铁掺杂HTiNbO5纳米片及其催化环氧苯乙烷醇解的性能

通过先将层状HTiNbO₅用四丁基氢氧化铵层离成单层纳米片,然后与铁溶胶重组,最后在不同温度（200~500℃）下焙烧,得到了一系列铁掺杂的HTiNbO₅纳米片。研究结果表明,铁溶胶掺杂有利于提高催化剂的比表面积和酸性,所得催化剂在环氧苯乙烷的醇解反应中表现出很好的催化效果。其中,水解时间为1h的铁溶胶与HTiNbO₅纳米片重组且在400℃下焙烧后所得催化剂的催化效果最好,优于未掺杂和Fe³⁺直接絮凝的HTiNbO₅纳米片。     

钆及双稀土元素掺杂TiO2可见光催化降解罗丹明B的研究

以钛酸丁酯为前驱体，采用溶胶一凝胶法制备了钆及双稀土元素共掺杂纳米TiO2光催化剂，研究了自制催化剂在可见光下对有机染料罗丹明B催化降解反应的活性。稀土掺杂后的TiO2在可见光下催化活性比纯的TiO2有显著的提高。当Gd^3＋与TiO2的摩尔比为1．5％，催化剂经过500℃焙烧，对罗丹明B的降解率达到99．5％；Gd^3＋：La^3＋：TiO2的摩尔比为O．5：0．5：100，焙烧温度为600℃，降解率高达99．9％，比双元素掺杂的结果更好。     

纳米Ni/TiO_2粉体的制备及其光催化性能

以四氯化钛为主要原料,通过溶胶法合成了纳米TiO2和Ni/TiO2粉体。研究发现掺杂镍,能够有效延缓锐钛矿型TiO2向金红石型TiO2转变,提高Ni/TiO2粉体的催化活性;在500℃焙烧的Ni/TiO2催化剂,能较好催化溴甲酚绿染料在紫外光下降解。     

S掺杂的HTiNbO5纳米片: 一种新型高效可见光催化剂

将层状HTiNbO₅剥层絮凝成HTiNbO₅纳米片, 然后与硫脲焙烧, 制得了S掺杂的HTiNbO₅纳米片. 与原始HTiNbO₅和HTiNbO₅纳米片相比, 该样品具有较大的比表面积和明显的可见光吸收. 以罗丹明B为降解物, 评价了该催化剂的吸附性能和可见光催化性能. 结果表明, HTiNbO₅纳米片和S掺杂的HTiNbO₅纳米片都具有很好的吸附能力和很高的可见光降解速率. 然而, 对于罗丹明B的矿化, S掺杂的HTiNbO₅纳米片可以达到41%矿化率, 而HTiNbO₅纳米片上矿化单几乎为零. 这说明S掺杂能有效改善纳米片的光催化效果. 最后, 对可能的光催化机理进行了探讨.     

纳米Fe/TiO_2粉体的制备及其光催化性能

光催化法是近年来发展较快的一种环境治理技术,掺杂型TiO_2催化剂是当前研究的焦点之一.以四氯化钛为主要原料,利用简单的溶胶法制备了纳米TiO_2、Fe/TiO_2粉体,研究发现掺杂铁,能够有效地延缓锐钛矿型TiO_2向金红石型TiO_2的转变,提高Fe/TiO_2粉体的光催化活性,并且500℃焙烧后的Fe/TiO_2催化剂,在紫外光下催化活性较好.     

蛋氨酸改性TiO2空心纳米盒高效可见光催化RhB分解和NO氧化

由高能面 TiO2纳米片 (TiO2-NSs) 组装成的 TiO2空心纳米盒 (TiO2-HNBs)显示出比单独 TiO2-NSs 更强的光催化性能, 但是 TiO2-HNBs 依然属于紫外光催化剂, 无法充分利用太阳能. 因此, 开发具有可见光响应的由高能面 TiO2-NSs 组装而成的 TiO2-HNBs 具有重要意义. 本文将立方体 TiOF2与含有 N 和 S 元素的生物分子蛋氨酸混合, 通过一步焙烧制备了具有可见光响应活性的 N 和 S 元素共掺杂的 TiO2-HNBs(掺杂催化剂标记为 TMx, 未掺杂催化剂标记为 Tx, x 代表焙烧温度).由立方体 TiOF2到锐钛矿相 TiO2空心纳米盒的转变是一个自模板转化过程. 氟离子的存在降低了 TiO2高能面(001)面的表面能, 从而使得高能面 TiO2纳米片的形成变得可能. 因此, 热处理立方体 TiOF2可得到由高能面 TiO2纳米片组装的 TiO2空心纳米盒.本文系统研究了焙烧温度 (300-500 ℃) 对所制 TiO2-HNBs 结构与光催化性能的影响. 结果发现, 在 350 ℃下焙烧, TiOF2完全转化成锐钛矿相 TiO2-HNBs. 但是焙烧蛋氨酸与 TiOF2的混合物, 需 400 ℃才能完全实现 TiOF2到锐钛矿相TiO2-HNBs 的转变. 这说明蛋氨酸的加入阻碍了 TiOF2向锐钛矿相 TiO2-HNBs 的转变. XPS 结果显示, 经过 400 ℃焙烧的蛋氨酸改性样品 (TM400), N 和 S 元素成功掺入了 TiO2-HNBs 晶格, 使其产生可见光催化活性.相对于 400 ℃焙烧 TiOF2所得样品 T400, 蛋氨酸改性的 TM400 催化剂可见光降解罗丹明 B 染料 (RhB) 和 NO 氧化的性能分别提升了 1.55 倍和 2.0 倍, 这与其更强的可见光吸收性能和光生载流子分离效率有关. 400 ℃焙烧的蛋氨酸改性的 TM400 可见光催化活性稳定, 连续 5 次可见光催化 RhB 降解后, 其活性没有明显改变, 显示了潜在的应用前景.     

