磁场处理燃料油的光谱分析

本文采用了紫外光谱、红外光谱、激光喇曼光谱、荧光和磷光等多种光谱分析方法。通过紫外、红外和激光喇曼光谱分析，由吸收峰的位移来判断油分子结构的变化：实验已证明吸收峰基本上无位移，从而证明油分子的官能团未因磁场作用而产生变化。通过荧光和磷光光谱分析，由其发射光谱强度的变化来判断磁场作用使油分子状态变化的情况，以及油分子由激发单态窜跃到三重态的情况；实验结果证明，荧光和磷光发射光谱强度基本上无变化。这证明磁场（１００mt数量级）并使油分子处于激发状态，也不能有与自旋S＝1相联系的磁矩存在。     

Autocorrelation Function of Hydrogen Atoms in Magnetic Fields

The autocorrelation function is an important quantity that can reflect the dynamical properties of the Rydberg wave packet and can be measured in experiments. Applying time-dependent perturbation theory and rotating wave approximation, we derive the autocorrelation function of the double-pulse laser describing the evolution of a Rydberg wave packet of hydrogen atoms in magnetic fields. The resulting expression is written as a sum of the modified Caussian terms. Each Caussian term comes from a parent semiclassical closed orbit. It provides a direct explanation and experimentally controllable measurement scheme, which allows us therefore to recognize the closed orbit and to determine its returning time in high precision.     

Introduction and Applications of a Generalized Intermediate Entangled State Representation

We introduce a generalized intermediate entangled state representation ｜β〉Λ to study the energy spectrum of an electron in a uniform magnetic field and a harmonic potential through algebraic calculatiOn. We find that the degeneracy of the energy levels is disappeared due to the existence of the additional potential. We make it clear that the eigenfunction is just the expression of eigenvector, defined in n Fock space, in ｜β〉Λ representation.     

静磁场中的互作用能

讨论了在激发磁场的电流保持不变时和束缚磁荷作为磁场的不变时，两种情况下磁场的相互作用能。结果与静电场类似，两种情况的互作用能中都含有相互磁化，致使物体磁化状态改变作的功。     

定轴转动带电体的远区磁场分布

类比定轴转动刚体转动惯量以及电偶极子电场的计算方法，得出定轴转动带电体的磁矩及其远区磁场分布。     

反铁磁铜氧化合物中的磁致形状记忆

La2-xSrxCuO4(以下称LSCO)是最早发现的高温超导体之一.当x≈0.15时,它具有最高的超导转变温度,Tc=33K.对于x<0.02的轻度掺杂,材料的低温相是反铁磁绝缘体.在室温以上时,层状化合物LSCO晶格具有四方对称性;当冷却样品通过特征温度To,将发生从四方到正交的结构相变.此时,晶体发展出一种被称为孪晶的畴结构,被畴壁分开的相邻区域具有不同的晶轴取向.正交结构的晶格常数a=05339nm,b=0.5422nm,两者相差约1%.为了探求高温超导机理,LSCO曾被广泛深入地研究.由于在超导LSCO中根本不存在41meV反铁磁自…     

"导棒"的启动方式与收尾状态探析

机车的启动问题是机械能部分的重要内容．无独有偶，在磁场中滑轨上的导棒也存在类似的启动问题(简称滑轨问题)，而且两者之间还有相通之处．笔者下面就磁场中导棒的启动方式与收尾状态逐一剖析，与同行探讨．     

提高YBCO块材在外磁场中悬浮力

本给出了三种提高YBCO块材在外磁场中悬浮力的方法．第一种方法是增强外磁场，对于此方法，本研究了一块直径为30mm的圆柱状YBCO块材分别在圆柱状NdFeB永磁体和NdFeB永磁导轨上的悬浮力．测量结果表明在77K温度下YBCO块在圆柱状NdFeB永磁体上的最大悬浮力为50N，在NdFeB永磁导轨上的最大悬浮力为103．ON．第二种方法是提高YBCO块材自身的性能，包括临界电流密度、俘获磁通和块材尺寸，对于此方法，本仅研究了块材尺寸对悬浮力的影响．三块直径分别为30mm、35mm、40mm的圆柱状YBC0块材在NdFeB永磁导轨上的悬浮力被测量，77K温度下5mm悬浮间距时的悬浮力分别为103．ON、134．5N、175．ON．第三方法是将YBCO块材变成准永久磁体，此种情况下，直径为40mm的圆柱状YBCO块材在77K温度下5mm悬浮间距时的悬浮力高达218．3N．     

Structure of Callisto and Ice Holes on Its Surface

The discovery of the induced magnetic field of Callisto that is a satellite of Jupiter has been interpreted as evidence for a subsurface salty liquid-water ocean,so we consider a layered structure of callisto,i.e.,a rock-metal core,an outer layer of ice and a middle layer of ocean.For the rock-metal core we try to indicate how the temperature,pressure and mass density depend on the depth.Due to motionn across the magnetic field of Jupiter in a plasma environment,the ice shell of Callisto must be broken down by electric current.     

谈"楞次定律"的教学

“楞次定律”是《电磁感应》这一章教学的重点和难点。为了帮助学生理解楞次定律和应用楞次定律在解题过程中避免常犯的错误，笔者在教学中采取了以下几点做法。