稀土掺杂氧卤玻璃光谱性质研究(英文)

本研究主要目的在于探索适用于宽带光纤放大器和蓝绿光激光器用稀土掺杂基质玻璃材料．通过对掺Er^3＋重金属氧氟玻璃的光谱性质和析晶稳定性研究以及稀土离子掺杂重金属氧卤玻璃的上转换发光研究，为其在宽带掺Er^3＋光纤放大器和蓝绿光波段激光器中的潜在应用提供基础．研究结果表明：重金属PbF2的加入提高了掺Er^3＋硅酸盐玻璃和锗酸盐玻璃的带宽特性和增益性能；首次在Er^3＋／Yb^3＋共掺和Er^3＋单掺硅酸盐玻璃发现上转换蓝光；重金属氟化铅的加入提高了Er^3＋单掺锗酸盐和碲酸盐玻璃的上转换发光；在室温下同时

Kinetic studies on the effects of rare earth elements (REES) on the growth of Microcystis and their accumulation by Microcystis

In the paper the kinetic effects of La3+ and Ce4+ on the growth of Microcystis and the accumulation kinetics of Microcystis in the single and combined systems of La3+ and Ce4+ were studied. The mechanism of the effects of La3+ and Ce4+ on the growth of Microcystis and their accumulation kinetics were also discussed. In the single system, La3+ stimulated the growth of Microcystis at initial concentrations below 2 mg / 1, but inhibited it above 2 mg / 1. Ce4+ accelerated the growth of Microcystis at initial concentrations below 0.2 mg / 1 and inhibited at above 0.2 mg /l. Furthermore, the stimulation weakened with the increase of initial concentrations of La3+ and Ce4+. In the combined system, the growth of Microcystis was accelerated in the over all cases. In the single system, the amount of La3+ and Ce4+ uptake was more at higher initial concentrations than at lower ones. At the same initial concentrations, La3+ and Ce4+ uptake in the combined system was less than that in the single system. The kinetic process of La3+ and Ce4+ adsorpted by Microcystis can be explained with the second order kinetics adsorption model.

稀土掺杂长余辉发光玻璃的研究

稀土掺杂的长余辉发光玻璃是一种新型的发光材料，其应用范围可以从传统的弱光照明领域延伸到信息存储领域。我们在探找新型的长余辉发光玻璃体系的过程中，总结了一些设计长余辉玻璃材料的方法，研究了稀土离子在玻璃基质中的发光行为和斓系离子与材料中缺陷的作用。我们在论文中首次报道了稀土掺杂的碱土硼硅酸盐玻璃的长余辉发光和光激励长余辉发光现象。试激活的碱土硼硅酸盐玻璃（Ro-BZO3-5102：TbZo3，R＝Mg，ca，s几B。）在254 nm紫外光辐照30 min以后，余辉时间长达6-10个小时。将激发后的玻璃避光保存24小时至余辉消失后，再使用低能量的366 nm的紫外光檄发样品，玻璃会重新发射长余辉，即产生光激励长余辉发光；而未预先经254 nm紫外光辐照的玻璃没有光激励长余辉现象发生。在这一体系中，光激励长余辉的衰减与首次激发的长余辉的衰减具有不同的衰减规律，辅以吸收光谱和热释光谱的表征，我们对其发光的机理进行了探讨。我们还研究了三价稀土离子在碱土硼硅酸盐玻璃中的发光性质，以及共掺稀土和其他金属离子对试激活的碱土硼硅酸盐玻璃荧光和长余辉发光的影响。此外1本论文还首次报道了Du3+，Tm+和Zr4+等离子在玻璃中的长余辉发光现象。

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。

CALCULATED ELECTRONIC AND MAGNETIC-STRUCTURES OF THE NEW TERNARY RARE-EARTH IRON NITRIDE ND2FE17N3

The electronic and magnetic structures of Nd2Fe17 and Nd2Fe17N3 have been calculated using the first-principle, spin-polarized orthogonalized linear combination of atomic orbitals method. Comparative studies of the two materials reveal important effects of the nitrogen atoms (at 9e site) on the electronic and magnetic structures. Results are presented for the total density of states, site-projected partial density of states and the spin magnetic moments on four nonequivalent Fe sites. The highest magnetic moments are found to be located on the 6c site for Nd2Fe17 and on the 9d site for Nd2Fe17N3, in agreement with the neutron and Mossbauer experiments. The variation trends of the magnetic moments on different Fe sites are discussed in terms of the separation between Fe and N atoms. Compared with Nd2Fe17, an increase in the exchange splitting of the Fe d band is found in Nd2Fe17N3, which accounts for its higher Curie temperature as observed in experiments. The calculated results show that the nitrogen atoms are charge acceptors in these compounds.