Crystallographic and magnetic properties of hydride R3Fe29-xTxHy (R=Y, Ce, Nd, Sm, Gd, Tb and Dy; T=V and Cr)

The crystallographic and intrinsic magnetic properties of hydride R3Fe29-xTxHy (R=Y, Ce, Nd, Sm, Gd, Tb, and Dy; T=V and Cr) have been investigated. The lattice constants and the unit cell volume of R3Fe29-xTxHy decrease with increasing R atomic number from Nd to Dy, except for Ce, reflecting the lanthanide contraction. Regular anisotropic expansions, mainly along the a- and b-axis rather than along the c-axis, are observed for all the compounds upon hydrogenation. Hydrogenation leads to an increase in Curie temperature. First-order magnetization processes (FOMP) occur in magnetic fields of around 1.5 T and 4.0 T at 4.2 K for Nd3Fe24.5Cr4.5H5.0 and Tb(3)Fc(27.0)Cr(2.0)H(2.8), and around 1.4 T at room temperature for Gd3Fe28.0Cr1.0H4.2 Abnormal crystallographic and magnetic properties of Ce3Fe29-xTxHy suggest that the Ce ion is non-triply ionized.

Pressure behavior of deep centers in ZnSxTe1-x alloys

We have measured photoluminescence of ZnSxTe1-x alloys (x > 0.7) at 300 K and under hydrostatic pressure up to 7 GPa. The spectra contain only a broad emission band under excitation of the 406.7 nm line. Its pressure coefficients are 47, 62 and 45 meV/GPa for x = 0.98, 0.92 and 0.79 samples, which are about 26%, 7% and 38% smaller than that of the band gap in the corresponding alloys. The Stokes shifts between emission and absorption of the bands were calculated by fitting the pressure dependence of the emission intensity, being 0.29, 0.48 and 0.13 eV for the three samples, respectively. The small pressure coefficient and large Stokes shift indicate that the emission band observed in our samples may correspond to the Te isoelectronic center in the ZnSxTe1-x alloy.

Hydrogenation and anisotropic expansions in R3Fe29-xTx (R = Y, Ce, Nd, Sm, Gd, Tb and Dy; T = V and Cr)

A systematic study of the phase formation, structure and magnetic properties of the R3Fe29-xTx compounds (R=Y, Ce, Nd, Sm, Gd, Tb, and Dy; T=V and Cr) has been performed upon hydrogenation. The lattice constants and the unit cell volume of R3Fe29-xTxHy decrease with increasing R atomic number from Nd to Dy, except for Ce, reflecting the lanthanide contraction. Regular anisotropic expansions mainly along the a- and b-axis rather than along the c-axis are observed for all of the compounds upon hydrogenation. Hydrogenation leads to an increase in the Curie temperature and a corresponding increase in the saturation magnetization at room temperature for each compound. First order magnetization processes (FOMP) occur in the external magnetic fields for Nd3Fe24.5Cr4.5H5.0, Tb3Fe27.0Cr2.0H2.8, and Gd3Fe28.0Cr1.0H4.2 compounds.

Structural and magnetic properties of hydrides R3Fe29-xVxHy (R = Y, Ce, Nd, Sm, Gd, Tb, and Dy)

A systematic investigation of crystallographic and intrinsic magnetic properties of the hydrides R3Fe29 - xVxHy (R = Y, Ce, Nd, Sm, Gd, Tb, and Dy) has been performed in this work. The lattice constants a, b, and c and the unit cell volume of R3Fe29 - xVxHy decrease with increasing rare-earth atomic number from Nd to Dy, except for Ce, reflecting the lanthanide contraction. Hydrogenation results in regular anisotropic expansions along the a-, b-, and c-axes in this series of hydrides. Abnormal crystallographic and magnetic properties of Ce3Fe27.5V1.5H6.5, like Ce3Fe27.5V1.5, suggest that the Ce ion is non-triply ionized. Hydrogenation leads to the increase in both Curie temperature for all the compounds and in the saturation magnetization at 4.2 K and RT for R3Fe29 - xVx with R = Y, Ce, Nd, Sm, Gd, and Dy, except for Tb. Hydrogenation also leads to a decrease in the anisotropy field at 4.2 K and RT for R3Fe29 - xVx with R = Y, Ce, Nd, Gd, Tb, and Dy, except for Sm. The Ce3Fe27.5V1.5 and Gd3Fe28.4V0.6 show the larger storage of hydrogen with y = 6.5 and 6.9 in these hydrides. (C) 1998 Elsevier Science B.V. All rights reserved.

