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.

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.

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.

A 5.6-mW Power Dissipation CMOS Frequency Synthesizer for L1/L2 Dual-Band GPS Application

This paper presents a wide tuning range CMOS frequency synthesizer for dual-band GPS receiver, which has been fabricated in a standard 0.18-um RF CMOS process. With a high Q on-chip inductor, the wide-band VCO shows a tuning range from 2 to 3.6GHz to cover 2.45GHz and 3.14GHz in case of process corner or temperature variation, with a current consumption varying accordingly from 0.8mA to 0.4mA, from a 1.8V supply voltage. The measurement results show that the whole frequency synthesizer costs a very low power consumption of 5.6mW working at L I band with in-band phase noise less than -82dBc/Hz and out-of-band phase noise about -112 dBc/Hz at 1MHz offset from a 3.142GHz carrier.

1.3 mu m high indium content (42.5%) GaInNAs/GaAs quantum wells grown by molecular beam epitaxy

High structural and optical quality 1.3 mu m GaInNAs/GaAs quantum well (QW) samples with 42.5% indium content were successfully grown by molecular beam epitaxy. The growth of well layers was monitored by reflection high-energy electron diffraction (RHEED). Room temperature photoluminescence (PL) peak intensity of the GaIn0.425NAs/GaAs (6 nm / 20 nm) 3QW is higher than, and the full width at half maximum (FWHM) is comparable to, that of In0.425GaAs/GaAs 3QW, indicating improved optical quality due to strain compensation effects by introducing N to the high indium content InGaAs epilayer. The measured (004) X-ray rocking curve shows clear satellite peaks and Pendellosung fringes, suggesting high film uniformity and smooth interfaces. The cross sectional TEM measurements further reveal that there are no structural defects in such high indium content QWs. (c) 2006 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim.

Strain-Compensated InGaAs/InAlAs Quantum Cascade Detector of 4.5 mu m Operating at Room Temperature

We present a strain-compensated InP-based InGaAs/InAlAs photovoltaic quantum cascade detector grown by solid source molecular beam epitaxy. The detector is based on a vertical intersubband transition and electron transfer on a cascade of quantum levels which is designed to provide longitudinal optical phonon extraction stairs. By careful structure design and growth, the whole epilayer has a residual strain toward InP substrate of only -2.8 x 10(-4). A clear narrow band detection spectrum centered at 4.5 mu m has been observed above room temperature for a device with 200 x 200 mu m(2) square mesa.

VLBI observations of a sample of 15 EGRET-detected AGNs at 5 GHz

We report VLBI observations of 15 EGRET-detected AGNs with European VLBI Network (EVN) at 5 GHz. All sources in the sample display core-jet structures.

