处理, 纳米 CaCO₃ 粉体悬浮液流变行为发生较大的变化, 稳态剪切黏度大大降低, 表现出较小的动态弹性储能模量和黏性损耗模量, 而损耗因子较大.     

纸张涂料用纳米CaCO3表面改性的研究

利用铝锆偶联剂对纳米CaCO₃进行表面改性。采用红外光谱(IR)、X射线衍射分析(XRD)、热分析(TG-DTG)对改性前后的纳米CaCO₃进行了表征。通过透射电镜(TEM)、粒度分析、吸油值、比表面积及静滴接触角等实验对纳米CaCO₃的表面改性效果进行评价。红外光谱分析表明，偶联剂以化学键合的方式在纳米CaCO₃的表面形成化学吸附。TEM及粒度分析结果显示，未改性纳米CaCO₃存在严重的团聚现象，而改性后纳米CaCO₃的分散性有很大改善。经表面改性，水滴在纳米CaCO₃粉体压片表面静滴接触角变大，改性纳米CaCO₃同时具有亲水性和亲油性，能够较好地分散在水和有机相中。将改性前后的纳米CaCO₃分别加入到纸张涂料体系中，制得纳米CaCO₃复合纸张涂料。涂料流变实验表明，经铝锆偶联剂表面改性的纳米CaCO₃制得的复合纸张涂料具有较高的动态弹性模量和粘性模量。     

Er3+/Yb3+共掺杂La2TiO5荧光粉体的制备及上下转换荧光性质

使用溶胶-凝胶法制备了Er³⁺单掺及Er³⁺/Yb³⁺共掺La₂TiO₅荧光粉体样品。经过1 100 ℃下3 h的煅烧,得到了较好的微晶。X射线粉末衍射测试表明样品中不含杂质相。扫描电镜观察表明样品颗粒范围为100~300 nm。紫外激发光谱中,在250~320 nm范围内出现Er离子和临近配位氧离子之间强烈的电荷转移跃迁峰,在350~500 nm出现Er离子f-f跃迁尖锐的吸收峰。在378 nm激发下,Er离子发射强烈的特征绿光(546 nm, ⁴S_3/2-⁴I_15/2),当Er离子物质的量分数达到1%,发射峰强度达到最大。在980 nm激发下的上转换光谱中,Yb离子的共掺杂有效的敏化上转换发光强度。详细讨论了样品的上下转换发光机理及相应能量传递过程。同时测试了样品的荧光衰减和量子产率。     

ZnWO4∶Er3+，Yb3+纳米棒的制备及发光性能

采用水热法以聚乙二醇为分散剂合成了Er³⁺,Yb³⁺共掺的ZnWO₄纳米棒。X射线衍射、透射电子显微镜分析结果表明：所得产物为直径约20 nm的ZnWO₄纳米棒。在激发波长为980 nm的半导体激光器做光源激发下,确定样品的3个发射峰的发光中心位于532、553和656 nm,分别对应于铒离子 ²H_11/2→ ⁴I_15/2, ⁴S_3/2→ ⁴I_15/2和 ⁴F_9/2→ ⁴I_15/2的跃迁。     

Er3+/Yb3+共掺杂La2TiO5荧光粉体的制备及上下转换荧光性质研究

使用溶胶-凝胶法制备了Er³⁺单掺及Er³⁺/Yb³⁺共掺La₂TiO₅荧光粉体样品。经过1 100 ℃下3 h的煅烧,得到了较好的微晶。X射线粉末衍射测试表明样品中不含杂质相。扫描电镜观察表明样品颗粒范围为100~300 nm。紫外激发光谱中,在250~320 nm范围内出现Er离子和临近配位氧离子之间强烈的电荷转移跃迁峰,在350~500 nm出现Er离子f-f跃迁尖锐的吸收峰。在378 nm激发下,Er离子发射强烈的特征绿光(546 nm, ⁴S_3/2-⁴I_5/2),当Er离子物质的量分数达到1%,发射峰强度达到最大。在980 nm激发下的上转换光谱中,Yb离子的共掺杂有效的敏化上转换发光强度。详细讨论了样品的上下转换发光机理及相应能量传递过程。同时测试了样品的荧光衰减和量子产率。     

