卟啉锡敏化TiO2纳米管的光催化活性和光电性能

制备了反-二羟基-5,10,15,10-四苯基卟啉锡敏化的TiO₂纳米管,并以对硝基苯酚为模型污染物,对其在可见光照射下的光催化活性进行了研究。同时,将卟啉锡敏化的TiO₂纳米粒子作为参照物,探讨了形貌对催化剂光催化活性的影响。实验结果表明,卟啉锡的引入可以明显地增强TiO₂纳米管的可见光催化活性。与TiO₂纳米粒子相比,卟啉锡对TiO₂纳米管的敏化作用更加显著,表明催化剂的形貌在光催化过程中具有重要作用。此外,我们还考察了卟啉锡敏化的TiO₂纳米管的光电化学行为,并与其光催化活性相关联。最后,对卟啉锡的敏化机理进行了初步的探讨。     

CdS/TiO2纳米管复合结构的制备与光电性能研究

利用阳极氧化法在钛金属基底表面制备一层TiO2纳米管阵列薄膜,然后通过水热反应在TiO2纳米管上负载CdS纳米粒子,形成CdS/TiO2纳米管的复合结构。利用SEM、XRD、XPS、UV-Vis等手段对其形貌和结构进行表征。进一步考察了CdS/TiO2纳米管的光电性能和光催化活性,结果表明,相比于TiO2纳米管,CdS/TiO2纳米管复合结构在紫外光和可见光下都具有更好的光催化活性及光电性能。     

Fe、N共掺杂TiO2纳米管阵列的制备及可见光光催化活性

应用电化学阳极氧化法结合浸渍和退火后处理制备了Fe和N共掺杂的TiO2纳米管阵列光催化剂,并用场发射扫描电镜(FESEM)、X射线衍射(XRD)、X射线光电子能谱(XPS)和俄歇电子能谱(AES)仪对其进行了表征.结果表明,Fe、N共掺杂对TiO2纳米管阵列的形貌和结构没有明显影响,Fe和N均掺入了TiO2晶格.紫外-可见(UV-Vis)漫反射光谱显示Fe和N共掺杂TiO2纳米管阵列的吸收带边较纯TiO2纳米管阵列和单一掺杂TiO2纳米管阵列红移,可见光吸收增强.以可见光催化降解罗丹明B(RhB)考察了材料的光催化活性,Fe和N共掺杂TiO2纳米管阵列对RhB的降解速率较纯TiO2纳米管阵列和单一掺杂TiO2纳米管阵列明显提高,证明了Fe、N共掺杂产生的协同效应提高了TiO2纳米管阵列在可见光照射下的光催化活性.     

卟啉敏化二氧化钛复合微球的制备及其光催化性能

采用溶胶-凝胶法制备了5-(对-烯丙氧基)苯基-10,15,20-三对氯苯基卟啉(APTCPP)敏化的TiO2复合微球APTCPP-MPS-TiO2.运用紫外-可见光漫反射吸收光谱、热重分析、X射线衍射、光电子能谱和扫描电镜等手段对TiO2复合微球进行了表征.考察了复合微球在可见光照射下对α-松油烯的光催化氧化活性.结果表明,复合微球中TiO2主要以锐钛矿晶型存在,微球粒径约为0.7～1 μm.卟啉的加入有效提高了TiO2复合微球对α-松油烯的光催化活性,催化氧化产物主要是土荆芥油素.     

掺杂Cu的TiO2纳米粒子的制备、表征及其光催化活性

采用Sol-gel法制备了纯的和掺杂不同量Cu的TiO2纳米粒子,并用TG-DTA,XRD,XPS,UV-Vis和荧光光谱对样品进行了表征,考察焙烧温度和Cu含量对TiO2纳米粒子的性质及光催化活性的影响,初步探讨了Cu的掺杂对TiO2相变的作用机制及样品荧光光谱与光催化活性的关系.结果表明,Cu2+的掺杂对TiO2的相变有很大的促进作用,并使其光谱响应范围向可见光区拓展.Cu的掺杂未引起新的荧光现象,但适量Cu的掺杂能够降低TiO2纳米粒子的荧光强度.此外,在光催化降解苯酚的实验中,于500℃处理的掺杂Cu的TiO2纳米粒子的光催化活性较高,与表征结果一致.而掺杂不同量Cu的TiO2的光催化活性顺序与样品荧光光谱强度的顺序相反,即荧光光谱强度越低,其光催化活性越高.     

