Er3+:Yb3+共掺杂氟氧混合物玻璃的上转换发光研究

制备了化学配方为 (5 0 -x)GeO2 ·PbF2 ·WO3·(6 +x)CdF2 ·1 4Yb2 O3·0 6Er2 O3(x =10 ,2 0 ,30 )氟氧混合物玻璃。研究了 930nm发光二极管激发下Er3+ :Yb3+ 共掺杂情形下的Er3+ 离子的上转换发光特性 ,观测到了Er3+ 离子中心波长位于 5 4 3,5 5 0和 6 5 5nm处的三个强荧光发射带。通过对样品的反斯托克斯喇曼光谱的测量 ,确定了基质的最大声子能量 ,在此基础上分析了上转换荧光的产生机制。利用基质的平均电负性差和平均阳离子场强这两个参数 ,讨论了基质材料中GeO2 和CdF2 含量的调整对上转换发光的影响。     

Be++离子基态非相对论能量和波函数的变分计算

采用了一种包含坐标张弛系数的试探波函数,对Be++离子的基态能量和解析波函数进行了变分计算,得到了比较理想的结果.     

基于Schrdinger方程的耦合常数解析延拓方法

基于Schrdinger方程,利用耦合常数解析延拓方法研究了球对称的方势阱、Woods-Saxon势和谐振子势中的单粒子共振态的能量与宽度.分析了耦合常数的取值区间和Pade多项式阶数对计算结果的影响.结果发现,在适当的耦合常数取值范围内,随着Pade多项式阶数的增加可以得到稳定和收剑的单粒子共振态能量与宽度.     

磁暴形态类型与行星际磁云特征

本文分析了6个不同特征的行星际磁云所引起的急始型磁暴形态的类型差别,得到的主要结论是:磁云前高密度结构是决定磁暴初相特征的重要因素;在磁云磁场强度相近的条件下,背景太阳风及磁云的速度均影响着磁暴主相的发展;磁暴强主相的开始及恢复决定于磁云磁场矢量相对于黄道面倾角的指向;强正磁云引起的磁暴的主要特征是主相长时间的延迟;磁云过后,太阳风流速仍继续影响着磁暴主相的恢复.     

可调谐激光晶体S因子和声子能量的估算

本文采用了一种特别的多模电-声子耦合模型,利用室温光谱数据估算可调谐激光晶体的黄昆-里斯(Huang-Rhys)S因子,并与单模耦合模型的结果作了比较.最后,还讨论了S因子与晶场强度及基质晶体价键特性之间的关系.     

Isospin Effect of Coulomb Interaction on Nuclear Stopping in Intermediate Energy Heavy Ion Collisions

Nuclei offer an interesting isospin situation where symmetry potential, Coulomb term and isopin dependent nucleon-nucleon collisions are simultaneously present. However, in general, Coulomb potential is not studied in the heavy ion collisions. As we know that the Coulomb potential is an important asymmetry term which can bring important isospin effect into the observable in the intermediate energy heavy ion collisions. Recently extensions by Colonna et al.[1] to finite nuclei show that Coulomb and surface effects reduce instability regions. So in this paper the isospin effects of Coulomb term and symmetry potential on the nuclear stopping at intermediate energy heavy ion collisions are studied by using isospin-dependent quantum molecular dynamics model (IQMD).     

峰值能量检测及其在被动声纳显示中的应用

本文介绍子带峰值能量检测方法及其在被动声纳显示和检测中的应用[2-4]，同时提出了波束域宽带峰值能量检测算法。新的波束域算法是在已有波束形成的基础上进行处理，不需对原系统进行较大的修改。通过波束域宽带峰值能量检测处理，可以改善声纳显示效果，更加清晰地显示目标方位。相对于高分辨率波束形成算法，两种峰值能量检测算法的运算量都比较低，具有一定的工程应用前景。通过计算机仿真和实测数据处理，验证了所述两种峰值能量算法在提高显示清晰度，减小测向模糊度方面的优点。     

Tritium Burn-up Depth and Tritium Break-Even Time

Similarly to but quite different from the xenon poisoning effects resulting from fission-produced iodine during the restart-up process of a fission reactor, we introduce a completely new concept of the tritium burn-up depth and tritium break-even time in the fusion energy research area. To show what the least required amount of tritium storage is used to start up a fusion reactor and how long a time the fusion reactor needs to be operated for achieving the tritium break-even during the initial start-up phase due to the finite tritium breeding time that is dependent on the tritium breeder, specific structure of breeding zone, layout of coolant flow pipe, tritium recovery scheme, extraction process, the tritium retention of reactor components, unrecoverable tritium fraction in breeder, leakage to the inertial gas container, and the natural decay etc., we describe this new phenomenon and answer this problem by setting up and by solving a set of equations, which express a dynamic subsystem model of the tritium inventory evolution in a fusion experimental breeder （FEB）. It is found that the tritium burn-up depth is 317g and the tritium break-even time is approximately 240 full power days for FEB designed detail configuration and it is also found that after one-year operation, the tritium storage reaches 1.18kg that is more than the least required amount of tritium storage to start up three of FEB-like fusion reactors.