反质子与原子核弹性散射的分析

用反质子与核的光学势分析了反质子入射能量为50MeV和180MeV时¹²C,^16,18O,⁴⁰Ca和²⁰⁸Pb核的弹性散射微分截面.讨论了反质子光学势是强吸收型的特点.从寻找最佳符合实验的光学势分析中发现:弥散参数a的可变性很小,且它随核的增大而增大.光学势的实部是一个浅位.光学势在核中的吸收系数趋于零,因此弹性散射主要发生在核的表面.     

镜核间的反质子与核的电荷交换反应

研究镜核之间的反质子与原子核的电荷交换反应. 在扭曲波冲量近似下,用严格的分波法分析反质子能量是179.7MeV和46.8MeV下¹³N(p,n)¹³C和¹⁵O(p,n)¹⁵N可能到达的能态的微分截面. 并指出同位族相似态跃迁与非相似态跃迁的差异.     

中能区反质子与核的非弹性散射

运用多次散射理论的光学势获得反质子的扭曲波.在扭曲波冲量近似下,讨论了中能区反质子与原子核的非弹性散射.考虑了反质子能量从180MeV到1800MeV这一能区¹²C,的2+,3-态微分截面.在这一能区的低能端,(E=180MeV)DWIA能够很好的符合实验,同时,预示了更高能量可能出现的微分截面的理论结果.     

中能区反质子与原子核的弹性散射

运用实验的pN散射振幅和多次散射理论,在冲量近似下考虑反质子能量从180MeV至1800MeV的光学势,发现此能区反质子光学势的虚部强度在130—140MeV附近.用所获得的光学势,计算¹²C,²⁶O,⁴⁰Ca和²⁰⁸Pb等满壳层核在五个能量下的弹性散射微分截面.看到所用的光学势,在180MeV能很好地符合实验数值.本文还预示了此能区在各个核上的理论结果.     

反质子与核的电荷交换反应和非弹性散射

在扭曲波冲量近似下,讨论了反质子与核的电荷交换反应A(p,n)B和非弹性散射A(p,p′)*A.并具体地计算能量为E_p=179.7MeV和46.8MeV下¹²C(p,n)¹²B,¹⁸O(p,n)¹⁸N和¹⁸O(p,p′)¹⁸O的微分截面.用严格的分波法处理扭曲波.非弹性散射的微分截面能符合实验.同时预示了在这些能量下,反质子与核发生电荷交换反应可能出现的微分截面理论结果.     

反质子与原子核的非弹性碰撞

在扭曲波冲量近似的框架下,本文讨论了A(p,p)A非弹性碰撞.并具体地计算了能量为46.8MeV和179.7MeV的¹²C(p,p)¹²C的 2⁺,3^－态微分截面.用严格的分波法处理扭曲波.计算表明,反质子非弹性过程用DWIA是一个好的近似.同时,讨论了束缚态行为的重要性.由于反质子受核的强吸收原因,要求具有准确的核外束缚态波函数.     

反质子与核非弹性碰撞中的自旋效应

A(p,p)A*非弹性碰撞过程,若反质子的光学势包含了自旋轨道耦合势,它在碰撞过程中不但能激发正常宇称态,也能激发反常的宇称态,以及非弹性过程的极化度.本文在DWIA框架下导出了微分截面(dσ/dΩ)_f,i,极化度P(θ).并对入射能量为46.8MeV和179.7MeV ¹²C(p,p)¹²C*的2⁺,3^－和1⁺态微分截面、极化度进行严格的分波方法计算.计算与实验符合很好.由于反常宇称态的非弹过程已被测得,表明反质子光学势的自旋效应不容忽视.     

三种NN湮没势和p+ 12C非弹性散射

在Glauber多重散射理论框架下,使用跃迁密度方法和3种NN湮没势,计算了入射动量为600MeV/c的反质子在¹²C上的非弹性散射微分截面.理论曲线与实验数据符合得甚好     

过程J/ψ→p+X,X→Δ+π产生重子共振态X的研究

利用螺旋度角分布分析和推广的矩分析方法,讨论了J?ψ衰变过程J/ψ→p+X,X→Δ+π,其中p和Δ分别是反质子和自旋–宇称为(3/2)⁺的Δ重子,给出了相应于自旋–宇称为(1/2)^±,(3/2)^±和(5/2)^±的重子共振态(包括混杂重子态)X的角分布和矩表达式.它们可以用来确定重子共振态X的自旋.     

在大气深度x=700克/厘米2处反质子的垂直流强

在大气深度x=700克/厘米²处,利用高能加速器数据计算了产生的反质子的垂直流强。与实验结果比较表明:直到E₀=10⁵GeV的初级宇宙线能量,pN碰撞产生反质子的规律是与高能加速器能区上pp碰撞产生反质子的规律一致的。     

雷达波段内磁性吸波颗粒光散射特性分析

针对目前在微波雷达隐身技术中广泛运用的吸波材料颗粒,根据米氏(Mie)散射理论对磁性吸波颗粒在雷达波段内的光散射特性进行了数值模拟和计算分析.在Mie系数中引入磁导率变量,分别计算了磁导率、折射率及颗粒粒径等参数对吸波颗粒光散射特性的影响;同时对比分析了磁性与非磁性吸波颗粒的散射光强、散射系数、吸收系数等散射特性规律.数值计算结果表明,颗粒磁特性的变化对其散射性能造成影响,磁导率的增大将使颗粒的吸收性能增强而后向散射强度减弱,有利于吸波颗粒雷达散射截面的减小,同时磁导率变化对颗粒散射特性的影响受到复折射率的制约.     

