硬X光光电成像系统面密度分辨能力

 针对基于将X光转换成可见光接收的硬X光光电成像系统,研究了系统面密度分辨能力的理论模型,获得了系统面密度分辨能力的上下限的表达式;建立了对硬X光成像系统对面密度分辨能力的测量方法。利用自制面密度分辨率板,实验测量了由射频X光机、转换屏、光纤锥耦合和CCD相机组成的硬X光光电成像系统在不同照射量下的面密度极限分辨能力的上下限值。实验结果与理论分析模型分析趋势一致,在未饱和条件下面密度分辨力上限随着照射量的增加而不断增加,而面密度分辨力下限随着照射量的增加将减小。     

密度的概念及其应用

分析在大学物理课程中密度概念的定义并将密度划分为线密度、面密度和体密度三类,进而对求解与密度有关的问题进行分析和讨论.     

从媒质受力分析其电极化响应与磁化响应的两种等效描述

本文以媒质所受电磁场作用力为纽带,分别从极化电荷分布与电极化强度出发推导媒质所受电场作用力,从磁化电流与磁化强度出发推导媒介所受磁场作用力,不仅可以得到电极化强度与极化电荷体密度的关系以及磁化强度与磁化电流体密度的关系,还可直接得到孤立媒质边界处极化电荷面密度与电极化强度的关系以及磁化电流面密度与磁化强度的关系,故这种方法具有很强的通用性且更易理解.     

双Maxwell分布电子驱动的等离子体

本文给出当电子为双Maxwell分布且电子温度空间均匀时三流体的一个均匀电场解;由它得出的电子,离子特性与实验和数值计算结果基本符合。 关键词：     

大型激光原型装置低燃料面密度诊断技术

由于某大型激光原型装置内爆实验的燃料面密度很低,提出了利用充纯D燃料内爆产生的初级DD中子和次级DT中子的产额比值来诊断燃料面密度的方法。在该原型装置的首轮内爆实验中,利用研制的高灵敏塑料闪烁体探测器对初级DD中子产额和次级DT中子产额进行了测量。通过实验发现,当初级DD中子产额高于108时,可以测得次级DT中子实验数据。建立了均匀内爆模型,用初级和次级中子产额比值法对燃料面密度进行计算,获得的该原型装置首轮内爆实验燃料压缩的平均面密度小于4.0 mg/cm2。     

靶材料面密度用β射线测量的定标问题

 惯性约束聚变靶材料面密度及其均匀性分布可以通过β射线束透射法进行测量,要完成这一测量,需首先用一系列面密度已知、组成成分与待测材料相同的标准材料对测量装置进行刻度。针对惯性约束聚变靶材料一类还处于研制阶段的新材料的密度测量,提出了用成分相近的材料作为替代标准进行刻度的方法,并用蒙特卡罗方法模拟计算了不同能量电子穿过不同材料的透射率,得到了这种刻度方法对测量结果带来的误差大小,用纸作标准测量CH泡沫靶材料的误差只有百分之几,这一误差在实际测量中可以由蒙特卡罗模拟方法得到修正。该刻度方法解决了惯性约束聚变靶材料一类新材料面密度用β透射法测量中的定标问题。     

稳态自洽密度分布的三参量解族

本文利用严格的解析方法求得了激光等离子体中稳态自洽密度分布的三参量解族。讨论几种特殊情况,指出Lee等人给出的平台型密度分布只是其中的一种特殊情况。 关键词：     

利用热纠缠态表象获得Caldeira-Leggett密度算符方程的积分形式解

开放量子系统,即系统-热库模型,可以用一个关于密度算符的主方程来描述,比如,用来描述固态物理中耗散现象的Caldeira.Leggett主方程.虽然已经有人为了求解此主方程的约化密度矩阵的精确表达式而做过一些努力,但迄今还未见有解答.本文使用了一种全新的方法来求解Caldeira-Leggett方程,用这个新方法可以得到积分形式的显式表达.该方法的要点在于利用有序算符内积分技术把关于密度算符的微分方程首先转化成关于密度态矢量的微分方程,再将密度态矢量投影到热纠缠态表象中,Caldeira-Leggett方程就转变成了关于波函数的微分方程,而波函数是函数.这样就可以使用数学中求解微分方程的方法来求解出波函数.再次利用有序算符内积分技术,再将波函数转化为态矢量和算符,就得到了Caldeira-Leggett方程的积分形势解.     