一维异核配合物[KNd(bta)2(H2O)6]·H2O的水热合成，晶体结构和荧光性质

以双四唑胺(H₂bta)、NdCl₃·6H₂O、KOH为原料,用水热法合成了1个一维异核的Nd³⁺配合物[KNd(bta)₂(H₂O)₆]·H₂O。通过X-射线单晶衍射、元素分析、红外光谱对该配合物进行了结构表征。该化合物属于单斜晶系,P2₁/m空间群。每个Nd³⁺与2个来自bta^2-离子的4个氮原子和5个水分子形成了1个盖帽的四方双锥,通过bta^2-和水分子桥联配体把Nd³⁺和K⁺连接成一维链状结构,链与链之间通过O-H…N和N-H…O氢键作用形成三维超分子结构。紫外吸收光谱和荧光光谱表征结果显示该配合物的水溶液在292和412 nm表现出双四唑胺的特征吸收峰和荧光发射特征峰。     

超细钴纳米粒子催化1-己烯低压氢甲酰化反应的原位红外光谱研究

利用原位透射红外光谱研究了2.8 nm超细钴纳米粒子在2~3 MPa合成气(CO:H₂ = 1:1)和100 ^oC条件下催化的1-己烯氢甲酰化反应. 结果表明, 在反应中出现与Co₂(CO)₈类似的红外吸收峰(2071, 2041和2022 cm^-1), 被证明是不同Co位点端式吸附CO. 首次观测到了位于2054 cm^-1处吸收峰处的物种, 可能归属为RCH₂CH₂COCo. 通过此中间物种,产物醛可以在钴催化剂表面经由结合一个氢原子脱除反应而获得.     

CaCO3纳米微粒的层状液晶模板法制备及其生长过程中的形貌演变

在Triton X-100/n-C₁₀H₂₁OH/H₂O体系中，低角X射线衍射测试表明层状液晶的溶剂层厚度小于3 nm。利用层状液晶为模板制备了CaCO₃纳米微粒，并用透射电子显微镜(TEM)、X射线衍射(XRD)和选区电子衍射(SAED)进行了表征。TEM结果表明所得CaCO₃纳米粒子的形貌为球形，粒径在2～8 nm，分布较窄。XRD表明CaCO₃纳米微粒的物相为方解石型和球霰石型混合结构。在制备过程中，Ca(OH)₂的加入和CaCO₃纳米微粒的析出并未破坏层状液晶的对称性和长程有序性。此外，在Triton X-100/CH₃CH₂OH体系中，研究了CaCO₃纳米微粒的生长行为，发现小的纳米微粒先通过导向聚集生长成小的梭状物，然后小的梭状物继续生长，最后发生Ostwald陈化形成较为均一的两头尖的带状纳米结构，其宽度在50～200 nm，长度约为2 μm。     

多孔纳米Ce-M-O (M＝Pr, La)粉末的微波诱导燃烧合成及其表征

使用Ce(NO₃)₃•6H₂O, Pr(NO₃)₃•6H₂O, La(NO₃)₃•6H₂O, 尿素为原料, 利用微波引诱燃烧法合成了多孔纳米Ce-M-O (M＝Pr, La)固溶体. 使用XRD, X光电子能谱仪(XPS), Raman光谱仪, 红外光谱仪(FT-IR), 透射电镜(TEM), 场发射扫描电镜(FE-SEM)等仪器对纳米粉体进行了表征. XRD分析显示Ce-M-O粉体的粒径在20～50 nm之间, 且所有样品均具有萤石结构. XPS证明在Ce-Pr-O固溶体中Pr以＋3和＋4两种形式存在. Raman光谱表明随着M^3＋的掺杂, 在CeO₂晶格中产生氧缺陷, 且缺陷浓度随掺杂量增加不断提高. 红外光谱证明Ce—O键的吸收峰在1400 cm^－1左右, 且由于M^3＋的掺杂在2346 cm^－1的吸收峰消失. TEM照片说明样品具有类盘状的网络纳米微晶结构. 扫描图像说明产物具有多孔的外貌特征, 且孔径分布在2～40 nm之间.     

