NiTi合金中马氏体相的低频力学谱研究

我们用最近研制成功的LMA型低频力学谱测试系统对NiTi合金马氏体相进行了在很大频率范围内（0．003～1Hz）的低频等温力学谱和温度谱的测量．我们研究的形状记忆合金NiTi（Ni50．2at％）试样长34mm，直径1mm细丝．经一定热处理，分别在333K．343K和353K做了内耗随频率的变化的测量。实验表明：频率越小，内耗越大，也就是内耗随频率减少而增大。同时我们采用阶梯升温的方法在八个温度下每个温度测量三种频率（1Hz，0．1Hz，0．01Hz）的内耗，结果清楚地表明：不同频率下，内耗峰都出现在372K（99℃）。而且频率越低，峰高越高。这是具有相变峰的特点：相变峰的峰温不随测量频率不同而变化，相变峰高度随频率减少而增大。我们还测量了在1Hz与0．5Hz频率下内耗随温度的变化。本文用马氏体相的位错理论初步讨论了上述实验结果。     

具有周期孔洞和振荡系数的二阶椭圆算子谱分析与数值模拟

讨论具有周期孔洞和振荡系数的二阶椭圆算子的谱问题，得到该问题的多尺度渐近分析公式，并给出数学证明. 文中数值结果也验证了该方法的有效性.     

The Analysis and Improving of the Microwave Exciter in the Lower Hybrid Wave System

When we carry out lower hybrid wave heating and current driving plasma experiment at tokamak, we need mega-watt order of microwave power. The microwave signal at frequency of 2450 MHz is generated by a microwave exciter. According to the experiment＇s demands, the microwave exciter must provide output power of 1.5～ 2. 5 W with stabilized frequency and amplitude tobe used as the klystron input. Being amplified by the klystron, the microwave signal is transmitted through the transmitting system to the antenna and is emitted into the HL-2A tokamak. So we can see that the microwave exciter＇s function is very important to the lower hybrid wave heating and current driving plasma experiment.     

A Compact Magnetically Insulated Line Oscillator with New-Type Beam Dump

We present a compact improved model of the magnetically insulated line oscillator with new-type beam dump and other novel features. In the experiments, high-power microwave of the TM01 mode is generated from the device with a frequency range of 1.73-1.78 GHz and a peak power level of above 2 GW, when the diode voltage is taken in the range 520-540kV, and the diode current is in the range 58-62kA. This confirms the simulation results.     

A modal analysis for the acoustic radiation problems, Ⅱ. Examples

The acoustic radiation modes and the field distribution modes describe the radiation patterns of a complex vibrating surface and the field distribution patterns respectively. The physical meanings of the acoustic radiation modes and the field distribution modes are revealed by numerical method. For a sphere body, a spinning body and a rectangular body, the geometrical patterns of the acoustic radiation modes and the field distribution modes are given. The radiation mode 1 represents the radiation behavior of a monopole radiator, the radiation modes 2 through 4 represent the radiation behavior of dipole radiators respectively, and the radiation modes 5 through 9 represent the radiation behavior of quadrapole radiators respectively. The acoustic radiation modes and the field distribution modes introduce the multi-pole decomposition method into discussion of the acoustic radiation problems.     

中微子物理若干前沿问题

 在过去的几年间,大量的实验结果已经表明中微子有非零质量以及轻子味混合。这一进展为我们打开了一个全新的值得探索的基本粒子世界。关于中微子我们已经知道了多少,我们想要发现什么?本文将从理论与唯象的观点进行阐述。目前中微子物理的前沿问题主要包括:中微子真的发生味转化吗?有几代中微子?存在惰性中微子吗?中微子的质量是多少?中微子是马约拉纳粒子还是狄拉克粒子?轻子味混合矩阵的混合角有多大?轻子味混合矩阵包含CP破坏位相吗?如果包含,那么在中微子振荡和无中微子双β衰变中,这些位相会导致可探测的CP破坏效应吗?     

破解太阳中微子失踪之谜

 2001至2003这3年时间里,太阳中微子的研究进入了一个黄金时期。在这个时期中,一个困扰了物理学家40年的难题被漂亮地解决了。这个难题的解决对于物理学和天文学来说都非常重要。本文将简要回顾3年来关于太阳中微子研究的惊人进展。太阳中微子的产生20世纪上半叶,物理学家们普遍相信太阳发光图1太阳内部的典型核聚变反应是由于其内部不断发生从氢到氦的核聚变反应。根据这一理论,在太阳内部每4个氢核(即质子)转化成1个氦核(4He)、2个正电子(e+)和2个神秘的中微子(νe),见图1所示。     

Viscosity Characteristic in Metallic Melts with Medium／Short-Range Order Structures

Viscosities and liquid structure of alloys Cu75Al25, Cu87Sn13 and Al-12.5%Si and pure metals Cu and Sn are investigated by using torsional oscillation viscometry and high temperature x-ray diffractometry. The viscosities of pure metals and eutectic alloy melts along with the short-range order structure are found to follow the Arrhenius law in a wide range of temperature above the liquidus. The breakpoints in Arrhenius plots emerge when the structures of alloy melts are transformed from the medium-range order structure to the short-range order structure. It has been found that the change of the viscosity of the metallic alloys is a characteristic of microstructure transformation in the related melts.     

太阳中微子失踪案和中微子振荡

 (续前)五、“中微子振荡”是物理学家的法宝按照粒子物理的标准模型,中微子质量为零,它们以光速运动。存在着3种不同类型(即3种“味”)的中微子:电子型中微子(记为νｅ),μ-中微子(记为νμ)和τ-中微子(记为ντ),它们之间彼此不相关,分别只同电子、μ轻子和τ轻子密切相关。不过,早在戴维斯等人公布首批氯探测器的探测结果的1968年,庞托科沃就提出了这3种“味”的中微子很有可能互相来回地转化,称为“中微子振荡”。在太阳内部的热核燃烧过程中产生的中微子都是νｅ。但它们在从太阳到地球的漫长行进过程中,νｅ不断地转化为νμ和ντ。     

齐次群上的平均振荡问题

本文通过构造ｋ－容许覆盖，定义了齐次群上平均振荡空间，并得到该函数空间上的若干等价范数刻划，拓广了文［４］中的结果。