Hole trap levels in Mg-doped GaN grown by metalorganic vapor phase epitaxy

Hole trap levels in a Mg-doped GaN grown by metalorganic vapor phase epitaxy (MOVPE) are studied with deep level transient spectroscopy (DLTS). The Mg concentration of the sample was 4.8 x 10(19) cm(-3), but the hole concentration was as low as 1.3 x 10(17) cm(-3) at room temperature. The DLTS spectrum has a dominant peak D-1 with activation energy of 0.41+/-0.05 eV, accompanied by two additional peaks with activation energies of 0.49+/-0.09 eV (D-2) and 0.59+/-0.05 eV (D-3). It was found that the dominant peak D-1 consists of five peaks, each of which has different activation energy and capture cross section. A relevant model for these levels is presented in relation to the Mg-N-H complexes. (C) 1998 American Institute of Physics. [S0003-6951(98)04340-X].

Crystallographic and magnetic properties of the hydrides R3Fe29-xCrxHy (R = Y, Ce, Nd, Sm, Gd, Tb, and Dy)

A systematic study of the structural and intrinsic magnetic properties of the hydrides R3Fe29-xCrxHy (R = Y, Ce, Nd, Sm, Gd, Tb, and Dy) has been performed. Hydrogenation lends to a relative volume expansion of the unit cell and a decrease in x-ray density for each compound. Anisotropic expansions mainly along the n- and b-axes rather than along the c-axis for all of the compounds upon hydrogenation are observed. The lattice constants and the unit-cell volume of R3Fe29-xCrx and R3Fe29-xCrxHy decrease with increasing R atomic number from Nd to Dy, except for Ce, reflecting the lanthanide contraction. Hydrogenation results in an increase in the Curie temperature and a corresponding increase in the saturation magnetization at room temperature for each compound. After hydrogenation a decrease of 0.34 mu(B)/Fe in the average Fe atomic magnetic moment and a slight increase in the anisotropy field for Y3Fe27.2Cr1.8 are achieved at 4.2 K. First-order magnetization processes (FOMP) occur in magnetic fields of around 1.5 T and 4.0 T at 4.2 K for Nd3Fe24.5Cr4.5H5.0 and TD3Fe27.0Cr2.0H2.8, and around 1.4 T at room temperature for Gd3Fe28.0Cr1.0H4.2. The abnormal crystallographic and magnetic properties of Ce3Fe25.0Cr4.0 and Ce3Fe25.0Cr4.0H5.4 suggest that the Ce ion non-triply ionized.

Raman scattering from In1-x-yGaxAlyAs quaternary alloys

Raman scattering studies were reported of In1-x-yGaxAlyAs/InP lattice matched quaternary alloys. The quaternary alloys a.ere grown on (100) oriented InP substrates by MBE method. The composition and intensity dependence of optical phonon mode frequencies show that the quaternary alloys exhibit three-mode behavior, i.e. InAs-like, GaAs-like and AlAs-like modes. Polarization analysis of the Raman spectra shows that the LO phonon modes are Raman active in the depolarized configuration and Raman inactive in the polarized configuration. TO phonon modes were also observed due to disorder effects, resulting in the asymmetrical shapes of the Raman peaks of the optical phonons.

Crystallographic and magnetic properties of nitride R3Fe29-xCrxN4 (R = Y, Ca, Nd, Sm, Gd, Tb, and Dy)

A systematic investigation of crystallographic and magnetic properties of nitride R3Fe29-xCrxN4 (R=Y, Ce, Nd, Sm, Gd, Tb, and Dy) has been performed. The lattice constants and unit cell volume decrease with increasing rare earth atomic number from Nd to Dy, reflecting the lanthanide contraction. After nitrogenation the relative volume expansion of each nitride is around between 5% and 7%. The nitrogenation results in a good improvement in the Curie temperature, the saturation magnetization and anisotropy fields at 4.2 K, and room temperature for R3Fe29-xCrxN4. Magnetohistory effects of R3Fe29-xCrxN4 and R3Fe29-xCrx (R=Nd and Sm) are observed in a low field of 0.04 T. First order magnetization process occurs in Sm3Fe24.0Cr5.0N4 in magnetic fields of 2.8 T at 4.2 K. After nitrogenation, the easy magnetization direction of Sm3Fe24.0Cr5.0 is changed from the easy-cone structure to the uniaxial. The good intrinsic magnetic properties of Sm3Fe24.0Cr5.0N4 make this compound a hopeful candidate for new high-performance hard magnets. (C) 1998 American Institute of Physics.