低温凝胶燃烧法合成Y2O3∶Er3+，Yb3+纳米晶上转换发光材料

分别以柠檬酸和甘氨酸为燃烧剂,采用低温凝胶燃烧法合成了Er³⁺、Yb³⁺共掺Y₂O₃纳米晶粉体。通过TG-DSC、XRD、SEM等分析手段对两种燃烧剂所对应的反应过程及纳米晶粉体的物理性能进行了分析,结果表明甘氨酸法具有更高的反应效率、更好的粉体分散性及粒径均匀性。在980 nm激光二极管(LD)激发下,对甘氨酸法所得样品的上转换发光性能分析表明,绿光和红光发射谱带分别来自于Er³⁺的⁴S_3/2/ ²H_11/2→ ⁴I_15/2和⁴F_9/2→ ⁴I_15/2跃迁。此外,对Er³⁺和Yb³⁺掺杂浓度、粉体煅烧温度对纳米晶样品上转换发光性能的影响进行了讨论。     

Li_(1.3)Ti_(1.7)Al_(0.3)(PO_4)_3,Na_(1.3)Ti_(1.7)Al_(0.3)(PO_4)_3的离子交换研究

研究了在不同温度下的NaNO3和AgNO3水溶液中Li1.3Ti1.7Al0.3(PO4)3和Na1.3Ti1.7Al0.3(PO4)3离子交换行为.实验表明Li1.3Ti1.7Al0.3(PO4)3和Na1.3Ti1.7Al0.3(PO4)3均显示出了高选择性与Na+和Ag+进行离子交换的特征,且对Ag+的选择性高于Na+.升高温度可显著提高Ag/Li和Ag/Na的交换反应速度.     

Crystal growth, structure determination, and optical properties of new potassium-rare-earth silicates K3RESi2O7 (RE=Gd, Tb, Dy, Ho, Er, Tm, Yb, Lu)

Single crystals of K₃RESi₂O₇ (RE=Gd, Tb, Dy, Ho, Er, Tm, Yb, Lu) were grown from a potassium fluoride flux. Two different structure types were found for this series. Silicates containing the larger rare earths, RE=Gd, Tb, Dy, Ho, Er, Tm, Yb crystallize in a structure K₃RESi₂O₇ that contains the rare-earth cation in both a slightly distorted octahedral and an ideal trigonal prismatic coordination environment, while in K₃LuSi₂O₇, containing the smallest of the rare earths, lutetium is found solely in an octahedral coordination environment. The structure of K₃LuSi₂O₇ crystallizes in space group P6₃/mmc with a=5.71160(10) Å and c=13.8883(6) Å. The structures containing the remaining rare earths crystallize in the space group P6₃/mcm with the lattice parameters of a=9.9359(2) Å, c=14.4295(4) Å, (K₃GdSi₂O₇); a=9.88730(10) Å, c=14.3856(3) Å, (K₃TbSi₂O₇); a=9.8673(2) Å, c=14.3572(4) Å, (K₃DySi₂O₇); a=9.8408(3) Å, c=14.3206(6) Å, (K₃HoSi₂O₇); a=9.82120(10) Å, c=14.2986(2) Å, (K₃ErSi₂O₇); a=9.80200(10) Å, c=14.2863(4) Å, (K₃TmSi₂O₇); a=9.78190(10) Å, c=14.2401(3) Å, (K₃YbSi₂O₇). The optical properties of the silicates were investigated and K₃TbSi₂O₇ was found to fluoresce in the visible.     

Near infrared study of aqueous rare-earth ethylsulfates

The near infrared spectra of aqueous solutions of the ethylsulfates of La, Nd, Gd, Tb, Er, Yb, Lu, Y, and Na have been determined from about 0.2 mol-dm^–3 to nearly saturation. The extinction coefficients of water have been calculated taking into account the absorption of ethylslfate anions determined in separate experiments. Their values appeared to be nearly the same as that of pure water. The relative contents of free OH groups in 0.5 and 0.7M solutions have been estimated from the absorbances at 1160 nm. They were lower in solutions of the heavy rare-earth ethylsulfates (Tb, Er, Yb, Lu) than in equimolar solutions of the lighter ones (La, Nd), confirming our previous view that secondary hydration of the heavy trivalent rare-earth cations is distinctly stronger than that of the lighter ones. A comparison of the spectra of these aqueous ethylsulfates with those of perchlorates shows that the structure-breaking ability of the C₂H₅SO ₄ ^– ion is much smaller than that of perchlorate anion.     

