由刘维尔方程推导玻尔兹曼方程

刘维尔方程是统计物理中基本方程，因而原则上统计物理中许多重要方程都可以由刘维尔方程导出，本文尝试由刘维尔方程推导玻尔兹曼方程．     

拉氏方程,阿贝尔方程的张量推导

本文应用线性代数、张量分析的基本概念说明拉氏方程、阿贝尔方程可以看作是牛顿方程在约束所允许的矢量空间中的协变分量形式，从而在不直接引用虚位移原理的前提下，导出这两个分析力学的基本方程．     

Bargmann–Wigner方程与高自旋场方程

在坐标表象中由Bargmann-Wigner方程导出了便于求解的高自旋场方程,并给出了相应的拉氏函数.     

从Schroedinger方程引申到Dirac方程的一种简单方法

从Schroedinger方程出发，结合自旋的唯象描述、简单的相对论考虑和适当的猜测，写出了Dirac方程的正确形式     

三类非线性演化方程新的Jacobi椭圆函数精确解

应用修正影射法分别求解三类非线性演化方程,即非线性Klein-Gordon方程,mKdV方程和广义Boussinesq方程,得到了一些新的Jacobi椭圆函数展开解,包括Jacobi椭圆函数解、混合Jacobi椭圆函数解、孤子解和三角函数解. 关键词： Klein-Gordon方程 mKdV方程 广义Boussinesq方程 Jacobi椭圆函数     

超导体流体动力学方程

本文从超导体中准粒子和声子的动力学方程及序参量方程出发得到了超导体流体动力学方程,从理论上证明了出现准粒子从浓度小的区域向浓度大的区域反常扩散的可能性以及对于短波涨落的稳定项。 关键词：     

弹性介质的Lagrange动力学与地震波方程

本文将地球介质看作是弹性介质, 从弹性体的Navier方程出发, 建立均匀弹性介质和非均匀弹性介质的分析动力学方程——Lagrange方程, 利用弹性介质的Lagrange方程导出匀弹性介质和非均匀弹性介质的地震波方程, 为用Lagrange分析动力学研究地球介质中地震波传播规律和解决地震勘探中的有关问题提供基础. 关键词： 地震勘探 弹性介质 Lagrange 方程 地震波方程     

Manning-Rosen标量势与矢量势的Klein-Gordon方程和Dirac方程的束缚态

给出了具有Manning-Rosen型标量势与矢量势的Klein-Gordon方程和Dirac方程的束缚态解，其解可用超几何函数表示. 关键词： Manning-Rosen势 Klein-Gordon方程 Dirac方程 束缚态     

几个典型的数学物理方程的物理解读

拉普拉斯方程、 泊松方程、 热传导方程( 扩散方程)和波动方程是大学物理教学中常见的几个典型的微 分方程, 分别涉及到了流体力学、 电磁学、 热学和波动等重点教学内容. 探索了如何用直观明确而容易理解的物理 语言解读这些方程. 从拉普拉斯方程的物理本质出发, 通过改变该方程右端的形式, 分别引出泊松方程、 热传导方 程( 扩散方程)和波动方程, 详细阐述了上述方程与相关物理现象之间的内在联系, 提出了一种关于以上方程的纵 向对比讲授法, 为学生深入理解典型的数学物理微分方程的物理含义提供了可行的思路     

试探方程法及其在非线性发展方程中的应用

提出了一种比较系统的求解非线性发展方程精确解的新方法, 即试探方程法. 以一个带5阶 导数项的非线性发展方程为例, 利用试探方程法化成初等积分形式，再利用三阶多项式的完 全判别系统求解，由此求得的精确解包括有理函数型解, 孤波解, 三角函数型周期解, 多项 式型Jacobi椭圆函数周期解和分式型Jacobi椭圆函数周期解 关键词： 试探方程法 非线性发展方程 孤波解 Jacobi椭圆函数 周期解     

关于"太阳在银河系中所受引力与到银心距离r的关系"的讨论

讨论了银道面内的引力场强分布和太阳在银河系中所受引力与到银心距离r的关系，指出引力场强g并不是与r的平方成反比，这是由于银河系的大小和形状不能忽略造成的．强调了万有引力定律的适用条件．     

On the calculation of the bremsstrahlung in the region of the plasma frequency

On the basis of the classical theory of radiation produced in incomplete Coulomb interaction, a formula is derived for the coefficient of the bremsstrahlung of fully ionized plasma. In the region of rectilinear approximation a comparison is made with the results of the quantum formula derived from the Born approximation. Furthermore, the influence of dispersion upon the emission coefficient is taken into account; some relations for the region of dispersion are given.     

On the predictability of the positions of the convergence zones in the ocean

The disagreement between the experimental and calculated positions of the first convergence zone are known from many publications. The most probable cause for such a disagreement, namely, the incorrect specification of the input data for the calculations, is considered. The lack of simultaneity between the hydrological surveys of the region and the acoustic experiments is emphasized. The experimental data obtained by the author in five ocean regions are presented. These data characterize the diurnal variability of the distance from the source to the nearest boundary of the convergence zone. The relations proposed by different researchers for calculating the sound speed from the temperature, salinity, and hydrostatic pressure are analyzed. It is shown that these relations lead to a substantial difference in the estimated depth dependence of the hydrostatic gradient of the sound speed. The position of the first convergence zone is calculated for the propagation conditions determined by vertical temperature and salinity profiles with the subsequent recalculation of these profiles into sound speed profiles by using eight different formulas known from the literature. It is shown that different formulas lead to different values of the distance to the first zone; this difference is substantially greater than that between the calculations and experiment. The necessity of improving the recalculation relations in view of the experimental data on sound propagation in natural oceanic waveguides, including the data on the actual positions of the convergence zones, is emphasized.     

Dependence of the Intensity of the Spectral Lines and the Composition of the Sample and the Plasma Parameters of the Unipolar Arc

The investigation was made of the dependence of the intensity of Tl, Ga, Mo, Mg, Mn, Sn, Bi, Ni, Zn, Pt and Au spectral lines and the plasma parameters (temperature T, electron concentration n_e, degree of 6 ionnization α) from concentration of lithium additive.     

Extracting the wavefunction of the LSP at the LHC

We consider associated production of squarks and gluinos with the lightest supersymmetric particle (LSP), or states nearly degenerate in mass with it. Though sub-dominant to pair production of color SU(3)-charged superpartners, these processes are directly sensitive to the wavefunction composition of the lightest neutralinos. Exploiting event-shape variables - including some introduced here for the first time - we are able to identify the composition of the LSP by selecting events involving a single high-pT jet recoiling against missing transverse energy. We illustrate the proposed technique on a set of benchmark cases and propose methods for applying these results in more realistic experimental environments.     

Set the controls for the heart of the Sun

In this paper we describe experiments conducted with high-power lasers that are attempting to replicate, for a very short time and in miniature, conditions found in the Sun. Experiments to date have reached conditions in the outer part of the Sun. To reach the Sun's centre requires compression of material to very much greater than solid density and heating to over ten million degrees. To achieve this, a new class of experiments and a new generation of high-power lasers are required.     

On the Question of the Source of the Apokamp

Technical Physics - The object of this work is the apokamp—a new type of plasma jet, which is formed from a bright offshoot emerging at the bending point of a channel of a high-voltage...