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?     

佯谬的功劳

 互相排斥的东西结合在一起,不同的音调造成最美的和谐。一切都是斗争所产生的。---赫拉克里特一块石头再硬也只能是一块石头,只有当两块石头彼此撞击的时候才会产生绚丽夺目的火花,物理学正是在一块块坚硬石头的相互撞击中走到了今天。是同时代的或不同时代的物理学家跨越时空的对话使物理学蜕变成了今天的模样。真正的物理学家就像孩童信任自己的母亲那般相信他所持的理论,所以当他的理论受到挑战的时候,他们也会像孩童一样彼此争执,物理学的理论正是在这样的一天天的论战中完善起来的。每一个新的理论问世的时候,总会有大批言论接踵而至,有疑问有赞同更多的是反对。     

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。     

太阳核心中7Be电子俘获几率的计算

在太阳核心的条件下,⁷Be原子被完全电离.所以,重新计算的⁷Be和⁸B太阳中微子流强分别约为4.00×10⁹cm^－2·s^－1和6.18×10⁶cm^－2·s^－1,而标准太阳模型预言的⁷Be和⁸B太阳中微子流强则分别是4.80×10⁹cm^－2·s^－1和5.15×10⁶cm^－2·s^－1.这将进一步增大在Super Kamiokande太阳中微子实验上中微子流强的实验测量值与理论预计值之间的差异.