旋转工况下小型液冷源设计

设计了一种适用于旋转工况的小型液冷源,该液冷源采用强迫风冷换热器的原理。液冷源液路循环采用闭式系统设计以适应旋转工况的要求,液位检测采用光电式液位传感器,通过单向阀和电磁阀的组合使用可有效防止水锤效应。该系统具有体积小、重量轻、环境适应性强等优点。     

多元微分学中几个重要概念间的因果关系

通过一些反例说明多元函数的极限、连续、偏导数存在、方向导数存在、可微等概念之间的关系。     

换个角度讲解"uL=-eL"

对纯电感电路，中等职业学校教材是这样分析“uL=-eL”：电路图如图1所示，假定通过线圈的电流是按初相等于零的正弦交流电，即i=Im sinωt，它将产生自感电动势eL，根据图1所假定的电压uL、小自感电动势eL、电流i的正方向，运用基尔霍夫回路电压定律，沿回路顺时针（或逆时针）方向绕行一周，     

Form Invariance and Noether Symmetries of Rotational Relativistic Birkhoff Systems

Under the infinitesimal transformations of groups,a form invariance of rotational relativistic Birkhoff systems is studied and the definition and criteria are given,In view of the invariance of rotational relativistic Pfaff-Birkhoff-D‘ Alembert principle under the infinitesimal transformations of groups,the theory of Noether symmetries of rotational relativistic Birkhoff systems are constructed.The relation between the form invariance and the Noether symmetries is studied ,and the conserved quantities of rotational relativistic Birkhoff systems are obtained.     

基于旋转描述的三维几何造型方法

提出了一种能用凸四边形表示并可作平面展开的三维实体造型的设计方法。该方法用旋转描述表把二维平面展开图和三维实体联系起来，模拟人工折叠过程，由二维平面展开图逐次旋转变换完成三维造型重建。造型重建后，再通过纹理映射将平面设计图案映射到实体的各个面上，完成对实体着色渲染，生成具有真实感的三维实体。     

Gamow—Teller Resonance of 90Zr in a Relaztivistic Approach

We establish the formalism of nuclear spin-isospin excitations,especially the Gamow-Teller resonance in a fully consstent relativistic random-phase approximation.A relativistic form of the Landau-Migdal parameter g‘ is adopted as a residual spin-isospin correlation force.In the non-relativistic limit it reproduces the excitation energy of the giant Gamow-Teller resonance state obtained in the non-relativistic model.The Gamow-Teller resonance for finite nuclei is investigated in a relativistic approach for the first time.It is found that the Ikeda sum rule of 90Zr is quenched about 8% in the Hartree as well as the correlated strengths due to the poles of the negative Dirac states at energies above 1 GeV.     

Rotational Deformation of Neutron Stars

The rotational deformations of two kinds of neutron stars are calculated by using Hartle‘s slow-rotation formulism. The results show that only the faster rotating neutron star gives an obvious deformation. For the slow rotating neutron star with a period larger than hundreds of millisecond, the rotating deformation is very weak.     

问题88

零向量是一个特殊向量．有这样一个命题：零向量与任意非零向量方向相同．关于其真假有两种不同的观点。