焙烧方法和焙烧条件对纳米Au/HZSM-5催化剂金粒径和催化性能的影响

采用负压沉积沉淀法制备了纳米Au/HZSM-5催化剂前体,研究了深床焙烧和等离子体焙烧两种方法,以及焙烧温度和焙烧气氛对催化剂中纳米金粒径和催化性能的影响,并采用ICP、TEM、XRD、UV-vis、XPS等表征方法对催化剂金粒子进行了物化性能表征,采用合成气羰基化制乙酸甲酯反应表征催化性能。结果表明,不同焙烧方法和不同焙烧温度及气氛对负载型纳米Au/HZSM-5催化剂中金粒径、形貌、物化性质和催化性能有明显影响。其中,以等离子体焙烧方法在500℃氮气气氛下制备的纳米1.86%Au/HZSM-5催化剂中的金粒径最小,为2-5 nm。用于催化合成气羰基化制乙酸甲酯反应,原料中CO的转化率为67%,乙酸甲酯选择性可达78%。     

蛋氨酸改性TiO_2空心纳米盒高效可见光催化RhB分解和NO氧化（英文）

由高能面TiO_2纳米片(TiO_2-NSs)组装成的TiO_2空心纳米盒(TiO_2-HNBs)显示出比单独TiO_2-NSs更强的光催化性能,但是TiO_2-HNBs依然属于紫外光催化剂,无法充分利用太阳能.因此,开发具有可见光响应的由高能面TiO_2-NSs组装而成的TiO_2-HNBs具有重要意义.本文将立方体TiOF_2与含有N和S元素的生物分子蛋氨酸混合,通过一步焙烧制备了具有可见光响应活性的N和S元素共掺杂的TiO_2-HNBs(掺杂催化剂标记为TMx,未掺杂催化剂标记为Tx,x代表焙烧温度).由立方体TiOF_2到锐钛矿相TiO_2空心纳米盒的转变是一个自模板转化过程.氟离子的存在降低了TiO_2高能面(001)面的表面能,从而使得高能面TiO_2纳米片的形成变得可能.因此,热处理立方体TiOF2可得到由高能面TiO_2纳米片组装的TiO_2空心纳米盒.本文系统研究了焙烧温度(300.500 oC)对所制TiO_2-HNBs结构与光催化性能的影响.结果发现,在350 ℃下焙烧,TiOF_2完全转化成锐钛矿相TiO_2-HNBs.但是焙烧蛋氨酸与TiOF2的混合物,需400 ℃才能完全实现TiOF_2到锐钛矿相TiO_2-HNBs的转变.这说明蛋氨酸的加入阻碍了TiOF_2向锐钛矿相TiO_2-HNBs的转变.XPS结果显示,经过400℃焙烧的蛋氨酸改性样品(TM400),N和S元素成功掺入了TiO_2-HNBs晶格,使其产生可见光催化活性.相对于400 ℃焙烧TiOF_2所得样品T400,蛋氨酸改性的TM400催化剂可见光降解罗丹明B染料(RhB)和NO氧化的性能分别提升了1.55倍和2.0倍,这与其更强的可见光吸收性能和光生载流子分离效率有关.400 ℃焙烧的蛋氨酸改性的TM400可见光催化活性稳定,连续5次可见光催化RhB降解后,其活性没有明显改变,显示了潜在的应用前景.     

纳米NiO催化乙烷低温氧化脱氢制乙烯

 用溶胶-凝胶法制备了纳米氧化镍。TEM结果表明，在380℃下焙烧的氧化镍粒子大小在10 nm以下。与大尺寸氧化镍相比，纳米氧化镍对乙烷氧化脱氢反应的催化性能有较大的改善，在获得相当收率时反应温度大约下降125℃。关于热点问题，可以通过催化剂与石英沙混合得到解决。     

纳米Co/TiO2 粉体的制备及其光催化性能

以钛酸丁酯为主要原料,利用溶胶-凝胶法制备了纳米TiO2,Co/TiO2粉体.掺杂钴能够延缓TiO2由锐钛矿相向金红石相转变,从而提高纳米Co/TiO2粉体的催化活性.经500 ℃焙烧的纳米Co/TiO2粉体,在紫外光源下能有效催化直接溴酚兰染料降解.     

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.     

Metal-organic deposition of YBa2Cu3Ox and Bi2Sr2Ca1Cu2Ox films on various substrates starting from different fluorine-free metallorganic compounds

YBa₂Cu₃O_x (Y-123) and Bi₂Sr₂Ca₁Cu₂O_x (Bi-2212) films on various substrates have been prepared by Metal-Organic Deposition starting from different metallorganic fluorine-free compounds and using a very simple instrumentation. The processing conditions include a rapid pyrolysis step in air and an annealing step in oxygen for Y-123 and in air for Bi-2212. The films obtained have been characterized by X-ray diffraction (XRD) and the formation of a superconducting phase of Y-123 or Bi-2212 was confirmed measuring the critical temperature (T _c) with Ac-susceptibility and resistive measurements. Microstructure and final cationic ratios have been studied by scanning electron microscopy (SEM) and energy dispersive spectroscopy (EDS).     

Decomposition of P2S2N4(Si(CH3)3)4A12C14 as Studied by FT-Raman and Quantum Chemistry Means

The dimeric title compound decomposes upon heating to give the monomer and desulphurized monomer as shown by FT-Raman and quantum chemical means.     

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.