电感耦合等离子体光谱法(ICP-AES)测定银精矿中铜、铅、锌、砷、镉、钙、镁、锰含量

针对银精矿样品复杂,难消解的特点,研究了不同酸溶法和碱熔法对样品的消解情况,建立了硝酸,盐酸,氢氟酸,高氯酸消解银精矿的方法。根据元素灵敏度和抗干扰性,选定各元素的测定波长。通过酸溶样和碱熔样测定结果比对,验证了方法准确性。建立了四酸消解-电感耦合等离子体光谱法测定银精矿中铜、铅、锌、砷、镉、钙、镁、锰含量的方法,元素的线性相关系数均在0.9999以上。通过共存元素干扰实验,确定了银精矿中高含量元素(铜、铅、锌、铁、锑、铋等)对测定元素结果没有影响。方法检出限：Cu 0.0063 mg/L, Pb 0.0159 mg/L ,Zn 0.0090 mg/L,As 0.0192 mg/L, Cd 0.0093 mg/L ,Ca 0.0084 mg/L, Mg 0.0075 mg/L, Mn 0.0081 mg/L。测定下限：Cu 0.0105mg/L,Pb 0.0265 mg/L, Zn 0.0150 mg/L, As 0.0320 mg/L, Cd 0.0155 mg/L, Ca 0.0140 mg/L, Mg 0.0125 mg/L,Mn 0.0135 mg/L。3个样品的相对标准偏差在0.87%~3.56%之间,加标回收率在95.00%~103.56%之间。方法流程短,操作简单,快速,灵敏度和再现性高,结果准确可靠,可以满足银精矿中铜、铅、锌、砷、镉、钙、镁、锰含量的测定。     

Structural studies of five layer Aurivillius oxides: A2Bi4Ti5O18 (A=Ca, Sr, Ba and Pb)

The room temperature structures of the five layer Aurivillius phases A₂Bi₄Ti₅O₁₈ (A=Ca, Sr, Ba and Pb) have been refined from powder neutron diffraction data using the Rietveld method. The structures consist of [Bi₂O₂]²⁺ layers interleaved with perovskite-like [A₂Bi₂Ti₅O₁₆]²⁻ blocks. The structures were refined in the orthorhombic space group B2eb (SG. No. 41), Z=4, and the unit cell parameters of the oxides are a=5.4251(2), b=5.4034(1), c=48.486(1); a=5.4650(2), b=5.4625(3), c=48.852(1); a=5.4988(3), b=5.4980(4), c=50.352(1); a=5.4701(2), b=5.4577(2), c=49.643(1) for A=Ca, Sr, Ba and Pb, respectively. The structural features of the compounds were found similar to n=2-4 layers bismuth oxides. The strain caused by mismatch of cell parameter requirements for the [Bi₂O₂]²⁺ layers and perovskite-like [A₂Bi₂Ti₅O₁₆]²⁻ blocks were relieved by tilting of the TiO₆ octahedra. Variable temperature synchrotron X-ray studies for Ca and Pb compounds showed that the orthorhombic structure persisted up to 675 and 475 K, respectively. Raman spectra of the compounds are also presented.     

B2O3-Bi2O3-ZnO-Al2O3玻璃助烧剂对BaTiO3陶瓷烧结条件、晶体结构和介电性能的影响

通过调节B₂O₃-Bi₂O₃-ZnO-Al₂O₃(BBZA)玻璃的添加量研究其对钛酸钡(BaTiO₃)陶瓷烧结条件、晶体结构和介电性能的影响。结果表明：添加适量的BBZA玻璃能够有效地将BaTiO₃陶瓷烧结温度由1 350℃降至950℃,并使其致密化。同时,添加BBZA玻璃后,BaTiO₃的晶体结构随着烧结温度的升高而发生转变(立方相→四方相)。另外,BBZA玻璃的引入使BaTiO₃陶瓷的居里峰得到了有效的抑制和拓宽。陶瓷微观形貌显示,玻璃相均匀分布在BaTiO₃晶粒表面。优化的BaTiO₃陶瓷制备条件如下：BBZA添加量(质量分数)为2.0%,烧结温度为950℃。在该条件下制备的BaTiO₃陶瓷介电常数达到1 364,介电损耗低至1.2%。     

Preparation of ZrO2-TiO2-CeO2 and Its Application in the Selective Catalytic Reduction of NO with NH3

TiO₂,ZrO₂-TiO₂,andZrO₂-TiO₂-CeO₂ were prepared by co-precipitation method and characterized by X-ray diffraction (XRD), specific surface area measurements (BET), temperature programmed desorption (NH₃-TPD), oxygen storage capacity (OSC), and temperature programmed reduction (H₂-TPR). The results showed that ZrO₂-TiO₂-CeO₂ exhibited large number of surface strong acid, possessed some oxygen storage capacity, and strong redox property. The three materials were used as supports and the monolith catalysts were prepared with 1% (w) V₂O₅ and 9% (w)WO₃ for selective catalytic reduction (SCR) of NO with ammonia in the presence of excessive O₂, and the results of catalytic activity showed that the catalyst used ZrO₂-TiO₂-CeO₂ as support yielded nearly 100% NO conversion at 275 °C at a gas hourly space velocity (GHSV) of 10000 h⁻¹, and it had the best catalytic activity and showed great potential for practical application.     

