Vaidya-Bonner时空中荷电Dirac粒子的Hawking辐射

在Vaidya-Bonner时空中对荷电Dirac旋量粒子的动力学行为进行了研究,得到荷电Dirac方程的径向部分在黑洞视界附近的渐近解,并且准确地定出了带电蒸发黑洞的事件视界、Hawking温度以及Dirac粒子的Hawking辐射谱。从而为处理动态黑洞辐射反作用问题提供了一种新的方法。     

强磁场中无自旋和自旋粒子的Synchro-Curvature辐射谱

Synchro-Curvature辐射是张家铝和郑广生最近提出的一种新的、更普遍的辐射机制,它全面描述了一个相对论性带电粒子在弯曲磁场中运动时所产生的辐射特征.这种新辐射机制概括了通常同步辐射及曲率辐射的全部经典结果,揭示了其间的有机联系和统一性.并为精确讨论脉冲星研究中的辐射问题给出了普遍而简单的统一公式.不过由于脉冲星磁场已高达10⁸T,量子效应不能不考虑,应用最近Lieu和Axford发展的GFWW方法推广了张家铝和郑广生的结果,对无自旋的K-G粒子及有自旋的Dirac粒子给出了其相应的Synchro-Curvature量子辐射谱公式,并讨论了它们的辐射特性.     

正弦平方势及其面沟道辐射的一般特征

本文用经典电动力学方法,在一般情况下导出了带电粒子面沟道辐射的谱分布,讨论了沟道和准沟道粒子对辐射的贡献。利用我们曾经提出的正弦平方势,解析地处理了辐射谱的一般特征,计算了正电子沿硅单晶(110)面沟道辐射的最大能量和谱分布。将理论同实验进行了比较,发现二者符合很好。     

对稳态NUT- Kerr-Newman黑洞的量子隧穿特征的研究

运用Parikh的量子隧穿模型, 研究了NUT- Kerr- Newman黑洞的量子隧穿辐射特征. 研究结果表明, 当考虑能量守恒与角动量守恒时, 稳态NUT- Kerr- Newman黑洞的真实谱不再是纯热谱, 视界处粒子的隧穿率与Bekenstein-Hawking熵有关, 且满足量子力学中的幺正性原理.     

控制论在现代物理中应用伪位势理论与孤粒子理论

§1 引言本文系应用 Galilean 度规变换及 Galilean 度规微分算子变换,将 KDV方程、SG 方程和 NLS 方程化为广义的牛顿近似方程;从而引出了各种类型的伪位势函数.给出了伪位势函数与孤粒子解之间的明确关系,它说明了孤粒子解的出现是由位势所确定的.这可能意味着孤粒子解的真正物理意义!同时,我们还将证明位势与谱在数学结构上的明确形式.另外,我们还讨论由位势的作用,求出高斯分布的广义力学体系以及黑体辐射的 Planck公式的黑体辐射空间中的广义力学体系.这里的“势”可以看作是宇宙里的存在的控制.     

等离子体中磁单极子的辐射和能量损失

本文对磁单极子在等离子体中的辐射和能量损失作了仔细的研究,文中推导出产生磁单极子辐射的一般公式;获得了与荷电粒子颇不相同的Cerenkov辐射功率和谱;求出了在宇宙等离子体中和金属内它的能量损失。并指出,基于等离子体在普通介质中的Cerenkov辐射,因此可用来检测磁单极子的可能性。     

多成分密集随机散射粒子多层随机介质的辐射传输

本文研究有多种成分和大小分布的密集随机分布的球形散射粒子多层随机介质的辐射传输.数值地讨论了冰雪等效球形粒子的大小分布及其有效平均值.由Gauss求积法离散坐标的特征值-特征矢量法,求解两个密集散射粒子层的矢量辐射传输方程和四个耦合的边界条件,得到极化的辐射亮度温度,以及和各有关参数之间的定量函数关系.并与干雪和湿雪的遥感数据进行了比较和分析.     

确定球对称动态时空与平面对称动态时空Hawking效应的普适方法

本文建议了一种普遍适用的研究动态球对称或动态平面对称时空中Hawking效应的新方法,并给出其理论依据.在广义乌龟坐标交换下,Klein-Gordon方程在视界附近一定会化成波动方程的标准形式,从而自动得出决定事件视界位置的方程及Hawking辐射温度.在弱辐射情况下,其结果的一级近似与考虑辐射反作用得到的近似结果完全一致.     

一层空间非均匀的随机介质的二维热辐射传输

本文讨论一层空间非均勻的随机散射元介质的二维热辐射传输方程的求解。由Fourier变换和矩阵表示,可得到一维的Stokes矢量谱函数的辐射传输方程。利用小反照率近似的迭代法求解,得到辐射传输积分方程的零阶解和一阶解。对散射粒子分数体积比具有Gauss形式的非均勻分布的大气雨、云、植被的垂直和水平极化的辐射亮度温度给出了数值结果;并对辐射亮度温度与散射元不均匀分布、波长、极化、下垫界面的介电特性等关系进行了讨论。     

偶极磁场中的SVC辐射模型及其随磁场变化的辐射——Ⅱ.SVC辐射机制及其辐射随磁场变化

本文计算了太阳射电缓变成分(SVC)的射电辐射,着重研究了由联合辐射机制产生的SVC辐射的主要辐射特性(亮度分布、亮温度谱、流量密度谱、偏振度谱)和SVC辐射源的几何特性(高度和半径),及其随磁场强度的变化。     

有限域上的逻辑函数与其Chrestenson谱的关系

本文首先给出了有限域上逻辑函数的Chrestenson线性谱的新定义(不同于文献[1]所给出的),如同Chrestenson循环谱一样,重新定义的Chrestenson线性谱也是有限域Fq到复数域的映射,且证明了它们之间在实质意义下可以相互线性表出;最后我们还用重新定义的Chrestenson线性谱给出了有限域上逻辑函数的反演公式.     