Crystallographic and magnetic properties of R3Fe29-xVxN4 (R = Y, Ce, Nd, Sm, Gd, Tb, and Dy)

A systematic investigation of crystallographic and magnetic properties of nitride R3Fe29-xVxN4 (R = Y, Ce, Nd, Sm, Gd, Tb, and Dy) has been performed. Nitrogenation leads to a relative volume expansion of about 6%. The lattice constants and unit cell volume decrease with increasing rare-earth atomic number from Nd to Dy, reflecting the lanthanide contraction. On average, the Curie temperature increases due to the nitrogenation to about 200 K compared with its parent compound. Generally speaking, nitrogenation also results in a remarkable improvement of the saturation magnetization and anisotropy fields at 4.2 K and room temperature for R3Fe29-xVxN4 compared with their parent compounds. The transition temperature indicates the spin reorientations of R3Fe29-xVxN4 for R = Nd and Sm are at around 375 and 370 K which are higher than that of R3Fe29-xVx, for R = Nd and Sm 145 and 140 K, respectively. The magnetohistory effects of R3Fe29-xVxN4 (R = Ce, Nd, and Sm) are observed in low fields of 0.04 T. After nitrogenation the easy magnetization direction of Sm3Fe26.7V2.3 is changed from an easy-cone structure to the b-axis. As a preliminary result, a maximum remanence B-r of 0.94 T, an intrinsic coercivity mu(0)H(C) of 0.75 T, and a maximum energy product (B H)(max) of 108.5 kJ m(-3) for the nitride magnet Sm3Fe26.7V2.3N4 are achieved by ball-milling at 293 K.

Growth and characterization of InAsSb alloys by metalorganic chemical vapour deposition

Low pressure metalorganic chemical vapour deposition (LP-MOCVD) growth and characteristics of InAssb on (100) Gasb substrates are investigated. Mirror-like surfaces with a minimum lattice mismatch are obtained. The samples are studied by photoluminescence spectra, and the output is 3.17 mu m in wavelength. The surface of InAssb epilayer shows that its morphological feature is dependent on buffer layer. With an InAs buffer layer used, the best surface is obtained. The InAssb film shows to be of n-type conduction with an electron concentration of 8.52 x 10(16) cm(-3).

含钇的耐热稀土镁合金的结构和性能研究

耐热、高强和抗高温蠕变的稀土镁合金是镁合金研究与开发的重要研究课题之一。本论文主要集中于对Y和其它稀土元素复合加入镁后的镁合金结构和性能的研究。探讨了Y与其它重稀土元素如Gd、Ho复合加入镁后的镁合金的时效硬化行为和结构性能，也研究了Y与混合轻稀土金属如富铈、富镧复合加入镁后对镁合金性能的影响。还对新型Mg-Y压铸镁合金的开发为目标，探讨了这一新型合金开发的可行性。具体结果如下： 1. 研究了Y加入到Mg-10Gd-0.4Zr合金中对合金的时效硬化和性能的影响规律和Mg-10Gd-6Y-0.4Zr合金在225℃和250℃时效210h内的沉淀析出相的转变以及合金的时效硬化行为。随着Y含量的增加，合金的时效硬化反应显著增强，合金的高温拉伸强度随Y含量的增加而线性增强，其原因是合金中的β'相有好的热稳定性。 2. 研究了Y和Ho元素复合加入镁后镁合金的时效硬化反应和组织性能。研究发现，在250℃时效时，当Y和Ho元素复合加入镁后，合金固溶体的时效分解速度加快，促进了合金的时效硬化，并且，随着Y含量的增加，合金的时效硬化反应增强，力学性能也相应提高。β-Mg24Y(Ho)5和（或）β'相对合金的时效硬化起了主要的作用，而且，位错密度增加也是合金性能提高的重要原因。 3. 探讨了Y和混合轻稀土富铈（和富镧）复合加入镁后对镁合金的性能影响。富铈和富镧在镁中低的固溶度导致单独加入镁后的时效硬化反应很弱，当Y和混合轻稀土富铈（和富镧）复合加入后，合金的时效硬化反应明显增强，并随着Y含量的增加，时效硬化的反应也相应增强。富铈和富镧对Mg-Y合金固溶体的时效分解有明显的促进作用。除了基体中的沉淀强化外，仍然停留在晶界上的Mg12RE稀土相对合金的晶界也有明显的强化作用。 4. 研究开发了具有良好的力学性能和高温抗蠕变性能、低含量Y、Gd的稀土镁合金，实验结果表明该合金是一种有良好应用前景的压铸镁合金。