高Tc超导体R_1Ba_2Cu_3O_(2-x)(R-rare earth)的磁性和超异电性研究

本论文合成了R_1Ba_2Cu_3O_(2-x) (R = La、Nd、Sm、Eu、Gd、Dr、Ho、Er、Tm、Yb)、Y_2Ba_2Cu_3O_(2-x) (x = 0.10～1.17)和Y_1Ba_2Cu_3O_(7-x)S_x (x = 0～2)，并对磁性和超导电性进行了较为系统的研究。R_1Ba_2Cu_3O_(2-x)的磁化率在T > Tc的很宽的温度范围内服从Curic-Weiss定律，求得的有效磁矩略大于理论值，差值与Y_1Ba_2Cu_3O_(2-x)中Cu~(2+)磁矩相近，说明Cu~(2+)的磁矩对体系磁性有额外贡献，这贡献随R~(3+)离子中自旋平行的电子权的增多而增大。其高温下的磁化率CT > 700K)相对Curic-Weiss定律发生较大偏离，这偏离可能的来源有三个：高温下稀土离子发生较大的能级反转效应，高温下结构相变对磁性的影响，高温下氧含量减少造成Cu~(2+)磁矩增大。R_1Ba_2Cu_3O_(2-x)磁化率在T < Tc时也服从Curic-Weiss定律，R~(3+)磁矩是定域的，表明超导与磁性相互独立。互不相关，稀土磁矩与传导电子间无相互作用。用Sr取代R_1Ba_2Cu_3O_(2-x)中的Ba，没能使体系产生磁有序的变化，但却使有效磁矩增大，并完全破坏了样品的超导电性。Sm~(3+)磁化率不服从Curic-Weiss定律，在Sm_1Ba_2Cu_3O_(2-x)中Sm~(3+)显示了典型Van VlccK离子的特性。Y_1Ba_2Cu_3O_(2-x)随氧含量减少发生超导体一半导体一绝缘体的转化，当氧含量由6.90减小至6.49时发生由正交到四方的结构相变。当(7-x) = 5.83时有较多杂质相出现，123相开始分解。样品磁化率均服从Curic-Weiss定律，并随氧含量增大磁化率－温度曲线越来越趋于平缓（直线），当(7-x) = 6.90时磁化率基本不随温度变化，这时Pauli顺磁性占主导地位，这说明氧含量增加定域磁矩减少，求得的有效磁矩Peff随氧含量增大总趋势减小。提出了电子“巡游”的观点，较好地解释了上述现象，并推测出Cu(2)的d电子是离域的，对样品磁矩没有贡献，样品Peff来源于部分Cu(1)的定域Cu~(2+)的磁矩，上述推测被EPR结果证实。正交相Y_1Ba_2Cu_3O_(2-x)的EPR谱显示了中心对称成准立方晶场中Cu~(2+)(d~9, S = 1/2, I = 3/2)的EPR物性。而四方相样品的EPR谱却出现了明显的各向异性，说明观察到的为Cu(1)的EPR信号，由Cu(1)~(2+)的写域磁矩产生。Y_1Ba_2Cu_3O_(2-x)的EPR信号束源于本体相，而非Y_2Cu_2O_5、BaCuO_2、Y_2BaCuO_5等杂质相。各样品EPR信号的自旋浓度远小于1spin/cu，并随氧含量减小而增大，当(7-x) = 6.49、6.40时自旋浓度出现陡增，这时伴随由正交到四方的转化，证明了电子“巡游”观点的正确。用硫部分取代Y_1Ba_2Cu_3O_2g中的氧，当Y_1Ba_2Cu_3O_(2-x)Sx中x = 0.11时Tc = 92.6K，比Y_1Ba_2Cu_3O_(7-x)升高2K，但由于杂质相的存在，ΔTc加宽。其他样品多为半导体和绝缘体。硫取代0，当x = 0.04，0.06，0.11和1.20时磁化率服从Curic-Weiss定律，并且x = 0.87，1.2时分别在230K、240K出现反铁磁有序。其他样品由于Cu被还原为＋1价而变成抗磁性。x = 0.11 (Tc = 92.6K)，EPR谱为正交场中Cu~(2+)的信号。自旋浓度与温度无关。当所有Cu均为Cu~(1+)时，测问的是-s-的EPR信号，而Cu为混合价态(+1和+2时)测问是上述两种信号的叠加。

耐硫水煤气变换反应NiO-MoO_3-K_2CO_3/r-Al_2O_3催化剂研究

在本工作中，制备了一系列催化剂样品，其中有K、Ni、Mo单组份催化剂，K-Ni、K-Mo、Ni-Mo双组份催化剂及不同活性组份含量的K-Ni-Mo三组份催化剂。针对水煤气变换反应，对上述催化剂进行反应活性考察，得出如下结果：①催化剂各活性组份的最佳含量大致是NiO(3%), MoO_3(13%), K_2CO_3(6%)；②催化剂制备中的最佳焙烧温度在400 ℃左右；③催化剂使用前用H_2S/H_2的混和气进行预处理其效果最佳；④催化剂的催化活性与催化剂表面硫的含量有关，当催化剂表面处于严重缺硫状态时其活性下降；⑤反应的最佳汽:气 = 0.5-1.5；⑥加压有利于催化剂活性的提高，在加压情况下催化剂的活性随着反应温度的增加通过一极大值（在约200 ℃左右），不加压的反应催化剂活性随着反应温度的提高而增加。在催化剂的表征部分，利用XPS、XRD、紫外可见温反射光谱、SEM、ESR、比表面、TPR、酸度测定、TPD、TPS、TPS-TPR等实验对我们所制备的催化剂进行了研究。最后，我们用ESR和XRD实验技术研究了MoO_3、M_2CO_3 (M = Li、Na、K、Cs)-MoO_3加热过程中的固相反应，知道MoO_3在空气中焙烧时可以失去晶格氧，使晶体中的一些Mo~(6+)变成Mo~(5+)。在焙烧过程中，Li、Cs~+的加入将阻止MoO_3晶格氧向气相氧的转变，对Mo~(5+)的生成有抑制作用。加入一定量Na~+、K~+的MoO_3在焙烧过程中，其晶格氧被活化更易失去它们对Mo~(5+)的生成有促进作用，这种作用的大小是Na~+ > K~+。

