月球的形成

天文学家认为 ,月球是由一个像火星般大小的物体撞入地球 ,将物质溅射到围绕地球的轨道上形成的 .这一撞击还把地球上一天的时间延长到现今的 2 4小时 .月球中的物质一部分来自地球 ,其余部分来自撞击体 .科学家们对撞击体的物质在月球中所占的比例做了估计 ,结果分歧很大 .进行地球化学研究得到的估计值从小于 1%到大于 5 0 % ,而大多数地球物理模型则预言这一比例在 5 0 %到 90 %的范围 .在德国的天文学家通过将月球与地球岩石样品的成分进行比较 ,计算出月球上来自碰撞物体的物质不超过月球的三分之一 .此外 ,他们还估计 ,月球至少是在 4…     

Multiple—Scattering of Near—Edge x—ray Absorption Fine Structure of Sulphur—Passivated InP（100） Surface

We use the multiple-scattering cluster method to calculated the sulphur 1s near-edge x-ray absorption fine structure (NEXAFS) of S-passivated InP(100) surface.The physical origins of the resonances in the NEXAFS have been unveiled.It is shown that the most important resonance is attributed to the photoelectron scattering between the central sulphur and the nearest indium atoms.The studies show that two S-S dimers with the bond lengths of 2.05A and 3.05A coexist in the surface,meanwhile the bridge and antibridge site adsorption of single S could not be ruled out.We support the scanning tunnelling microscopy result that the S-passivated InP(100) surface exhibits significant discorder.     

Indriect Determination of CTMAB with Sodium Chloride and Ammonium Thiocyanate by Floatation and Separation of Zine

A new method for indirect determination of cetyl-trimethyl ammonium bromide (CTMAB) with NaCl and NH4SCH by floatation and separation of zinc has been studied.The study shows that Zn(Ⅱ） can associate with NH4SCN and CTMAB to form insoluble ternary ion-association complex,and the precipitate can float on the surface of the liquid phase.A good linear relationship is observed between the floatation yield(E%) of Zn(Ⅱ） and the amount of CTMAB.On the ground,CTMAB Can be indirectly determined by determining E% of Zn(Ⅱ）.The results were satisfactory.     

Proton Fraction in Neutron Star Matter and Three-Body Force Effects

The three-body force effects on the equation of state and its iso-spin dependence of asymmetric nuclear matter and on the proton fraction in neutron star matter have been investigated[1] within Brueckner Hartree-Fock (BHF) approach by using a microscopic three-body force. It is shown that, even in the presence of the three-body force, the empirical parabolic law of the energy per nucleon vs. isospin asymmetry β=(N-Z)/A is fulfilled in the whole asymmetry range 0 ≤β ≤1 and also up to high density. The three-body force provides a strong enhancement of symmetry energy at high density in agreement with relativistic approaches. Thecalculated proton fraction in β stable neutron star matter is given in Fig.l, where the thick solid line is the BHF prediction using AV18 TBF, while the dotted one is the BHF result using AVis. The thin solid line is the prediction of the Dirac-Brueckner approach taken from Ref.[2]. The results extracted according to the phenomenological paramete rizations of the symmetry energy suggested in Ref.[3] are also plotted. It is seen from     

詹特切克生平简介

 威利鲍德·詹特切克(WillibaldJentschke),是位于汉堡附近的德国粒子物理实验室DESY的创立者,欧洲核研究组织(CERN)的前负责人,他过完90岁生日之后,于2002年3月11日逝世。詹特切克1911年生于维也纳,24岁获得核物理学博士学位,他在维也纳一直工作到1951年,然后他到了伊利诺斯州的恩巴拉大学,任回旋加速器实验室的负责人。1955年,当汉堡大学让詹特切克负责实验物理学研究时,他申请基金在德国建立现代的核物理研究设施。     

双核系统核子转移驱动势与复合核的最佳激发能

计算了以208Pb为靶的一系列重离子熔合反应双核系统核子转移驱动势.它制约由输运方程所支配的核子转移速率,因而确定了双核系统形成复合核的几率.并由此可确定形成复合核所必须的最低激发能,即形成最稳定复合核的最佳激发能,得到了与已知实验值基本符合的结果. Particle transfer driven potentials in Di nuclear System (DNS) in heavy ion collisions based on 208Pb target are calculated. The driven potential controls the particle transfer velocity in the process governed by the diffusion equation, and as a consequence determines the compound nuclear formation probability of DNS. The minimum excitation energy to form a compound nucleus, which is the optimum excitation energy to form the most stable compound nucleus, has been calculated, and the results are basica...     

怀念核物理学家虞福春教授

回顾了虞福春教授一生的业绩，他是一位杰出的实验物理学家，1950年，他最早发现核磁共振谱线的化学位移，为核磁共振技术在化学领域的应用打开了大门，他测定了许多原子核的自旋和磁矩，为检验核壳结构模型作出了重要贡献，他又是一位优秀的教育家，培养了一大批物理人才，他的教学思想已经影响了几代学生。     

单粒子势模型下价核子的密度分布

依据实验事实，利用单粒子势模型，计算了一些核态外层价核子的密度分布.计算给出了价核子在核外部分布的概率和贡献，以此作为晕核态的判断标准.通过研究均方根半径随结合能变化的规律，指出了晕核态存在的条件，尤其是质子晕核态存在的条件.这些对判断和寻找晕核态有现实的指导意义. 关键词： 单粒子势模型 价核子 密度分布 中子晕核态 质子晕核态     

核结构数据库(NSDB)

基于最新的实验评价和模型计算的核结构数据, 组建了一个更新的核结构数据库(NSDB), 目前,该数据库包括稳定同位素的丰度和原子质量, 原子核基态和分离激发态的性质, 及原子核的变形、半径及其它性质等三部分的数据.     

三包层WⅠ和WⅡ型单模光纤波导色散特性的研究

研究了三包层WⅠ和WⅡ型单模光纤的波导色散特性。结果发现在相同条件下，三包层WⅠ和WⅡ型单模光纤零色散点的调节范围比传统的双包层W型单模光纤明显增大。详细分析了几何参量P、Q和光学参量R1、R2对单模传输时的波导色散特性和低次模截止频率的影响。所得的研究结果为获得更为理想的色散补偿、色散平坦光纤及设计新型无源光器件提供了重要的依据。计算波导色散的方法可推广到多包层光纤。