具有Manning-Rosen势的Schrdinger方程的任意l波束缚态解析解

使用完全量子化规则计算了具有离心项的Manning-Rosen势,根据动量积分∫rBrAk(r)dr-∫r0Br0Ak0(r)dr=nπ和一种新的近似化条件,得到了系统的任意l波Schrdinger方程的解析解和能谱方程.最后简单讨论了l=0和α=0或1束缚态能谱的有关性质.     

任意维l态Woods-Saxon势的精确解析解

在D维空间下使用完全量子化规则计算了具有离心项的Woods-Saxon势的Schrdinger方程,根据动量积分∫xBxAk(x)dx-∫x0Bx0Ak0(x)dx=nπ和Pekeris近似化条件,得到了系统的任意l波Schrdinger方程的解和能谱方程.最后,简单讨论了其跨纬度退化完全能谱的有关性质.     

sl玻色子体系在U（2l＋1）←→0（2l＋2）过渡区的严格解

利用无穷维李代数方法得到了相互作用sl玻色子体系在U（2l 1)←→0(2l 2)过渡区的能谱和波函数的严格解。给出了该系统Bethe假定方程的数值解法。     

任意维l态Woods-Saxon势的精确解

在D维空间下使用完全量子化规则计算了具有离心项的Woods-Saxon势,根据动量积分 (其中 )和Pekeris近似化条件,得到了系统的任意l波Schrödinger方程的解和能谱方程．讨论了束缚态能谱的有关性质．     

任意维l态Woods-Saxon势的精确解

在D维空间下使用完全量子化规则计算了具有离心项的Woods-Saxon势,根据动量积分 (其中 )和Pekeris近似化条件,得到了系统的任意l波Schrödinger方程的解和能谱方程．讨论了束缚态能谱的有关性质．     

具有Manning-Rosen标量势与矢量势的Klein-Gordon方程的任意l波束缚态近似解析解

在球坐标系中研究了具有离心项的Manning-Rosen型标量势与矢量势的Klein-Gordon方程.在标量势等于矢量势的条件下,运用合适的指数近似将具有离心项的径向Klein-Gordon方程转化成超几何微分方程,从而获得了系统的任意l波Klein-Gordon方程解析束缚态径向波函数.最后,对l=0和α=0或1两种特殊情况进行了简单讨论.     

扭振阶梯形变幅杆频率方程的一般表示

利用变截面杆扭报方程和边界条件，导出的扭振阶梯形变幅杆的频率方程，在S1=S2，或l1=l2时，并不适于实际情况．本文首先导出了扭振声传输线方程，并用之对阶梯形变幅杆的频率方程作了一般表示．     

几种扭振复合超声变幅杆的研究

对左、右段为圆柱型、中间段为变截面杆的三段式复合扭振超声变幅杆给出了频率方程和参数计算通式据此得出中间段l2分别为指数型、类国雄型、类悬镇线型和类余弦型，而l1=l3≠0，或l1≠0；或l3≠0的各种组合复合杆的参数计算式，并算出了其参数值，给出了主要参数曲线．测试了十组典型试件的谐振频率和放大系数，实验结果与理论值基本一致，本法可组合成许多适应各种用途的扭振复合杆     

A=15和17原子核单粒能谱的理论计算

根据由格林函数方法导得的满壳层相邻核能谱所满足的方程,在取质量算符（按G矩阵展开）的一级近似下,应用Hamada-Johnston势,计算了A=15核的0s_1/2、0p_3/2、0p（1/2）空穴态和A=17核的0d_5/2、1s_1/2、0d_3/2粒子态能谱与相应的跃迁振幅比,计算中严格顾及了G矩阵的能量相关性。文中对能谱方程自洽求解的收敛速度以及截断近似和选作表象的单粒谐振子势参数对计算结果的影响进行了考察。本文还讨论了质心伪态的消除问题,给出了引入质心谐振子势后计算G矩阵的具体公式。除Os（1/2）态外,本文算得的能谱均消除了质心伪态的影响。与以往重整化的Brueckner-Hartree-Fock（RBHF）计算相比,本文采用的方法计算简单,结果与实验符合颇好。     

几种扭振复合超声变幅杆的研究

对左、右段为圆柱型、中间段为变截面杆的三段式复合扭振超声变幅杆给出了频率方程和参数计算通式据此得出中间段l2分别为指数型、类国雄型、类悬镇线型和类余弦型，而l1=l3≠0，或l1≠0；或l3≠0的各种组合复合杆的参数计算式，并算出了其参数值，给出了主要参数曲线．测试了十组典型试件的谐振频率和放大系数，实验结果与理论值基本一致，本法可组合成许多适应各种用途的扭振复合杆     

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．     

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.     

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.     

干涉仪系统传递函数测量及影响因素的分析

波前功率谱密度(PSD)被用于评价惯性约束聚变(ICF)激光驱动器光学元件中频段的波前误差。干涉仪对PSD较高空间频率分量的测量存在失真效应,可通过干涉仪系统传递函数(STF)的检测标定来获得真实的波前PSD分布。采用台阶板位相比较法测得大口径菲索相移干涉仪检测系统在透射和反射检测情形下的传递函数。对传递函数测试算法进行了比较分析,明确了干涉仪系统zoom倍率的改变等因素对传递函数测量的影响,为波前PSD的准确检测奠定了基础。     

From the Solution of the Tsarev System to the Solution of the Whitham Equations

We study the Cauchy problem for the Whitham modulation equations for increasing smooth initial data. The Whitham equations are a collection of one-dimensional quasi-linear hyperbolic systems. This collection of systems is enumerated by the genus g=0,1,2, ... of the corresponding hyperelliptic Riemann surface. Each of these systems can be integrated by the so-called hodograph transformation introduced by Tsarev. A key step in the integration process is the solution of the Tsarev linear overdetermined system. For each g>0, we construct the unique solution of the Tsarev system, which matches the genus g+1 and g–1 solutions on the transition boundaries.     

On the Problem of the Amenability of the Gauge Group

Let G be one of the local gauge groups C(X, U(n)),C (X, U(n)), C(X, SU(n)) or C (X, SU(n)) where X is a compact Riemannian manifold. We observe that G has a nontrivial group topology, coarser than its natural topology, w.r.t. which it is amenable, viz. the relative weak topology of C(X, M(n)). This topology seems more useful than other known amenable topologies for G. We construct a simple fermionic model containing an action of G, continuous w.r.t. this amenable topology.     

Testing the mechanism for the LSP stability at the LHC

The lightest supersymmetric particle (LSP) is a natural candidate for the cold dark matter of the universe. In this Letter we discuss how to test the mechanism responsible for the LSP stability at the LHC. We note that if R-parity is conserved dynamically one should expect a Higgs boson which decays mainly into two right-handed neutrinos (a “leptonic” Higgs) or into two sfermions. The first case could exhibit spectacular lepton number violating signals with four secondary vertices due to the long-lived nature of right-handed neutrinos. These signals, together with the standard channels for the discovery of SUSY, could help to establish the underlying theory at the TeV scale.     

地球的扁率对卫星运动的影响

指导出地球引力场的势能,分析了卫星的椭圆轨道旋进的现象。     

On the stability of the equilibria of the Rikitake system

In this note we present an analytical study of the stability of the equilibria of the Rikitake system. We prove that the two non-hyperbolic equilibria of the Rikitake system are unstable for all positive values of the parameters.