Vlasov方程的数值求解

研究环形加速器中的纵向微波不稳定性,发展了Vlasov方程在(J,φ)坐标下用正交多项式展开的数值计算程序,并把它用于对微波不稳定性的初步研究.     

全相对论性Vlasov－Maxwell方程的解析解

本文给出了全相对论性Ｖｌａｓｏｖ－Ｍａｘｗｅｌｌ方程的解析解。该解是Ｓｗａｄｅｓｈ［１］结果的推广，它既适用于高温聚变等离子体，也适用于有相对论漂移速度的等离子体。     

巨共振激发的相对论效应

在相对论量子场论（ＱＨＤ）的框架下,得到了相对论线性Ｖｌａｓｏｖ方程．依此计算了球形核１６Ｏ、４０Ｃａ、９０Ｚｒ及２０８Ｐｂ的巨偶极共振的强度函数分布．结果表明,相对论效应是不可忽视的．计算得到的巨共振中心能量稍高于非相对论线性Ｖｌａｓｏｖ方程给出的对应值,与实验结果比较都有较好的符合．对计算结果作了简要的讨论,发现核子有效质量和平均场自旅轨道耦合力对巨共振能量有重要影想． In the framework of relativistic quantum hadron dynamical (QHD) theory,under semiclassical approximation and taking into vacuum fluctuation, a relativistic Vlasov equation (RVE) has been derived. Using RVE and considering other relativistic effects, we have studied the isovector dipole giant resonances built on ground state in spherical nuclei.The main results show that the resonance energies for each multipole are larger than those obtained from the non-relativistic classical Vlasov approach...     

非旋转银河系的重力不稳定性

银河系中星体分布的重力不稳定性在天文物理是个熟知的问题.尝试以加速器物理的方法初步分析了这个现象, 得到非旋转银河系在它的大小超过某阈值时会呈现不稳定现象的结论,而此阈值与银河系的质量密度有关.     

△粒子的相对论BUU方程

在与核子相对论BUU方程相统一的框架内,利用闭合时间回路格林函数方法导出了△粒子的相对论BUU方程,并同时给出平均场与碰撞项的解析表达式.结果表明,核子与△粒子的BUU方程是相互联立的.     

全相对论性Vlasov—Maxwell方程的解析解

本文给出了全相对论性Ｖｌａｓｏｖ－Ｍａｘｗｅｌｌ方程的解析解。该解是Ｓｗａｄｅｓｈ＾［＾１＾］结果的推广，它既适用于高温聚变等离子体，也适用于有相对论漂移速度的等离子体。     

相对论动力学方程的一个简单例解

采用在牛顿力学中常用的方法,用一种简洁的数学形式给出了一维运动情形下受恒力作用的粒子的相对论动力学方程的一个例解,详细讨论了相对论粒子的加速度、速度和运动方程与牛顿力学中对应物理量的区别和联系.     

相对论Dirac方程中矩阵维数的证明

利用Ｄｉｒａｃ方程中α，β矩阵的代数性质，构成Ｄｉｒａｃ群，再用群的性质，证明α，β矩阵一定是４×４矩阵，进而找出Ｐａｕｌｉ－Ｄｉｒａｃ表象中α，β矩阵的具体表示形式。     

狭义相对论中没有“矛盾方程”

根据洛伦兹变换把两个惯性系的坐标原点的时空坐标从一个坐标系变换到另一坐标系,从相对运动的角度说明洛伦兹变换是自洽的,运动物体上发生的自然过程比起静止物体的过程延缓了,并且两个坐标系中的观察者都认为对方的时钟变慢,是“动钟变慢”而非“动钟变快”,不会导致“矛盾方程”,不能混淆同一事件的变换规律与两个事件的变换结果．     

Landau damping of longitudinal oscillation in ultra- relativistic plasmas with nonextensive distribution

The generalized dispersion equation for longitudinal oscillation in an unmagnetized, collisionless, isotropic and relativistic plasma is derived in the context of nonextensive q-distribution. An analytical expression for the Landau damping is obtained in an ultra-relativistic regime, which is related to q-parameter. In the limit q → 1, the result based on the relativistic Maxwellian distribution is recovered. It is shown that the interactions between the wave and particles are stronger and the waves are more strongly damped for lower values of q-parameter. The results are explained by the increased number of superthermal particles or low velocity particles contained in the plasma with the nonextensive distribution.     

非均匀等离子体对强激光传播及电子束输运的影响

本文介绍近期针对非均匀等离子体对强激光传播和电子束输运影响取得的研究进展, 首先研究弱无序分布等离子体对强激光传播的影响, 提出强激光在弱无序等离子体中存在非线性分支流传输机制, 并阐明光电离效应及相对论效应对分支流的重要影响。此外, 研究等离子体密度梯度对相对论电子束输运过程的影响, 发现相对论电子束输运所激发的静电波在空间固定点处的波数或相速度随时间变化, 并且不依赖于等离子体密度的上升或下降, 静电波的局域空间波数最终随时间逐渐增大, 这导致在非均匀等离子体中静电波通过朗道阻尼方式将能量耗散转移给背景电子, 表现为一种由背景等离子体密度梯度引起的束流能量耗散新机制。     

量子等离子体中波的色散关系以及朗道阻尼

利用动理学理论研究量子等离子体中波的色散关系和电子朗道阻尼.从电子的量子流体动力学方程和动理学描述下的光子运动方程出发,研究量子效应对光子朗道阻尼的修正.研究发现量子效应只对纵波模式,即电子等离子体波的色散关系有修正,对横向电磁波的色散关系没有影响.量子效应减小了朗道阻尼,起着朗道增长的作用.关键词：量子等离子体朗道阻尼电子等离子体波色散关系     

Landau damping and inhomogeneous reference states

Landau damping is a fundamental phenomenon in plasma physics, which also plays an important role in astrophysics, and sometimes under different names, in fluid dynamics, and other fields. Its theoretical discussion in the framework of the Vlasov equation often assumes that the reference stationary state is homogeneous in space. However, Landau damping around an inhomogeneous reference stationary state, a natural setting in astrophysics for instance, induces new mathematical difficulties and physical phenomena. The goal of this article is to provide an introduction to these problems and the questions they raise.     

Self-consistency and search for collective effects in semiclassical pairing theory

A simple model, in which nuclei are represented as homogeneous spheres of symmetric nuclear matter, is used to study the effects of a self-consistent pairing interaction on the isoscalar nuclear response. Effects due to the finite size of nuclei are suitably taken into account. The semiclassical equations of motion derived in a previous paper for the time-dependent Hartree-Fock-Bogoliubov problem are solved in an improved (linear) approximation in which the pairing field is allowed to oscillate and to become complex. The new solutions are in good agreement with the old ones and also with the result of well-known quantum approaches. The role of the Pauli principle in eliminating one possible set of solutions is also discussed. The density response function is explicitly evaluated and it is shown that the energy-weighted sum rule is restored to its correct value by a part of the fluctuations of the imaginary pairing field. The remaining part of these imaginary fluctuations, together with the fluctuations of the real part, could give rise to collective excitations in the density response function. A detailed analysis of the monopole and quadrupole strength functions shows that there are practically no collective effects in these channels at low excitation energy.