修正屏蔽库仑势下二维尘埃等离子体的动力学和结构特性

本文考虑等离子体密度分布变化, 得到了修正屏蔽库仑势的解析解. 数值分析以及分子动力学模拟表明, 在常见实验室参数情况下, 等离子体密度分布变化引起的屏蔽库仑势修正对二维尘埃等离 子体系统的动力学和结构特性影响很小. 在极限参数情况下, 本模型的计算结果表明二维尘埃等离子体系统的扩散能力明显降低, 并且系统组态呈圆形分布. 此外, 本文还研究了实验室常见大小磁场对二维尘埃等离子体系统的影响. 关键词： 修正屏蔽库仑势 二维尘埃等离子体 分子动力学模拟     

钠原子能量的近似计算

用屏蔽库仑势简化了钠原子的哈密顿,用两次微扰法计算了钠原子的能量,结果与实验值符合得较好。     

电磁场矢势和标势从洛伦兹势变换到库仑势的证明

电磁场的标势φ与矢势A具有规范不变性,可以进行规范变换.证明了洛伦兹势经过规范变换成为库仑势.     

求解径向Schroedinger方程解析解的一种方法以及由此延伸的讨论—叠加势基态能级与势参数关系

采用转化法，可得到一系列具有球对称势函数的径向Schroedinger方程的解析解和能级方程。这种方法是用一个恰当的尝试波函数代入Schroedinger方程后，将微分方程变成简单的可解的代数方程组，由此大大简化了运算。本给出了库仑势、库仑势与谐振子势的叠加势以及离子与原子相互作用势的径向Schroedinger方程解析解，并得到能级方程。由于此方法中涉及一个势参数制约关系，为此以叠加势V(r)=-A1r^-1-A2R^-3 A3r^-4为例，讨论其基态能级。得出重要结论：在库仑势上叠加上两项逆幂指数势作用后基态能量将增大，但是并不是单调增大，而是与各项势参数有关。     

库仑势加新环形势的相对论束缚态

在标量势等于矢量势的条件下，获得了库仑势加新环形势的Klein-Gordon方程和Dirac方程的束缚态的精确解. 对于Klein-Gordon方程，获得了精确的能谱方程和归一化的波函数. 对于Dirac方程，给出了精确的能谱方程和归一化的旋量波函数. 关键词： 库仑势加新环形势 束缚态 精确解     

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利用试验势法和平均半径-屏蔽电荷迭代法研究基于解析势的相对论和非相对论屏蔽类氢模型。通过对屏蔽电荷的计算和比较,证实平均半径-屏蔽电荷迭代法无论在效率上还是计算精度上优于试验势法。与More和Faussurier屏蔽类氢模型比较,在电子电离能、离子总能量和电子跃迁能量的计算结果精度方面,基于解析势的相对论性屏蔽类氢模型占有优势。     

有效屏蔽势的能级和波函数

应用点正则变换和路径积分的方法求解有效屏蔽势的能谱和波函数；并且证明有效屏蔽势具有形不变性．从这点出发，可得到有效屏蔽势的能级.     

求解径向Schrodinger方程解析解的一种方法以及由此延伸的讨论--叠加势基态能级与势参数关系

采用转化法.可得到一系列具有球对称势函数的径向Schrodinger方程的解析解和能级方程.这种方法是用一个恰当的尝试波函数代入Schrodinger方程后,将微分方程变成简单的可解的代数方程组,由此大大简化了运算.本文给出了库仑势、库仑势与谐振子势的叠加势以及离子与原子相互作用势的径向Schrodinger方程解析解,并得到能级方程.由于此方法中涉及一个势参数制约关系,为此以叠加势V(r)=-A1r-1-A2r-3+A3r-4为例,讨论其基态能级.得出重要结论:在库仑势上叠加上两项逆幂指数势作用后基态能量将增大,但是并不是单调增大,而是与各项势参数有关.     

Floquet分波法与修饰势的引入研究

在研究激元激光场中电子与库仑势散射时，一般采用FCC藕合方法(Floquet-coupled-channel)并引入修饰势进行求解与计算。本对弱外光场条件下修饰势的引入进行了分析与推导，认为仅当自由电子的颤动半径小于原子尺度时，分数形式的修饰势的引入才是可行的，否则，分数形式的修饰势的引入是不严谨的，尽管修饰势的引入会给求解与计算带来极大的方便与可能。     

Floquet分波法与修饰势的引入研究

在研究激元激光场中电子与库仑势散射时,一般采用FCC藕合方法(Floquet-coupled-channel)并引入修饰势进行求解与计算.本文对弱外光场条件下修饰势的引入进行了分析与推导,认为仅当自由电子的颤动半径小于原子尺度时,分数形式的修饰势的引入才是可行的,否则,分数形式的修饰势的引入是不严谨的,尽管修饰势的引入会给求解与计算带来极大的方便与可能.     

