1000 resultados para Bi


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丙烷氧化反应中多组分氧化物Bi-V-Mo-O催化作用的红外光谱研究李静,宋伟,窦伯生(中国科学院长春应用化学研究所长春130022)关键词钼钒酸铋,丙烷,选择氧化,催化作用机理,红外光谱迄今对于含有钼、铋复合氧化物催化剂的活性中心和作用机理存在不同看...

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The structure and catalytic,activity for propylene oxidation of series oxides B2Mo3-3X-Nb2XO12-4X (X=0.00, 0.02, 0.05, 0.10, 0.15, 0.20, 0.25) have been studied by means of XRD, IR, Raman, SEM, ESR and so on. The results showed that in the range of X < 0.

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用ESR对比研究了掺杂Nb对α-Bi2Mo3O(12)催化剂丙烯还原和氧再氧化的影响,并用XPS原位Ar+溅射研究了催化剂的还原与再氧化过程,观察了上述过程中催化剂内金属离子的价态变化和晶格氧的扩散现象。提出了Bi-Mo间通过晶格氧扩散所发生的氧化还原作用及模型,探讨了Nb(5+)取代Mo(6+)产生的氧空位对加速晶格氧扩散所起的作用。

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采用常规固相反应于1200℃下制备了具有褐钇铌矿结构的Y2O3·Nb2O5·B2O3(Y(0.93)Eu(0.07))2O3·Nb2O5·B2O3和(Y(0.91)Eu(0.07)Bi0.02))2O3·Nb2O5·B2O3等光体,研究了它们的发光性质:结果表明,在268nm紫外光激发下,由于NbO4基团于410nm处发生1T→1A1跃迁,致使Y2O5·Nb2O5·B2O3呈现更亮的紫外发射。体系中的B2O3可降低反应温度,增强NbO4和Eu(3+)的发光强度。(Y(0.091)Eu(0.07)Bi(0.02))2O3·Nb2O5·B2O3燐光体系中所观察到的NbO4→Eu(3+)和Bi(3+)→Eu(3+)的能量传递使红光发射明显增强。

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本文用XRD,IR,Raman,SEM和ESR等方法研究了系列氧化物Bi_2Mo_(3-3x)Nb_(2x)O_(12-4x)(X=0.00,0.02,0.05,0.10,0.15,0.20,0.25)的结构和对丙烯氧化的催化活性,结果表明,在X≤0.25范围内,催化剂基本保持典型的α-Bi_2Mo_3O_(12)结构,少量Nb~(5+)的掺杂,可取代晶格中的Mo~(6+),产生氧空位,无序分布的氧空位的浓度先随X值的增加而增加,当X=0.15时达最大值,催化剂对丙烯氧化的催化活性与这种氧空位的浓度成正比,反应遵循Redox机理.

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以Mg(NO3)2、Ca(NO3)2、Eu(NO3)3、Bi(NO3)3、LiNO3和Si(OC2H5)4为反应物,采用溶胶-凝胶法,在比较低的温度下,首次合成0.701moIMgO-0.175molCaO-1.25moISiO2∶0.06molEu(3+),0.002moIBi(3+)(加入Li+作为电荷补偿剂)发光体。得到了最佳合成条件。研究了由溶胶向凝胶转变和凝胶向发光晶体的转变过程。探讨了发光体在不同激发波长激发下的发光特性以及在激活剂、敏化剂不同掺杂量下的发光行为。讨论了在(Mg(a)O-SiO2基质中Bi(3+)对Eu(3+)的能量传递和敏化作用。

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At room temperature, the Bi3+ ion shows broad band characters of its luminescence in Ca2B2O5, M3B2O6 ( M=Ca,Sr ) and SrB4O7. The maxima of the Bi3+ S-1(0)-->P-3(1) absorption bands are located in the range of 240-300nm, but the energy variation of the corresponding P-3(1)-->S-1(0) emissions is very large. The maxima of these emission bands change from 350nm in Ca3B2O6;Bi3+ to 586nm in SrB4O7:Bi3+. The Stokes shift of the Bi3+ luminescence increases from 6118 cm-1, in Ca2B2O5:Bi3+, to 24439 cm-1, in SrB4O7:Bi3+. The emission intensity of the Bi3+ luminescence increases with the decreasing Stokes shift. It has been found that in Ca2B2O5, the Bi3+ ion could transfer its excitation energy to the R3+ ions ( R=Eu, Dy, Sm, Tb ) , but in, Ca3B2O6 and Sr3B2O6, only Bi3+-->Eu3+ was observed. No energy transfer from Bi3+ to R3+ was detected in SrB4O7.