镁-锌-稀土系合金的组织和性能研究

　　制备了Mg-4.5wt%Zn-1～5wt%RE系合金（RE元素包括轻稀土：La、Ce、Nd、Sm；重稀土：Gd和Y），研究了铸态和热处理态合金的组织和性能。（1）适量的稀土元素均可细化合金晶粒，其中轻稀土元素的细化效果好于重稀土元素；（2）含轻稀土元素合金中的析出相主要为(Mg,Zn)17RE2和Mg4Zn7，而含重稀土元素的合金中的析出相主要为MgZnxREy(Mg3Zn6RE, Mg3RE2Zn3)和Mg4Zn7；（3）加入稀土元素后，合金的强度提高；稀土含量相同时，含轻稀土元素的强化效果较好。Mg-4.5Zn-1Ce合金具有最高的强度。T5处理态合金的抗拉强度、屈服强度和伸长率分别为236 MPa、111 MPa和15.8%，T6处理态合金分别为233 MPa、131 MPa和8.9%。强度提高的主要原因是合金中生成了大量的纳米级Mg4Zn7强化相，以及晶界沉淀相的连续性降低；（4）含重稀土元素合金的时效硬化效果高于含轻稀土元素的合金，经T6处理后，含重稀土元素合金的断裂强度和屈服强度均提高，而含轻稀土元素合金只有屈服强度提高。 　　研究了挤压变形Mg-4.5Zn-1Ce合金的组织和性能。473 K时效后峰值态合金具有较高抗拉强度和屈服强度，其值分别为291 MPa和239 MPa，比铸态分别提提高了55 MPa和128 MPa。高强度产生的原因是合金中生成了大量棒状和点状混合结构的纳米级Mg4Zn7强化相和晶粒的细化。 　　应用Edge-to-edge匹配模型成功预测了MgZn2/α-Mg体系中的位相关系，扩大了该模型的应用范围。并对模型进行了改进，主要体现在：1)确定匹配方向的平面上所有原子的中心位置需在平面上；2）匹配方向之间可任意配对。应用优化后的模型预测了Mg17Al12/α-Mg体系中的位相关系，预测结果与实验结果的吻合率为4/6，好于原模型预测的吻合率4/8。另外，使用优化后的模型，成功的预测出了理想的Burgers位相关系，从而证实了该位相关系是确实存在的，而不是near Burgers位相关系测定的误差。使用优化后的模型还成功的解释了该合金体系中稀土元素的晶粒细化机制和沉淀强化机制。

Mg-Al-Mn-RE系合金组织与性能研究

利用金属型铸造制备了Mg-5Al-0.3Mn-xRE (x = 0~4, wt%，RE = Ce, Nd, Sm, Y和(CeLa)混合稀土)系列合金，研究了铸态合金的组织和力学性能。利用轧制和挤压技术对优化出的合金进行了变形加工处理，并研究了合金加工后的组织和力学性能。 对于铸态合金，稀土元素不仅可以细化合金的晶粒，而且形成不同类型的Al-RE化合物，含Ce的合金中生成Al11Ce3相，含Nd或Sm的合金中，主要生成Al11Nd3 (Al11Sm3)相和少量的Al2Nd (Al2Sm)相，含Y的合金中生成Al2Y相。另外，添加稀土可以改变Mg17Al12相的形貌，使其变得更加细小、弥散。添加适量的稀土可以明显提高铸态合金在室温和150℃下的力学性能，Mg-5Al-0.3Mn-1.5Ce, Mg-5Al-0.3Mn-2Nd和Mg-5Al-0.3Mn-2Sm合金在各自的体系中具有最佳的综合力学性能。合金力学性能提高的主要原因是细晶强化、Al-RE化合物第二相强化以及减弱Mg17Al12相对合金高温力学性能的不利影响。 对Mg-5Al-0.3Mn-(1.0, 1.5, 2.0)Ce，Mg-5Al-0.3Mn-2Nd，Mg-5Al-0.3Mn-1.5(CeLa)和Mg-5Al-0.3Mn-3Y合金在300-400℃下进行了热轧制或挤压变形，与铸态合金相比，轧制和挤压合金具有更高的力学性能。轧制合金的室温抗拉强度为290-340 MPa，较铸态合金提高约50％，屈服强度约为210-260 MPa，较铸态合金提高约2倍。挤压态合金的抗拉强度为260-270 MPa，屈服强度为160-190MPa，伸长率为20-22％；150℃的力学性能也得到了明显改善。 结合热力学计算、合金化元素之间的电负性差、化合物相的生成焓数据以及相图计算，阐述了稀土化合物相的生成机制，稀土元素与Al元素之间的电负性差大于其与Mg之间的电负性差，且Al-RE相的生成焓远低于Mg-RE和Mg-Al相的生成焓，因此在Mg-Al合金中加入RE后，RE优先与Al形成Al-RE化合物。从晶粒细化、化合物强化相的生成和演变、变形加工处理的位错交互作用等方面讨论了合金的强化机制，认为细晶强化、第二相强化及形变强化是提高合金力学性能的主要机制。