Universal enveloping algebra and differential calculi on inhomogeneous orthogonal q-groups

We review the construction of the multiparametric quantum group ISO_q,r(N) as a projection from SO_q,r (N + 2) and show that it is a bicovariant bimodule over SO_q,r(N). The universal enveloping algebra U_q,r(iso(N)), characterized as the Hopf algebra of regular functionals on ISO_q,r(N), is found as a Hopf subalgebra of U_q,r(so(N + 2)) and is shown to be a bicovariant bimodule over U_q,r(so(N)).

An R-matrix formulation of U_q,r(iso(N)) is given and we prove the pairing U_q,r(iso(N)) — ISO_q,r(N)). We analyze the subspaces of U_q,r(iso(N)) that define bicovariant differential calculi on ISO_q,r(N).     

The construction of c-number fields and their nonlinear equations of motion for quantum many-body fermion systems

A k-dependent state has been constructed from two paris of mutually commuting Fermi-Dirac operators by replacing the Grassmann numbers in the conventional definition of a fermion coherent state. The Heisenberg time-dependent form of this state was then combined with a particular spin state to give a resultant state |G, the spin component containing a series of unknown k-dependent weights. A classical c-number field, φ(r,t), was then defined by an expectation value of the quantum field, ψ, using |G and an energy and time-dependent phase. It is demonstrated that the form of the equation of motion for φ_c(r,t) is identical to that for ψ.     

Relativistic symmetries with the trigonometric Pschl-Teller potential plus Coulomb-like tensor interaction

The Dirac equation is solved to obtain its approximate bound states for a spin-1/2 particle in the presence of trigonometric Pschl-Teller(tPT) potential including a Coulomb-like tensor interaction with arbitrary spin-orbit quantum number κ using an approximation scheme to substitute the centrifugal terms κ(κ± 1)r-2.In view of spin and pseudo-spin(p-spin) symmetries,the relativistic energy eigenvalues and the corresponding two-component wave functions of a particle moving in the field of attractive and repulsive tPT potentials are obtained using the asymptotic iteration method(AIM).We present numerical results in the absence and presence of tensor coupling A and for various values of spin and p-spin constants and quantum numbers n and κ.The non-relativistic limit is also obtained.     

Statistical analysis of the Perseus-Pisces redshift survey: spatial and luminosity properties

We analyze the spatial and the luminosity properties of the Perseus-Pisces redshift survey. We find that the two point correlation function (CF) Γ(r) is a power law up to the sample effective depth ( 30 h⁻¹ Mpc), showing the fractal nature of the galaxy distribution in this catalog. The fractal dimension turns out to be D 2. We also consider the CF ξ(r) and in particular the behavior of the “correlation length” r₀ (ξ(r₀)1) as function of the sample size. In this respect we find, unambiguously, that the luminosity segregation effect is not supported by any experimental evidence. In addition we have studied the galaxian number-density (n(r)) and number-counts (N(m)) in the VL subsamples finding a good agreement with the properties of a fractal distribution. In particular our conclusion is that the n(r) relation permits to extend the analysis of the fractal nature up to a deeper depth than that reached by the CF analysis, and, we find evidence for fractal properties up to the limiting depth of 130 h⁻¹ Mpc. We clarify the role of the small-scale fluctuations in the determination of the galaxy counts. Even in this case the results are in agreement with the previous ones. Finally we have considered the correlations between galaxy positions and luminosities by means of the multifractal analysis. We find clear evidence for self-similar behavior of the whole luminosity-space distribution. These results confirm and extend those of Coleman and Pietronero (1992).     

Electron paramagnetic resonance measurements for (La,Y)2/3(Ca,Ba)1/3MnO3

We have measured the paramagnetic (PM) resonance behavior as a function of temperature for various manganese perovskites (La,Y)_2/3(Ca,Ba)_1/3MnO₃ with an average A-site size r_A basically covering the whole region of ferromagnetic (FM) metallic ground state. We show that at least three regions with different magnetic behaviors can be distinguished by two phase lines: T_onset−r_A and T_c−r_A. For each given r_A, the complete PM and long-range FM behaviors appear above T_onset and below T_c, respectively; while some anomalous PM behaviors appear for the intermediate temperature range of T_onset<T<T_c . A possible magnetic transition process is discussed in order of decreasing temperature from high-T complete paramagnetism to low-T long-range ferromagnetism.     

