二维各向同性谐振子的径向阶梯算符

对二维各向同性谐振子的约化径向薛定谔方程，经变数变换后进行因式分解，以刘径向阶梯算符，并用以计算能量本征值与径向本径函数。     

经典轨道的封闭性和径向Schr?dinger方程的因式分解

研究表明,保证经典轨道具有封闭性的Bertrand定理可以进一步推广,在适当的角动量下,仍存在着非椭圆的闭合轨道．对于屏蔽Coulomb场,可获得广义Runge-Lenz矢量．这种轨道封闭性与径向Schr?dinger方程因式分解相对应．     

高维空间各向同性谐振子的超径向阶梯算符

用因式分解法找出高维空间各向同性谐振子的超径向阶梯算符，给出归一化系数的一般公式，计算能量本征值和超径向本征函数。     

二维与三维氢原子的另外四类升降算子及归一化系数

对氢原子的径向Schrodinger方程,完全用因式分解方法,导出关于主量子数n和角量子数l的另外两类升降算子.用它们构造出第三类、第四类升降算子.并通过计算给出了四类升降算子的归一化系数.     

N维氢原子的另外四类升降算子

从N维氢原子的径向Schrodinger方程出发,完全用因式分解方法,直接导出N(d≥2)维氢原子的另外第一类、第二类升降算子,并用这两类算子构造出新的第三类、第四类升降算子.当d=3和d=2时,得到三维与二维氢原子的升降算子和文献[5,7]中相同.     

二维氢原子径向方程的两种解法

本文利用两种方法求解二维氢原子的径向方程：一是升降算符法，由所定义的关于量子数ｍ的升降算符，给出了径向波函数之间的递推公式，求出了二维氢原子的能级和径向波函数的表达式；二是通过与三维氢原子径向方程的类比，在三维氢原子径向波函数的基础上，直接给出了二维氢原子径向波函数的一般表示式．两种解法所得结果完全一致．     

四元数在建立波动方程中的应用

用四元数对经典的能量，动量关系式进行因式分解，建立起了现今人们已知的所有不同形式的波动方程，这样既表明了不同微观粒子不同的波动方程有着同一个来源，也为建立未知粒子的未知的波动方程提供了可能性。     

K-G方程的因式分解

可以用超对称量子力学方法[1] 很好地处理一维势阱能量正征值问题 ,这都受启于Schrodinger的一维谐振子的因式分解法和能量升、降算符的概念[2 ] ,在此借助因式分解法处理K—G方程 ,并将自然地得到Dirac方程 ,而且自然地说明其性质。     

一类环状非球谐振子势场中相对论粒子的束缚态解

提出了一种新的环状非球谐振子势, 在标量势与矢量势相等的条件下，给出了其Klein-Gordon方程和Dirac方程的束缚态解. Klein-Gordon方程的θ角向波函数以超几何函数表示，径向波函数可用合流超几何函数或广义拉盖尔多项式表示，能谱方程由径向波函数满足的束缚态边界条件得到. Dirac方程的旋量波函数可用Klein-Gordon方程的解构造. 关键词： 环状非球谐振子势 Klein-Gordon方程 Dirac方程 束缚态     

Makarov势的Dirac方程的束缚态解

给出了Makarov型标量势与矢量势相等条件下的Dirac方程的束缚态解. Dirac方程的角向方程用因子分解方法求解，在得出角向波函数的过程中，自然地得到了属于同一本征值的不同角向波函数间的递推操作. 径向束缚态波函数用合流超几何函数表示，束缚态的能量方程可由径向波函数满足的边界条件得到. 关键词： Makarov势 Dirac方程 束缚态 因子分解方法     

CONSERVATION LAWS FOR HEATED LAMINAR RADIAL LIQUID AND FREE JETS

The conserved quantities for the heated radial liquid jet and the heated radial free jet are established by using conservation laws. The flow in a heated radial jet is described by Prandtl's momentum boundary layer equation, the continuity equation and the energy equation. Viscous dissipation is neglected. The multiplier approach is used to derive the conservation laws for the system of three equations for the velocity components and the temperature and three conserved vectors are obtained. The conservation laws for the system of two partial differential equations for the stream function formulation are also computed by the multiplier approach and three conserved vectors are obtained. One of these is a non-local conserved vector for the system. The conserved quantities for the heated radial liquid jet and the heated radial free jet, emitted into a stationary fluid of uniform temperature θ_∞, are derived by integrating the conservation laws across the jet.     

Spin 3/2 Field Equation: Separation and Solution in a Class of Lema?tre–Tolman–Bondi Cosmologies

The spin 3/2 field equation is studied in the general Lema?tre–Tolman–Bondi (LTB) space-time. The equation is separated by variable separation. The angular dependence factors out at the level of the general LTB metric. Due to spherical symmetry the separated angular equations coincide with those, previously integrated, relative to the Robertson–Walker and Schwarzschild metric. Separation of time and radial dependence is possible within a class of LTB cosmological models for which the physical radius is a product of a time and a radial function, the last one being further selected by the consistency condition of the radial equations. The separated time dependence, that can be integrated by series, results essentially unique. Instead the radial dependence can be reduced to two independent second order ordinary differential equations that still depend on an arbitrary radial function that is an integration function of the cosmological model. The generalization of the scheme to arbitrary spin field equation is suggested.     