(Ni-Mo)/TiO2纳米薄膜光催化降解刚果红的性能与机理

用恒电流复合电沉积方法制备(Ni-Mo)/TiO2薄膜,以扫描电子显微镜(SEM)、X射线衍射(XRD)、拉曼(Raman)光谱和紫外-可见漫反射光谱(UV-VisDRS)对薄膜的表面形貌、晶相结构和光谱特性进行了表征,以刚果红为模拟污染物对薄膜的光催化性能进行了测定,并讨论了刚果红溶液的pH值对薄膜光催化活性的影响.采用循环伏安技术和向溶液中加入活性物种捕获剂的方法对薄膜光催化降解机理进行了探索.结果表明:(Ni-Mo)/TiO2薄膜是由粒径为50-100nmTiO2纳米粒子相和纳米晶Ni-Mo固溶体相构成的复合薄膜.薄膜具有较高的光催化活性,卤钨灯照射80min后,复合薄膜光催化刚果红的降解率是多孔TiO2(DegussaP25)/ITO(氧化铟锡)纳米薄膜的2.43倍.(Ni-Mo)/TiO2薄膜光催化活性的提高主要归因于薄膜层中有效形成的(Ni-Mo)/TiO2异质结和良好的电子通道,以及Ni-Mo纳米晶合金对溶解氧和激发电子还原反应的催化作用.分别给出了在紫外和可见光下薄膜光催化降解刚果红的反应机理.     

铜卟啉-TiO_2复合光催化剂制备及降解4-NP的研究

合成了取代基数目不同的3种铜卟啉配合物,并与纯锐钛矿型TiO2作用,得到相应的铜卟啉敏化TiO2复合光催化剂.采用扫描电子显微镜(SEM)考察了铜卟啉-TiO2复合光催化剂的形貌特征,紫外-可见光谱和X射线衍射(XRD)分析结果表明,铜卟啉负载于TiO2表面,未改变TiO2的晶型.可见光降解4-硝基苯酚(4-NP)实验结果表明,复合催化剂性质稳定,可多次重复使用,卟啉环外围极性取代基数目越多,铜卟啉光敏化效果越好.     

Ag／TiO2复合纳米催化剂的制备和表征及其光催化活性

 采用光还原沉积贵金属法，制备了Ag／TiO2复合纳米催化剂．通过调节溶液的pH值控制TiO2表面负载银的形貌，利用AAS，XRD，TEM和XPS等手段对样品进行了表征．以苯胺氧化为模型反应，考察了Ag／TiO2复合纳米催化剂样品的光催化活性以及银沉积量和沉积形貌对催化剂活性的影响．结果表明，通过调控光还原沉积条件，可在平均粒径为24nm左右的TiO2颗粒上获得3nm左右均匀分散的银粒子；在TiO2上沉积适量的具有较高分散度的金属Ag，能有效提高TiO2对苯胺氧化反应的光催化活性．     

用TiO2，ZnO及Fe2O3纳米粒子光催化氧化庚烷的反应

 制备了三种n－型半导体氧化物TiO2，ZnO和Fe2O3纳米粒子，用X射线衍射和N2吸附技术分别对它们的结构及比表面积进行了表征．考察了三种氧化物粒子对庚烷的气相光催化氧化反应的催化活性．研究表明，对于同种催化剂，随着焙烧温度的升高，催化剂的粒径增大，比表 面积减小，光催化活性下降．三种催化剂纳米粒子的光催化活性顺序为TiO2（锐钛矿）＞ZnO＞Fe2O3，金红石型TiO2粒子的催化活性低于ZnO粒子．结合能带理论探讨了三种催化剂光催化活性差异的原因．     