X射线硬化对面密度测量灵敏度的影响

利用蒙特卡罗方法分别研究了3种能量X光机的光子穿透不同厚度铝的硬化情况及3种能量光机作为光源测量面密度的过程,并开展了相关实验研究,根据模拟结果对比分析了不同能量光机X射线硬化对面密度测量灵敏度的影响,结果表明:对同种能量光机的光子而言,随着面密度变大,射线硬化程度越严重,导致测量灵敏度下降;光子能量越低,测量灵敏度随面密度变大下降越快,反之亦然;对于某一范围面密度被测物,调整X光机电压使X光子刚好穿透并形成有效图像,可获得最理想的测量灵敏度。     

球形Dirac方程的空间格点求解及假态问题

本文在空间格点上利用虚时间步长方法求解了球形Dirac方程, 着重研究了出现的假态问题. 利用三点数值导数公式离散方程中一阶导数项, 可以证明对于量子数为 κ 和 -κ的单粒子能级能量是完全相同的, 其中一个为物理解, 另一个为假态. 通过在径向Dirac方程中引入Wilson 项, 可以解决假态问题, 得到全部物理解. 文章以 Woods-Saxon 势为例, 考虑 Wilson 项后, 得到与打靶法一致的结果.     

Determination of atomic positions of point defects in solids by ENDOR

The experimental results which are obtained from electron nuclear double resonance (ENDOR) of point defects in solids are briefly reviewed. From the relation between the experimental superhyperfine and quadrupole interaction tensors and the spin density distribution and charge density distribution, the details of the microscopic structure and thus the positions of atoms can in principle be obtained. For this, in general, a precise theory of the defect wave function is required. However, there are many cases in which simple approximations to the wave function can be used to determine atomic positions rather well. This is illustrated with several examples, mainly from ionic solids. The particular difficulties encountered in semiconductors and the influence of dynamical effects are also discussed.     

Abel inversion using Legendre polynomials approximations

An improved Abel inversion method based on Legendre polynomials approximations is presented for reconstructing the original radial distribution of plasma emission coefficients from projected intensities. The method uses the technique of overlapping two near segments for obtaining an excellent approximation of the intensity distribution. The approximated function of the intensity profile is a combination of various shifted Legendre polynomials which in the Abel inverse equation can be integrated exactly to deduce the emission coefficient. It is shown, using simulated intensity data with and without noise inverted for a comparison with those obtained by other methods, that the method is more accurate and has a better property of noise resistance. It is well suited for applying to experimental intensities distorted by noise.     

风沙稳定输运中起跳沙粒运动状态分布函数

本文用气固二相流模型模拟了风沙稳定输运过程。若起跳沙粒运动状态分布函数采用由实验得到的正态分布函数形式时,计算出的水平质量流量通量随高度的变化规律与实验结果不同。经深入分析,本文提出一新的起跳沙粒运动状态分布函数形式。其中初始起跳角的分布仍采用正态分布函数形式,而对初始起跳速度则采用指数函数和正态分布函数的分段函数形式。计算结果表明本文提出的起跳沙粒运动状态分布函数与实际情况吻合较好。     

200 keV V+注入花生种子深度-浓度分布的蒙特卡罗模拟

在对植物种子靶材料进行处理和对LSS理论进行修正的基础上,用蒙特卡罗方法模拟计算了在一维和二维近似情况下,200 keV V⁺注入花生种子的深度-浓度分布,得到了与实验结果较符合的曲线.并在同样初始条件和理论模型下,计算了200 keV N⁺注入植物种子的深度-浓度分布,为研究低能离子注入植物种子深度-浓度分布提供了一种初步的理论计算方法.     

Density of states of a disordered Hubbard model using the modified moments method

We apply the modified-moments method to compute the density of states of the impurity band of a doped semi-conductor in the intermediate region of impurity concentrations. This method is used to correct the density of states obtained by interpolating between the high and low concentration limit asymptotic expressions. The calculation is based on the Hubbard model in the atomic limit without spin ordering. The overlap integral is assumed to be a Gaussian function of the impurity separation. Use is made of the first seven moments of the exact distribution and of the low and high concentration limit approximations previously calculated. The first six moments are employed to determine the orthogonal polynomial expansion of the density of states while the seventh moment is used as a check on the accuracy of the distribution obtained. The results are similar to the previous ones using a truncated Edgeworth series for the correction term but the present method has the advantage of being a more systematic approach.     