Spectator fermion binding of bosons

We consider a two-component mixture of charged fermions on neutralizing background with all sign combinations and arbitrarily small mass ratios. In the two-impurity limit for the heavier component we show that the pair forms a bound state for all charge combinations. In the lowest order approximation we derive a closed-form expression for V_eff(r), the binding potential which has short-range repulsion followed by attraction. In the classical limit, when the mass of embedded particles is large, m₂ å m, we can calculate from V_eff(r) also the cohesive energy E and the bond length R of a metallic crystal such as lithium. For lithium metal the lowest-order result is R = 3.1 Å, E = −1.8 eV, while the corresponding experimental values are 3.4 Å and −1.6 eV. The same interaction for two holes on a parabolic band with m₂ > m gives the quantum mechanical bound state which one may interpret as a boson or local pair in the case of high-T_c and heavy-fermion superconductors.     

Ca1−xYxMnO3 manganites: synthesis and ESR characterization

Ceramic samples of Ca_1−xY_xMnO₃ were synthesized by a liquid-mix method obtaining single phase materials, for 0.1x1, with orthorhombic structure. The cell volume increases with x indicating that changes in the Mn electronic state overcomes the progressive diminishing of the (Ca, Y) cationic radius, r_Ca>r_Y. We observed a continuous broadening of the electronic spin resonance line width with x. This is explained in terms of the increasing orthorhombic distortions. We have measured the DC magnetization for the x=1 compound YMnO₃. Our results are compatible with a G-type antiferromagnet with T_N=44 K.     

基于太极形介质柱六角光子晶体禁带特性研究

提出了一种新型的非对称性散射体的二维六角晶格光子晶体结构–-太极形介质柱光子晶体. 利用平面波展开法从理论研究这种光子晶体结构的能带特性以及结构参数对完全禁带的影响. 研究表明:散射体对称性的打破, TE模和TM模能带宽度和数目都会有所增加, 有益于获得更宽的完全禁带以及更多条完全禁带.通过参数优化, 发现在ε = 17, R=0.38 μm, r=0.36R, θ = 0° 时, 获得最大完全带隙宽度0.0541(ωa/2πc); 在ε = 16, R=0.44, r=0.2R, θ = 0°时, 光子晶体完全带隙数目最多达到8条. 关键词： 光子晶体 禁带 平面波展开     

Towards a naturally small cosmological constant from branes in 6D supergravity

We investigate the possibility of self-tuning of the effective 4D cosmological constant in 6D supergravity, to see whether it could naturally be of order 1/r⁴ when compactified on two dimensions having Kaluza–Klein masses of order 1/r. In the models we examine supersymmetry is broken by the presence of non-supersymmetric 3-branes (on one of which we live). If r were sub-millimeter in size, such a cosmological constant could describe the recently-discovered dark energy. A successful self-tuning mechanism would therefore predict a connection between the observed size of the cosmological constant, and potentially observable effects in sub-millimeter tests of gravity and at the Large Hadron Collider. We do find self-tuning inasmuch as 3-branes can quite generically remain classically flat regardless of the size of their tensions, due to an automatic cancellation with the curvature and dilaton of the transverse two dimensions. We argue that in some circumstances six-dimensional supersymmetry might help suppress quantum corrections to this cancellation down to the bulk supersymmetry-breaking scale, which is of order 1/r. We finally examine an explicit realization of the mechanism, in which 3-branes are inserted into an anomaly-free version of Salam–Sezgin gauged 6D supergravity compactified on a 2-sphere with nonzero magnetic flux. This realization is only partially successful due to a topological constraint which relates bulk couplings to the brane tension, although we give arguments why these relations may be stable against quantum corrections.     

Quantum bound states with zero binding energy

After reviewing the general properties of zero-energy quantum states, we give the explicit solutions of the Schrödinger equation with E = 0 for the class of potentials V = −|γ|/r^ν, where −∞ < ν < ∞. For ν > 2, these solutions are normalizable and correspond to bound states, if the angular momentum quantum number l > 0. (These states are normalizable, even for l = 0, if we increase the space dimension, D, beyond 4; i.e for D > 4.) For ν < −2 the above solutions, although unbound, are normalizable. This is true even though the corresponding potentials are repulsive for all r. We discuss the physics of these unusual effects.