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本文报道了Eu~(3+)、D~(3+)在YV_(1-x)B_xO_(4-x)中的光谱性质。实验表明:B~(3+)取代V~(5+)时,可使基质和Dy~(3+)的发射强度及黄兰比下降,并使基质的吸收带短移。而B~(3+)取代Y~(3+)时,则可提高Dy~(3+)的黄兰比。同时我们还研究了Bi~(3+)和温度对YV_(0.69)B_(0.31)O_(3.69):Dy~(3+)中Dy~(3+)发射强度的影响。

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自Maeda发现高Tc超导体BiSrCaCuO以来,引起了人们广泛兴趣;由于它有较高的超导转变温度(Tc>100K),无剧毒、价廉和自高温冷却到室温无结构相变等特点,Bi系是一很有实用前景的高Tc超导体;已经确定Bi系中含有三个超导相(2201,2212,2223相),但是迄今要制得较纯的2223高Tc相还有一定困难,无疑这对它的基础研究和实用开发都受到了限制,因此制备更纯的Bi系2223相具有重要的意义。

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自发现BiSrCaCuO超导体以来,为了稳定2223高T_C相结构、增加其在超导体中的含量,在该体系中引入掺杂元素Pb被公认是最有效的方法。我们系统研究了V~(5+)、Nb~(5+)、Ta~(5+)高价离子的单独掺入Bi系中对

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已知在Bi系高Tc超导体中存在三个超导相:2223相的Tc~110k,c~37(?);2212相的Tc~85k,c~30.6(?);2201相的Tc~10k。在实验过程中,我们注意到还可能有另外的超导相存在,通过改变元素名义配比和制备工艺观察到一个具有2212相结构,但Tc却表现为~105k的新现象存在。 实验部分 样品制备采用固相反应方法将Bi_2O_3、PbO、Sb_2O_3、SrCO_3、CaCO_3、CuO(均为A.R.级)混匀、碾磨,于~810℃在刚玉坩埚中预烧20h;再碾,压片后于~870℃在磁舟中烧结60-240h,然后作测试分析。

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固相法合成系列名义组成为Bi_(2-x)Nb_xSr_2Ca_2Cu_3Oy(x=0—1.0)的样品,电学和磁学测量表明,当掺入x=0.2—0.3的Nb有明显加强2223相生成的作用,配比为Bi_(1.7)Nb_(0.3)Sr_2Ca_2Cu_3Oy时最佳;当掺Ba以部分取代Sr后有明显协同Nb促进22 23相生成的作用,比单掺Nb效果更为显著,其中以Bi_(1.7)Nb_(0.3)Sr_(1.8)Ba_(0.2)Ca_2Cu_3Oy为最优组成。热重分析(TGA)实验显示,掺Nb(Ba)后样品在~600°C出现吸氧增重;XPS中的O_(1s)峰显示掺Nb(Ba)后除~531eV的主峰外,在~529eV的肩峰更加明显;讨论了Nb(Ba)对晶体结构的可能影响。

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本文报导了Eu~(3+),Dy~(3+)在Ba_2RV_3O_(11)(R=Y,Gd,La)基质中的光谱性质、Bi~(3+)对Dy~(3+)发射强度的影响及温度对Dy~(3+)发射强度的猝灭情况.研究了被取代离子R~(3+)(R=Y,Gd,La)对基质电行迁移带、Eu~(3+)的红橙比、Dy~(3+)黄蓝比的影响,还给出了Dy~(3+)的浓度猝灭值.

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