Resummation with Wilson lines off the light cone

I review the resummation formalism for organizing large logarithms in perturbative expansion of collinear subprocesses through the variation of Wilson lines off the light cone. A master equation is derived, which involves the evolution kernel resulting from this variation. It is then demonstrated that all the known single- and double-logarithm summations for a parton distribution function or a transverse-momentum-dependent parton distribution can be reproduced from the master equation by applying appropriate soft-gluon approximations to the evolution kernel. Moreover, jet substructures, information which is crucial for particle identification at the Large Hadron Collider and usually acquired from event generators, can also be calculated in this formalism.     

相对论性带电粒子束在轴对称电场和磁场中的温度和能量展宽

从单粒子的相对论性运动方程出发,首先解出运动常数,然后用这些运动常数构成符合Vlasov方程的束粒子分布函数,再由该分布函数算出轴对称电场和磁场中相对论性带电粒子束的束温度和能量展宽,并且对弱相对论性情况和强相对论性情况作了讨论。 关键词：     

Application of the mutual-interaction method to a class of two-scatterer systems: II. Scatterer near an interface

Abstract

This paper applies the methodology developed in Part I to the problem of a separable scatterer near a dielectric (penetrable) or perfectly conducting (impenetrable) interface. For a penetrable interface, the scatterer may be on either side of the interface (exposed or embedded). As in Part I, the scatterer may also be an active element. Thus, our solutions extend the classic treatments of dipoles radiating near a planar dielectric interface. The mutual-interaction method accommodates a uniform half-space as an equivalent scattering plate of zero thickness that preserves amplitudes and phases of the transmitted and reflected waves. Because this scattering function necessarily includes a Dirac delta function, exact analytic solutions are possible for the class of separable scatterers, which include isotropic scatterers and electric or magnetic dipoles. The results can be interpreted within the context of image theory. Integrals similar to those derived by Sommerfeld must be evaluated to calculate the spatial fields for dielectric media; however, for highly conducting media good approximations are readily obtained.     

Application of the mutual-interaction method to a class of two-scatterer systems: II. Scatterer near an interface

This paper applies the methodology developed in Part I to the problem of a separable scatterer near a dielectric (penetrable) or perfectly conducting (impenetrable) interface. For a penetrable interface, the scatterer may be on either side of the interface (exposed or embedded). As in Part I, the scatterer may also be an active element. Thus, our solutions extend the classic treatments of dipoles radiating near a planar dielectric interface. The mutual-interaction method accommodates a uniform half-space as an equivalent scattering plate of zero thickness that preserves amplitudes and phases of the transmitted and reflected waves. Because this scattering function necessarily includes a Dirac delta function, exact analytic solutions are possible for the class of separable scatterers, which include isotropic scatterers and electric or magnetic dipoles. The results can be interpreted within the context of image theory. Integrals similar to those derived by Sommerfeld must be evaluated to calculate the spatial fields for dielectric media; however, for highly conducting media good approximations are readily obtained.     

STATISTICAL PROPERTIES OF RANDOM SPARSE ARRAYS

Theoretical models that can be used to predict the range of mainlobe widths and the probability distribution of the peak sidelobe levels of two-dimensionally sparse arrays are presented here. The arrays are considered to comprise microphones that are randomly positioned on a segmented grid of a given size. First, approximate expressions for the mean and variance of the squared magnitude of the aperture smoothing function are formulated for the random arrays considered in the present study. By using the variance function, the mean value and the lower end of the range i.e., the first 1 per cent of the mainlobe width distribution, can be predicted with reasonable accuracy. To predict the probability distribution of the peak sidelobe levels, distributions of levels were modelled by using a Weibull distribution at each peak in the sidelobe region of the mean squared magnitude of the aperture smoothing function. The two parameters of the Weibull distribution were estimated from the means and variances of the levels at the corresponding locations. Next, the probability distribution of the peak sidelobe levels were identified by following a procedure in which the peak sideload level was determined as the maximum among a finite number of independent random sidelobe levels. It was found that the model obtained from that approach predicts the probability density function of the peak sidelobe level distribution reasonably well for the various combinations of the two different numbers of microphones and the various grid sizes tested in the present study. The application of these models to the design of random, sparse arrays having specified performance levels is discussed.