叶轮S2流面气动半反问题通用解法的改进

经典S2流面方程在应用中,需要根据计算对象是轴流或径流式叶轮,选择求解的主方程,以避免求解中出现不稳定.本文建立了S2流面半反问题的通用方程,能够直接适合多种形式的叶轮.其次,建立S2流面的环量分布方程,使得在设计环量约束条件下,同时满足了库塔条件,而且环量的空间分布更加光滑连续.第三,提出了S2流面生成的方程,达到了S2流面的光滑性及其与流动的一致性.通过在轴流、向心混流两个计算案例的应用,证明了本文方法的可行性.     

Exact Solutions of the Klein-Gordon Equation with a New Anharmonic Oscillator Potential

We solve the Klein-Cordon equation with a new anharmonic oscillator potential and present the exact solutions. It is shown that under the condition of equal scalar and vector potentials, the Klein-Cordon equation could be separated into an angular equation and a radial equation. The angular solutions are the associated-Legendre polynomial and the radial solutions are expressed in terms of the confluent hypergeometric functions. Finally, the energy equation is obtained from the boundary condition satisfied by the radial wavefunctions.     

Separation of Spin 0, 1/2, 1 Field Equations in Lemaître-Tolman-Bondi Cosmological Model with Cosmological Constant

The problem of variable separation of the scalar field equation is approached within the Lemaître-Tolman-Bondi (LTB) cosmological model with cosmological constant Λ. Parametric solutions of the cosmological Newton-like equation of the model are preliminary determined that result factorized in the parameter and in the radial dependence. The result holds on a sufficient condition that relates the two arbitrary integration functions of the model. The condition is of the same type of the one that ensures, in absence of cosmological term, the separability of the spin field equations for spin 0, 1/2, 1. It is then shown that the scalar field equation results automatically separable in the class of LTB models determined. The separated radial equation results independent of Λ, while the separated time equation strictly depends on Λ. The separability of the field equations is then checked to hold, in the same context, for spinor field equation of spin 1/2 and spin 1.     

Scattering of a Klein-Gordon particle by a black hole

By using the curved space-time Klein-Gordon equation, the form of the wave function of a scalar particle near a nonrotating black hole is obtained. It is shown that although the radial wave function oscillates infinitely rapidly near the black hole, the probability density remains finite even on the event horizon. This is consistent with the fact that the Schwarzschild surface is nonsingular. An expression is given for the large angular momentum scattering differential cross section by comparing the asymptotic form of the radial wave equation with the corresponding Coulomb radial wave equation in ordinary quantum mechanics.     

基于三维Fokker-Planck方程的电子回旋波加热与电流驱动模拟

利用反弹平均的三维Fokker-Planck方程,对电子回旋波加热和电流驱动进行数值模拟.考虑超热电子径向扩散对电流驱动的影响,在方程中加入径向扩散输运项,采用九点格式的中心差分对方程进行数值离散得到系数矩阵,采用不完全LU分解对系数矩阵进行预处理,利用双共轭梯度稳定法求解得到分布函数.在不考虑电子径向扩散输运条件下,得到电子回旋波驱动电流密度与功率沉积密度的分布;考虑径向扩散输运的计算结果与BANDIT3D进行比较,驱动电流分布的趋势基本一致.     

Radial integrals, oscillator strengths, and polarizabilities of the thallium, lead and bismuth atoms

The radial integrals for transitions of 6p-electrons to the excited states in the Tl, Pb and Bi atoms have been found by numerical integration of the Dirac equation with an effective potential. The radial integrals for excitation of 6s- and 5d-electrons from the closed subshells have been obtained from analysis of the available experimental data on the oscillator strengths in Tl, Hg, Au and the polarizability of Hg. Using these radial integrals, we determine the polarizabilities of the Tl, Pb and Bi atoms by a simple method that is similar to Sternheimer's method.     

Solution of the Dirac equation in the tridiagonal representation with pseudospin symmetry for an anharmonic oscillator and electric dipole ring-shaped potential

An anharmonic oscillatory potential is proposed in which a noncentral electric dipole is included. The pseudospin symmetry for this potential is investigated by working in a complete square integrable basis that supports a tridiagonal matrix representation of the wave operator. The resulting three-term recursion relation for the expansion coefficients of the wavefunctions (both angular and radial) are presented. The angular/radial wavefunction is written in terms of Jacobi/Laguerre polynomials. The discrete spectrum of the bound states is obtained by the diagonalization of the radial recursion relation. The algebraic properties of the energy equation are also discussed, showing the exact pseudospin symmetry.     

强光场下电子与库仑势散射及多光子过程

对Schr?dinger方程引入修饰势,并将波函数展开为Floquet分波,即可实施分离变量。强光场时弱耦合法选取合适微扰量,径向波动方程可逐步近似求解。以圆极化强光场为例,计算了散射波函数、散射矩阵和截面。重要结论是:强光场下将出现多光子过程,对应m次多光子过程有相应的共振谱线族,谱线能量约为m?ω,并给出谱线强度计算公式。 关键词：