稀土在铝酸盐中发光性质的研究

分别采用溶胶凝胶方法，固相合成法，燃烧法，均相沉淀法在不同的铝酸盐中研究了稀土离子的发光性质及稀土离子之间的能量传递。并对各种方法合成的稀土铝酸盐的发光性能进行比较。全新方法——均相沉淀法合成的稀土铝酸盐既克服了传统的溶胶凝胶方法中有机碳对还原气氛的影响，又能够在较低温度下，较短的时间内合成铝酸盐，克服铝酸盐合成温度高时间长的弊病。以这种方法在750 ℃，4h即可合成发光性能较好的铝酸盐磷光体。系统的合成铝酸盐MAl_2O_4:Eu~(2+), RE~(3+) （M = Mg, Ca, Sr, Ba; RE = Y, La, Ce, Pr, Nd, Sm, Gd, Tb, Dy, Ho, Er, Tm, Yb, Lu）的发光及长余辉性质，发现Pr, Nd, Dy, Ho, Er均能够有效的延长MAl_2O_4:Eu~(2+)的发光寿命，同时增强MAl_2O_4:Eu~(2+)的发光亮度。其中以Dy, Eu共掺的铝酸盐磷光体的寿命最长。对于碱土金属，虽然同属于鳞石英结构，但其晶体结构存在明显差别：Mgl_2O_4:Eu~(2+)，RE~(3+)隶属于立方晶系，Ca Al_2O_4:Eu~(2+)，RE~(3+)和β－SrAl_2O_4:Eu~(2+)，RE~(3+)隶属于单斜晶系，Ba Al_2O_4:Eu~(2+), RE~(3+)隶属于六角晶系。所以在发光性能及长余辉性能上表现出不同的特性：Mg Al_2O_4:Eu~(2+)，RE~(3+) 和Ba Al_2O_4:Eu~(2+), RE~(3+)的发光分别为480nm, 500nm, 界于Ca Al_2O_4:Eu~(2+), RE~(3+) (436 nm)和 β－SrAl_2O_4:Eu~(2+)，RE~(3+) (520 nm)之间。而 Ca Al_2O_4:Eu~(2+)，RE~(3+)和β－SrAl_2O_4:Eu~(2+)，RE~(3+)由于同属于单斜晶系，所以其发光满足原子序数的变化规律：当某一原子取代较小的其他原子时，发光波长向短波移动。而且Ca Al_2O_4:Eu~(2+)，RE~(3+)和β－SrAl_2O_4:Eu~(2+)，RE~(3+)都具有较强的发光及余辉。发现新型长余辉发光物质碱土铝酸盐MA:Eu~(2+)，RE~(3+)，波长位于489nm，是一种发光和余辉都极强的发光材料。而且碱土铝酸盐MA:Eu~(2+)，RE~(3+)能与β－SrAl_2O_4:Eu~(2+)，RE~(3+)生成非常有效的混晶化合物，从而使其发光在489nm～520 nm的波长范围内移动而不影响化合物的发光性能。研究了SrGdAlO_4:RE~(3+) （RE = Ce, Pr, Nd, Sm, Eu, Tb, Dy, Ho, Er, Tm, Yb, Lu）的发光现象，观察到SrGdAlO_4:RE~(3+) （RE = Ce, Pr, Nd, Sm, Eu, Tb, Dy, Ho, Er）的特征发光，由于Tm, Yb, Lu 在可见区无吸收，所以观察不到它们的发光。讨论并研究了SrGdAlO_4:RE~(3+) 体系的Gd~(3+) → Gd~(3+)，Gd~(3+) → RE~(3+)的能量传递机理，总结了RE~(3+)对Gd~(3+)的激发能的俘获速率次序依次为： Eu ＞ Tb ＞Er ＞ Dy ＞ Sm ＞ Ho ＞ Nd，能量传递主要是通过偶极－偶极相互作用实现的。观察到SrGdAlO_4:Tb~(3+)长余辉发光。