R面、C面蓝宝石上生长的InGaN多层量子点的发光性质研究

采用表面钝化和MOCVD低温生长在蓝宝石（0001）面（即C面）和蓝宝石(1(1-bar)02)面（即R面）上形成了InGaN量子点，并构成了该量子点的多层结构。原子力显微镜测试的结果表明单层InGaN量子点平均宽约40nm，高约15nm；而多层量子点上层的量子点则比单层的InGaN量子点大。R面蓝宝石衬底上生长的InGaN量子点和C面蓝宝石衬底上生长的InGaN量子点相比，其PL谱不仅强度高，而且没有多峰结构。这是由于在C面蓝宝石衬底上生长的InGaN/GaN多层量子点沿生长方向[0001]存在较强的内建电场，而在R面蓝宝石衬底上得到的多层量子点沿着生长方向[11(2-bar)0]没有内建电场。InGaN量子点变温光致发光（PL）谱研究发现量子点相关的峰有快速红移现象，这是量子点系统所特有的PL谱特征。用在R面蓝宝石上生长的InGaN量子点作有源层有望避免内建电场的影响，得到高量子效率且发光波长稳定的发光器件。

1.5 mu m DFB integrated with vertical tapered spotsize converter fabricated by selective MOVPE

1.5 mu m DFB LD butt-joint integrated with vertical tapered spotsize converter was fabricated by LP-MOVPE. The vertical far field angle (FWHM) was decreased from 34degrees to 10degrees the threshold currents was as low as 19.8mA, the output power was 9.6mw at 100mA without HR coating and the SMSR was 35.8dB. The 1-dBm misalignment tolerance was 3.2 mu m, while the counterpart of the device without SSC was 2.2 mu m.

Fe-57 Mossbauer spectroscopic and magnetic studies of R3Fe29-xVx (R = Y, Ce, Nd, Sm, Gd, Tb, and Dy)

Mossbauer spectra for Fe atoms in the series of R3Fe29-xVx (R = Y, Ce, Nd, Sm, Gd, Tb, and Dy) compounds were collected at 4.2 K. The ratio of 14.5 T/mu(B) between the average hyperfine field B-hf and the average Fe magnetic moment mu(Fe)(MS), obtained from our data, in Y3Fe29-xVx is in agreement with that deduced from the RxTy alloys by Gubbens et al. The average Fe magnetic moments mu(Fe)(MS) in these compounds at 4.2 K, deduced from our Mossbauer spectroscopic studies, are in accord with the results of magnetization measurement. The average hyperfine field of the Fe sites for R3Fe29-xVx at 4.2 K increases with increasing values of the rare earth effective spin (g(J) - 1) J, which indicates that there exists a transferred spin polarization induced by the neighboring rare earth atom.

Mossbauer spectroscopy study of Fe-57 in R3Fe29-xTx (R=Y, Ce, Nd, Sm, Gd, Tb and Dy; T=V and Cr)

Fe-57 Mossbauer spectra for the Fe atoms in the R3Fe29-xTx (R=Y, Ce, Nd, Sm, Gd, Tb, Dy; T=V, Cr) compounds were collected at 4.2 K. The analysis of Mossbauer spectra was based on the results of magnetization and neutron powder diffraction measurements. The average Fe magnetic moments at 4.2 K, deduced from our data, are in accord with magnetization measurements. The average hyperfine field of Tb3Fe29-xCrx (x=1.0, 1.5, 2.0, and 3.0) decreases with increasing Cr concentration, which is also in accordance with the variation of the average Fe magnetic moment in the Tb3Fe29-xCrx compounds.

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.