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1.
采用碳布(CC)为柔性基底,通过水热法制备了MnO2/CC及N掺杂MnO2/CC无黏结剂负极材料,借助X射线衍射(XRD)、扫描电镜(SEM)、X射线光电子能谱(XPS)、比表面积测试和恒电流充放电对材料进行了结构表征及电化学性能测试。结果表明N掺杂MnO2/CC具有良好的倍率性能和循环稳定性。在0.1 A·g-1的电流密度下,其首次充电比容量为948.8 mAh·g-1,经过不同倍率测试后电流密度恢复至0.1 A·g-1时仍然保持有907.9 mAh·g-1的可逆比容量,容量保持率为95.7%。在1 A·g-1的大电流密度下,其首次充电比容量为640.3 mAh·g-1,循环100次后仍然保持有529.9 mAh·g-1的可逆比容量,容量保持率为82.8%,可逆比容量远高于商用MnO2。  相似文献   

2.
为探索一种高性能的锂离子电池负极材料,采用酸刻蚀法制备了高导电性、高稳定性的二维层状Ti3C2Tx,通过溶剂热法制备了具有高理论比容量的花瓣状VS2纳米片,再经过简单的液相混合得到了二维层状Ti3C2Tx-MXene@VS2复合物。通过扫描电子显微镜、透射电子显微镜、X射线光电子能谱、X射线衍射和能谱分析对复合材料的形貌和结构进行了表征,采用循环伏安、恒流充放电、长循环和交流阻抗谱对复合材料的电化学性能进行了研究。结果表明:VS2纳米片均匀地分布在Ti3C2Tx的层间及表面,该复合物具有高的可逆容量(电流密度为0.1A·g-1时,比容量为610.5mAh·g-1)、良好的倍率性能(电流密度为2A·g-1时,比容量为197.1mAh·g-1)和良好的循环稳定性(电流密度为0.2 A·g-1时,循环600圈后比容量为874.9 mAh·g-1;电流密度为2 A·g-1时,循环1 500圈后比容量为115.9mAh·g-1)。  相似文献   

3.
通过液相共沉淀法获得Zn和Co的前驱,经过600℃煅烧处理获得ZnCo2O4纳米颗粒组装的毛线团状的微球。电化学测试表明,在0.5 A·g-1的电流密度下循环200次可逆比容量保持为965 mAh·g-1;在0.8 A·g-1的电流密度下循环350次可逆比容量保持为882 mAh·g-1。倍率性能测试表明在2 A·g-1的电流密度时可逆比容量为736 mAh·g-1。  相似文献   

4.
王瑛  林宁 《无机化学学报》2016,32(12):2191-2197
通过液相共沉淀法获得Zn和Co的前驱,经过600℃煅烧处理获得ZnCo2O4纳米颗粒组装的毛线团状的微球。电化学测试表明,在0.5 A·g-1的电流密度下循环200次可逆比容量保持为965 mAh·g-1;在0.8 A·g-1的电流密度下循环350次可逆比容量保持为882 mAh·g-1。倍率性能测试表明在2 A·g-1的电流密度时可逆比容量为736 mAh·g-1。  相似文献   

5.
以(CH2OH)2、NH4F和HCl为电解液,纯Ti片、CuCl2和NaNO3为主要原料,联用阳极氧化和水热法制备CuO表面修饰锐钛矿TiO2纳米管阵列锂离子电池负极材料(CuO/TiO2)。使用扫描电子显微镜(SEM)、透射电子显微镜(TEM)、能谱仪(EDS)、X射线光电子能谱仪(XPS)和X射线衍射(XRD),研究样品的形貌特征、元素分布、价态和微观物相组成。利用电池充放电测试仪和电化学工作站,探讨材料的电化学嵌锂性能。结果表明,表面修饰后的锐钛矿TiO2纳米管阵列外侧出现了大量绒毛状纳米CuO,单个绒毛结构的宽度约4 nm,长度约10 nm。在0.3C的电流密度下进行恒电流充放电测试,首次放电容量为550 mAh·g-1,充电容量为490 mAh·g-1。50次循环后,可逆电流容量仍保持在320 mAh·g-1,具有良好的循环稳定性和电化学特性。  相似文献   

6.
采用水基流变相辅助的固相法,以异质碳蔗糖和石墨为碳源,合成了LiMn0.8Fe0.2PO4/C复合材料,研究了不同石墨加入方式对所制复合材料电化学性能的影响,并对所制备的LiMn0.8Fe0.2PO4/C复合材料进行了X射线衍射(XRD)、比表面积测试、扫描电子显微镜(SEM)、透射电子显微镜(TEM)等表征。结果表明,不同石墨包覆工艺对材料结构和电化学性能具有显著影响。前驱体煅烧后再加入石墨获得的样品纯度高,形貌呈均一的椭圆形,在0.1C下的放电比容量为149 mAh·g-1,达到其理论比容量的 87%;在 5C 下最大的放电比容量为 133 mAh·g-1;在 2C 倍率下经过 300 次循环后比容量维持在 127 mAh·g-1,衰减率仅为1.9%,表现出了优良的循环稳定性。  相似文献   