一步低温法制备可见光响应的棕色纳米TiO2及其光催化性能

光催化作为一种具有前景的技术,被广泛运用于有机物降解、废水处理、空气净化、抗菌、太阳能电池等领域.在众多的光催化材料中,纳米TiO2因具有性质稳定、耐腐蚀、廉价和无毒等优点而受到广泛关注.但纳米TiO2禁带宽度较大(3.2 eV)、只对紫外光有响应及电子-空穴对易复合等特性限制了它的应用.因此,提高纳米TiO2的可见光响应一直是研究的热点.本文发展了一种在低温下制备棕色纳米TiO2的改良溶胶-凝胶法.该法以钛酸四丁酯为钛源,无水乙醇为溶剂,形成溶胶后无需陈化和高温高压,在简单温和的条件下即可制备出棕色纳米TiO2.比较了低温干燥和高温焙烧两种处理方法,结果表明,随着制备温度的升高,样品的粒子尺寸增大,比表面积减小,颜色从白色转变为棕色,在更高的温度又变浅.样品的可见光吸收在180℃时达到最大,随后减弱.在优化温度180℃下制备的TiO2-180℃纳米粒子不仅具有较小的粒径(5.0 nm),较大的比表面积(213.45 m2/g),且在整个紫外-可见光区都具有较强的吸收,其禁带宽度低至1.84 eV.X-射线光电子能谱结果表明,TiO2粒子表面的–OH/H2O含量随制备温度升高而先增加后下降.Raman光谱中Eg峰的移动和变宽表明TiO2晶格可能存在缺陷或氧空位,而TiO2-180℃纳米粒子的电子顺磁共振图谱的g值在2.003左右,对应氧空位中的未成对电子,验证了以上推测.其中TiO2-180℃纳米粒子呈现为最强的EPR信号,表明其晶格内存在最高浓度的氧空位,这是其具有强可见光吸收的原因.光催化实验结果表明,在可见光照射下,TiO2-180℃可高效降解亚甲基蓝(MB).当C(MB)=10 mg/L,pH=4,催化剂添加量为0.07 g时,TiO2-180℃催化剂的光催化活性达到最佳,光照1 h后MB降解率达到99.33%,反应速率常数(0.08287 mg/(L·min))约为同条件下P25(0.01342 mg/(L·min))的6倍.同时,TiO2-180℃催化剂在不同单色光下的光催化活性与它对单色光的光响应大致相符.循环降解实验证明TiO2-180℃催化剂具有很好的稳定性.光猝灭实验表明,·OH在光催化降解过程占主导作用,而TiO2-180℃样品表面含有较多的–OH,有利于·OH的产生,乃至光催化反应.研究表明,晶格内高浓度的氧空位导致的强可见光响应,得益于低温制备条件而保留了大量–OH/H2O的纳米粒子表面以及更大的比表面积,共同促成了TiO2-180℃优越的光催化活性.所制备的棕色纳米TiO2经过进一步修饰后有望运用于实际应用中.     

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.     

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.     

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。     

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.     

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 Phase Relations in the System In2O3–TiO2–MgO at 1100 and 1350°C

The phase relations in the system In₂O₃–TiO₂–MgO at 1100 and 1350°C are determined by a classical quenching method. In this system, there are four pseudobinary compounds, In₂TiO₅, MgTi₂O₅ (pseudobrookite type), MgTiO₃ (ilmenite type), and Mg₂TiO₄ (spinel type) at 1100°C. At 1350°C, in addition to these compounds there exist a spinel-type solid solution Mg_2−xIn_2xTi_1−xO₄ (0≤x≤1) and a compound In₆Ti₆MgO₂₂ with lattice constants a=5.9236(7) Å, b=3.3862(4) Å, c=6.3609(7) Å, β=108.15(1)°, and q=0.369, which is isostructural with the monoclinic In₃Ti₂FeO₁₀ in the system In₂O₃–TiO₂–MgO. The relation between the lattice constants of the spinel phase and the composition nearly satisfies Vegard's law. In₆Ti₆MgO₂₂ extends a solid solution range to In₂₀Ti₁₇Mg₃O₆₇ with lattice constants of a=5.9230(5) Å, b=3.3823(3) Å, c=6.3698(6) Å, β=108.10(5)°, and q=0.360. The distributions of constituent cations in the solid solutions are discussed in terms of their ionic radius and site preference effect.     

Microstructures of Some Bi-W-Nb-O Phases

Microstructures of three Bi-W-Nb-O phases have been examined by using high-resolution transmission electron microscopy. Bi₁₇W₂Nb₃O₃₉ and Bi₁₇WNb₃O₃₆ have incommensurate superstructures derived from the defect fluorite-type δ-Bi₂O₃ and can be regarded as intermediate phases between the type II solid solutions in the Bi-Nb-O and Bi-W-O systems. Bi₈W₂Nb₂O₂₃ has a Bi₂WO₆-like subunit cell with a stepped superstructure. Formation mechanisms of various superstructures are discussed.     

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.