The crystal chemistry of Bi6TP2O15+x, T=Fe, Ni, Zn: Isomorphism and polymorphism, structural relationship to Bi6TiP2O16

The crystal structures of compounds with nominal compositions Bi₆FeP₂O_15+x (I), Bi₆NiP₂O_15+x (II) and Bi₆ZnP₂O_15+x (III) were determined from single-crystal X-ray diffraction data. They are monoclinic, space group I2, Z=2. The lattice parameters for (I) are a=11.2644(7), b=5.4380(3), c=11.1440(5) Å, β=96.154(4)°; for (II) a=11.259(7), b=5.461(4), c=11.109(7) Å, β=96.65(1)°; for (III) a=19.7271(5), b=5.4376(2), c=16.9730(6) Å, β=131.932(1)°. Least squares refinements on F² converged for (I) to R1=0.0554, wR₂=0.1408; for (II) R₁=0.0647, wR₂=0.1697; for (III) R₁=0.0385, wR₂=0.1023. The crystals are complexly twinned by 2-fold rotation about , by inversion and by mirror reflection. The structures consist of edge-sharing articulations of OBi₄ tetrahedra forming layers in the a-c plane that then continue by edge-sharing parallel to the b-axis. The three-dimensional networks are bridged by Fe and Ni octahedra in (I) and (II) and by Zn trigonal bipyramids in (III) as well as by oxygen atoms of the PO₄ moieties. Bi also randomly occupies the octahedral sites. Oxygen vacancies exist in the structures of the three compounds due to required charge balances and they occur in the octahedral coordination polyhedron of the transition metal. In compound (III), no positional disorder in atomic sites is present. The Bi-O coordination polyhedra are trigonal prisms with one, two or three faces capped. Magnetic susceptibility data for compound (I) were obtained between 4.2 and 350 K. Between 4.2 and 250 K it is paramagnetic, μ_eff=6.1 μ_B; a magnetic transition occurs above 250 K.     

Structure Study of Bi2.5Na0.5Ta2O9 and Bi2.5Nam−1.5NbmO3m+3 (m=2-4) by Neutron Powder Diffraction and Electron Microscopy

The crystal structures of Bi_2.5Na_0.5Ta₂O₉ and Bi_2.5Na_m-1.5Nb_mO_3m+3 (m=3,4) have been investigated by the Rietveld analysis of their neutron powder diffraction patterns (λ=1.470 Å). These compounds belong to the Aurivillius phase family and are built up by (Bi₂O₂)²⁺ fluorite layers and (A_m-1B_mO_3m+1)^2- (m=2-4) pseudo-perovskite slabs. Bi_2.5Na_0.5Ta₂O₉ (m=2) and Bi_2.5Na_2.5Nb₄O₁₅ (m=4) crystallize in the orthorhombic space group A2₁am, Z=4, with lattice constants of a=5.4763(4), b=5.4478(4), c=24.9710 (15) and a=5.5095(5), b=5.4783(5), c=40.553(3) Å, respectively. Bi_2.5Na_1.5Nb₃O₁₂ (m=3) has been refined in the orthorhombic space group B2cb, Z=4, with the unit-cell parameters a=5.5024(7), b=5.4622(7), and c=32.735(4) Å. In comparison with its isostructural Nb analogue, the structure of Bi_2.5Na_0.5Ta₂O₉ is less distorted and bond valence sum calculations indicate that the Ta-O bonds are somewhat stronger than the Nb-O bonds. The cell parameters a and b increase with increasing m for the compounds Bi_2.5Na_m-1.5Nb_mO_3m+3 (m=2-4), causing a greater strain in the structure. Electron microscopy studies verify that the intergrowth of mixed perovskite layers, caused by stacking faults, also increases with increasing m.     

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.