1.3μm分布反馈二极管激光器组件

开发了一种用于光纤公用天线电视（ＣＡＴＶ）的分布反馈激光二极管组成，组件包括１．３μｍＩｎＧａＡｓ／ＩｎＰ双沟－平面掩埋双异质结（ＤＣ－ＰＢＨ）分布反馈激光二极管和光隔离器，封装在蝴蝶型管壳内，组件的出纤线性功率为２．５ｍＷ，并具有极低的失真。     

Finite difference methods for solving the two-dimensional advection–diffusion equation

Using weighted discretization with the modified equivalent partial differential equation approach, several accurate finite difference methods are developed to solve the two-dimensional advection–diffusion equation following the success of its application to the one-dimensional case. These new methods are compared with the conventional finite difference methods in terms of stability and accuracy. The new methods are more accurate and often more stable than the conventional schemes.     

炸药爆轰产物驱动刚塑性球壳的加速运动

 从质量和动量守恒关系出发，导出了不可压缩刚塑性球壳在球面散心和聚心爆轰作用下的运动方程。应用本文结果计算球壳的加速运动与实验结果及动力有限元程序DYNA的数值摸拟结果吻合。     

纳秒级脉宽砷化镓激光器阵列

报导砷化镓激光器阵列的实验结果。该阵列光束的脉宽约０．７～５ｎｓ，近场光斑面积约１００ｍｍ×６ｍｍ；已被用于触发高功率电磁脉冲发生器中的半导体光导开关阵列。报导一种提高光脉冲重复率的方法—双脉冲序列法，用该方法使激光脉冲等效重复率达约１００ＭＨｚ；介绍一种使激光器阵列输出光斑中光能均匀分布的多光束叠加方案。     

利用X射线衍射研究冲击波合成纤锌矿型氮化硼

 用X射线衍射法，对不同结晶度的石墨型氮化硼（gBN）在冲击波作用下转变成的纤锌矿型氮化硼（wBN）产物进行了研究，对wBN中的杂质含量等进行了分析。结果表明：gBN的石墨化指数G.I值对wBN的产率有明显的影响。     

Method for calculating the complete expansion of the Glauber amplitude for nucleus-nucleus scattering

A method for calculating the complete expansion of the Glauber amplitude for nucleus-nucleus scattering processes is proposed. An example of the calculation of the elastic differential cross section is given as an illustration.     

207Bi L-subshell orbital electron capture probabilities and decay energy

The L₁ subshell orbital electron capture probability P_L1 in the decay of 33.4 y ²⁰⁷Bi to the 2339.89 keV level in ²⁰⁷Pb is measured to be 0.518 ± 0.081 (95% confidence) by a new method in which L₁ subshell characteristic X-rays in the L_γ X-ray peak are observed in an Xγt coincidence mode with 1770.23 keV γ-rays. The value of P_L2is 0.047 ± 0.015 (95% confidence). From these results a value of Q_EC = 39_-8⁺²¹ keV is obtained for capture transitions to the 2339.89 keV level. The absence of K-capture to this level also is established by absence of K X-rays in coincidence with 1770.23 keV γ-rays.     

γ射线暴的最新研究进展:火球模型、余辉及前身星

γ射线暴（称简γ暴）的研究在最近几年里有了巨大的突破。观测上，人们发现了γ暴的低能余辉以及与γ射线发同时的光学爆发，还发现了它位于宇学距离的寄主星系。越来越多的观测证据还表明长时标γ暴与恒星形成区、甚至可能与超新星成协。在γ暴的相对论火球模型框架下，人们对γ暴以及余辉的产生机制的认识也有了进展。进而人们对γ暴的前身星以及环境效应等有了新的认识。本文旨在对这些进展和认识给一个扼要的评述。