Beurling’s theorem for functions with essential spectrum from homogeneous spaces and stabilization of solutions of parabolic equations

The results of the paper are obtained for functions from homogeneous spaces of functions defined on a locally compact Abelian group. The notion of Beurling spectrum, or essential spectrum, of functions is introduced. If a continuous unitary character is an essential point of the spectrum of a function, then it is the c-limit of a linear combination of shifts of the function in question. The notion of a slowly varying function at infinity is introduced, and the properties of such functions are considered. For a parabolic equation with initial function from a homogeneous space, it is proved that the weak solution as a function of the first argument is a slowly varying function at infinity.     

Initial transient detection in simulations using the second-order cumulant spectrum

Procedures for detecting an initial transient in simulation output data are developed. The tests use the second-order cumulant spectrum which differs from the power spectrum in that the stationarity constraint is not required for the former. The second-order cumulant spectrum can be interpreted as the nonstationary power spectrum and is an orthogonal decomposition of the variance of a nonstationary process. The null hypothesis is that the simulation output data series is a covariance stationary process. Equivalently, all estimates of the second-order cumulant spectrum in the region which excludes the estimates of the power spectrum will have an expected value of zero. The test procedures are designed to detect initialization bias in the estimation of the mean and the variance. These procedures can be extended to detect bias in the moments of cumulants of ordern, wheren>2. Results are presented from the application of the test to simulated processes with superimposed mean and variance transients and anM/M/1 queue example.     

Wavelets Techniques for Pointwise Anti-H?lderian Irregularity

In this paper, we introduce a notion of weak pointwise H?lder regularity, starting from the definition of the pointwise anti-H?lder irregularity. Using this concept, a weak spectrum of singularities can be defined as for the usual pointwise H?lder regularity. We build a class of wavelet series satisfying the multifractal formalism and thus show the optimality of the upper bound. We also show that the weak spectrum of singularities is disconnected from the casual one (referred to here as strong spectrum of singularities) by exhibiting a multifractal function made of Davenport series whose weak spectrum differs from the strong one.     

Remark on the k-Space Problem for Complex Spaces

An example is given of a complex space (X,O) whose continuous spectrum S_c((O(X)) is not a k-space, thereby showing that the Gelfand topology on the spectrum can be different from the strong topology as well as from the direct limit topology.     

Analysis of deformations of the Earth's crust by laser interferometers

Results of measurement of phugoid oscillations of the Earth by a laser interferometric complex, which contains two interferometers of Michelson type, are given. Using the results of 900 h of processing, the spectrum of oscillations of the Earth in the range of periods from 20 to 310 min is obtained as well as the spectrum of free oscillations of the Earth in the seismic quiet time. The multiplet spectrum of oscillations of the Earth in the interval of 160 min is isolated.Translated from Dinamicheskie Sistemy, No. 9, pp. 60–65, 1990.     

On the Bifurcation of a Random Spectrum of Weakly Nonlinear Deep-Water Gravity Waves

The bifurcation of a narrow-band homogeneous random spectrum of deep-water gravity waves into an inhomogeneous random spectrum is studied under the assumption of weak nonlinearity. The modulational wavenumber for the bifurcation depends on the characteristic bandwidth of the spectrum as well as on the energy of the spectrum. The stability of the bifurcated spectrum is examined.     

Minimum-Variance Multitaper Spectral Estimation on the Sphere

We develop a method to estimate the power spectrum of a stochastic process on the sphere from data of limited geographical coverage. Our approach can be interpreted either as estimating the global power spectrum of a stationary process when only a portion of the data are available for analysis, or estimating the power spectrum from local data under the assumption that the data are locally stationary in a specified region. Restricting a global function to a spatial subdomain—whether by necessity or by design—is a windowing operation, and an equation like a convolution in the spectral domain relates the expected value of the windowed power spectrum to the underlying global power spectrum and the known power spectrum of the localization window. The best windows for the purpose of localized spectral analysis have their energy concentrated in the region of interest while possessing the smallest effective bandwidth as possible. Solving an optimization problem in the sense of Slepian (1960) yields a family of orthogonal windows of diminishing spatiospectral localization, the best concentrated of which we propose to use to form a weighted multitaper spectrum estimate in the sense of Thomson (1982). Such an estimate is both more representative of the target region and reduces the estimation variance when compared to estimates formed by any single bandlimited window. We describe how the weights applied to the individual spectral estimates in forming the multitaper estimate can be chosen such that the variance of the estimate is minimized.     

Epimorphisms of rings,interpretations of modules and strictly wild algebras

Abstract It is shown that an epimorphism from a ring R to a ring S induces an embedding of the Ziegler spectrum of S as a closed subset of the Ziegler spectrum of R.     

On the essential spectrum of ideal magnetohydrodynamics. Dedicated to harold grad on the occasion of his sixtieth birthday

The essential spectrum of magnetohydrodynamics (MHD) is shown to arise from waves propagating one-dimensionally along magnetic field lines. Different polarizations of these waves give rise to the “Alfven” and “ballooning” spectra. The essential spectrum of an axisymmetric equilibrium when a single azimuthal mode number is considered consists of the Alfven spectrum only, while the ballooning modes appear as intervals of accumulation of discrete eigenvalues with different mode numbers. We derive some necessary and one sufficient conditions for stability and show some examples where the criteria coincide to yield a simple condition for stability.