7.
首先采用共沉淀方法制备富锂锰基正极材料Li1.2Mn0.54Ni0.13Co0.13O2原始样品(P-LRMO),然后通过简单的湿化学法以及低温煅烧方法对其进行不同含量Ga2O3原位包覆。透射电子显微镜(TEM)以及X射线光电子能谱(XPS)结果表明在P-LRMO表面成功合成了Ga2O3包覆层。电化学测试结果表明:含有3%Ga2O3的改性材料G3-LRMO具有最优的电化学性能,其在0.1C倍率(电流密度为25 mA·g-1)下首圈充放电比容量可以达到270.1 mAh·g-1,在5C倍率下容量仍能保持127.4 mAh·g-1,优于未改性材料的90.7 mAh·g-1,表现出优异的倍率性能。G3-LRMO在1C倍率下循环200圈后仍有190.7 mAh·g-1的容量,容量保持率由未改性前的72.9%提升至85.6%,证明Ga2O3包覆改性能有效提升富锂锰基材料的循环稳定性。并且,G3-LRMO在1C倍率下循环100圈后,电荷转移阻抗(Rct)为107.7 Ω,远低于未改性材料的251.5 Ω,表明Ga2O3包覆层能提高材料的电子传输速率。  相似文献   

8.
分别以四水磷酸铁(FePO4·4H2O)和二水草酸亚铁(FeC2O4·2H2O)为铁源,采用简单便捷的流变相法制备了碳包覆LiFe0.5Co0.5PO4固溶体材料(LiFe0.5Co0.5PO4/C,简称为LFCP/C)。采用X射线衍射(XRD)、扫描电镜(SEM)、透射电镜(TEM)、恒流充放电等测试手段对复合材料的物相、形貌结构和电化学性能进行了表征和测试。结果表明,2种铁源得到的材料均为橄榄石晶型结构且结晶度良好,二者在颗粒尺寸分布、碳包覆效果和电化学性能方面具有显著的差别。用作锂离子电池正极材料时,以FeC2O4·2H2O为原料得到的LFCP/C具有更优异的电性能:在2.5~5.0 V电压范围内,0.1C倍率下(1C=150 mA·g-1),放电比容量为137.5 mAh·g-1,在10C仍具有57.6 mAh·g-1的放电比容量;0.5C循环100次后容量仍保持78.1%。该样品更佳的电化学性能主要得益于其更小的平均颗粒尺寸,更高的比表面积和理想的碳包覆效果。  相似文献   

9.
首先采用共沉淀方法制备富锂锰基正极材料 Li1.2Mn0.54Ni0.13Co0.13O2原始样品(P-LRMO), 然后通过简单的湿化学法以及低温煅烧方法对其进行不同含量 Ga2O3原位包覆。透射电子显微镜(TEM)以及 X射线光电子能谱(XPS)结果表明在 P-LRMO表面成功合成了 Ga2O3包覆层。电化学测试结果表明:含有 3 %Ga2O3的改性材料 G3-LRMO具有最优的电化学性能, 其在 0.1C倍率(电流密度为 25 mA·g-1)下首圈充放电比容量可以达到 270.1 mAh·g-1, 在 5C倍率下容量仍能保持 127.4 mAh·g-1, 优于未改性材料的 90.7 mAh·g-1, 表现出优异的倍率性能。G3-LRMO在 1C倍率下循环 200圈后仍有 190.7 mAh·g-1的容量, 容量保持率由未改性前的 72.9 %提升至 85.6 %, 证明 Ga2O3包覆改性能有效提升富锂锰基材料的循环稳定性。并且, G3-LRMO在 1C倍率下循环 100圈后, 电荷转移阻抗(Rct)为 107.7 Ω, 远低于未改性材料的 251.5 Ω, 表明 Ga2O3包覆层能提高材料的电子传输速率。  相似文献   

10.
以乙二胺四乙酸(EDTA)为配位剂,采用溶胶凝胶和溶剂热法相结合的方法合成了Li2MnSiO4/C纳米复合正极材料。经过EDTA配位的锂锰硅前驱体在氩气中经过700℃煅烧后,产生为颗粒尺寸约为50nm的Li2MnSiO4/C纳米复合粉体。在0.1C=33mA·g-1进行充放电测试时,其首次充电和放电比容量分别为223和140mAh·g-1,第5次循环放电比容量仍为138mAh·g-1;电流密度升至0.2C=66mA·g-1时,在第20次循环的放电比容量仍可稳定在80mAh·g-1左右。这些结果表明,EDTA的配位作用可抑制杂相的形成,这种分散性相对较好的纳米复合粉体Li2MnSiO4正极材料表现出提高的循环稳定性。  相似文献   

11.
娄太平  张乐  郭军兴 《化学学报》2010,68(6):466-470
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.  相似文献   

12.
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.  相似文献   

13.
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.  相似文献   

14.
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.  相似文献   

15.
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。  相似文献   

16.
The crystal structures of compounds with nominal compositions Bi6FeP2O15+x (I), Bi6NiP2O15+x (II) and Bi6ZnP2O15+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, μeff=6.1 μB; a magnetic transition occurs above 250 K.  相似文献   

17.
Tao Lin  Wei Li  Maochu Gong  Yao Yu  Bo Du  Yaoqiang Chen   《Acta Physico》2007,23(12):1851-1856
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.  相似文献   

18.
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 Mg2−xIn2xTi1−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.  相似文献   

19.
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.  相似文献   

20.
The crystal structures of Bi2.5Na0.5Ta2O9 and Bi2.5Nam-1.5NbmO3m+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 (Am-1BmO3m+1)2- (m=2-4) pseudo-perovskite slabs. Bi2.5Na0.5Ta2O9 (m=2) and Bi2.5Na2.5Nb4O15 (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. Bi2.5Na1.5Nb3O12 (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 Bi2.5Na0.5Ta2O9 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 Bi2.5Nam-1.5NbmO3m+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.  相似文献   

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