离轴球形粒子对高斯波束的散射光通量的计算

利用矢量球谐函数展开的方法,研究了离轴球形粒子对椭圆高斯波束的散射。根据其远区散射场的形式,得出了归一化散射场的斯托克斯参量(散射强度)与颗粒直径、折射率以及散射角的关系。建立了计算离轴球形粒子对高斯波束散射通量的解析模型,计算了散射光在任意散射方向上的光通量,得到了前向任意立体角内散射通量的计算公式,为激光散射探测提供了理论依据。     

激光散射场理论及其应用

在薄层散射的基础上，研究了寻常散射和非常散射的差别，建立起了散射椭圆的模型。然后从薄层散射过渡到厚层散射，检测了激光在水中的散射场和退偏振度，并对前向散射和后向散射导出了简化的场强计算公式：公式中的常数一散射率成为评价激光散射场和退偏振的依据。本研究的结论直接对提高水中目标探测的信噪比有现实意义。     

Scattering of Mathieu beams by a rigid sphere

Based on the recent results on the scattering of Bessel beams by a sphere and using the Whittaker integral, the scattering by a rigid sphere centred on a Mathieu beam is derived. The scattering field is expressed as a partial wave series involving the scattering angles relative to the beam axis and Mathieu beam parameters. Some numerical calculations are performed and it is shown that the illumination of a rigid sphere by a Mathieu beam produces asymmetrical scattering as a function of scattering angles θ and ?. The geometrical properties of the scattering Mathieu beam are noted.     

On the electronic structure of liquid metals

We consider the electronic structure of liquid metals as a problem of multiple scattering. The total scattering operator is developed in terms of the reaction operators of a single scattering event, having a ‘standing wave’ boundary condition. This method has several advantages with respect to the approach where the total scattering operator is developed in terms of the scattering operators of a single scattering. Since the reaction operators are hermitian, the occurring perturbation expansions have a real perturbation parameter, which is more easily handled. Furthermore, if in the expansion of the total scattering operator, only terms up to the second order are maintained, this approximate expression satisfies already the ‘optical theorem’, just as the exact total scattering operator. Finally, spurious damping terms are eliminated at the outset. For very dense systems we obtain practically non-attenuated waves and this can be understood as if the damping due to a single scattering event is compensated by the reaction of the surrounding scatterers.     

α粒子散射实验的理论模拟

本文在α粒子一次散射理论的基础上,进一步考虑了第二个原子对散射概率的贡献,建立了散射角与各散射参数间的关系.通过改变α粒子的入射能量以及两原子的位置参量,较好地模拟了各种情况下的散射概率随散射角的分布情况.     

Evaluation of numerical scattering in finite volume method for solving radiative transfer equation by a central laser incidence model

The numerical scattering caused by spatial discretization in finite volume method is discussed. Based on an analysis of the generation process of numerical scattering, a physical model of central laser incidence to a two-dimensional rectangle containing semitransparent medium is established to validate the numerical scattering, with Monte Carlo method as benchmark, in which numerical scattering does not exist. Numerical scattering will be affected by spatial grid number, spatial differential schemes and spectral absorption coefficient. With the spatial grid number increasing, numerical scattering will be decreased. The accuracy of the diamond scheme is the highest, and the exponential scheme is a bit lower, the lowest accuracy of the three schemes is the step scheme. The tendency of numerical scattering is reverse, i.e., the step scheme produces minimum numerical scattering, and exponential scheme produces more, while the diamond scheme produces maximum among three methods. When the bias of absorption efficient is high, the numerical scattering cannot be eliminated only by increasing the grid number. If we set the direction of laser incidence as central axis, it can be seen that numerical scattering distributed symmetry along the axis, which can be called as symmetrical cross-scattering. All of the three schemes show symmetrical cross-scattering.     

皮肤组织可见与近红外Mie散射光学特性分析

依据Mie单次散射理论, 并考虑到皮肤组织复折射率实部的色散, 分析了在可见与近红外波段皮肤组织对光的吸收、散射及散射的方向特性。研究表明, 散射系数和吸收系数均随皮肤组织中散射粒子半径的增加而增加, 而且, 对于大粒子, 在某一波长处表现出强烈的散射和吸收特性。当粒子半径大于临界半径时, 散射系数呈现振荡特性, 随着折射率虚部的增加, 振幅减小。皮肤组织呈现前向散射特性, 且散射粒子的半径越大, 前向散射特性越明显。     

光纤中拉曼散射回波超高灵敏度探测技术研究

与布里渊散射不同,石英光纤中斯托克斯拉曼散射与光纤所受应力无关,只是绝对温度的函数,而且其拉曼频移为1.395×1013 Hz, 比布里渊散射易于提取,作为分布式光纤温度传感器的传感信号有一定的优势,但斯托克斯拉曼散射信号比布里渊弱,其峰值功率在APD中产生的光电流在nA级,低于APD的噪声电流,经光电转换后信号的信噪比小于1,傅里叶变换以及小波变换都无法有效地处理这类信号。通过对斯托克斯拉曼散射信号进行特征分析后,采用累加与小波降噪的综合方法提取该信号,实现在APD噪声电流以下的超灵敏度探测,达到每度0.104 nA的温度灵敏度,低于本系统所有APD噪声电流2.3 nA的1个数量级。     

Practical methods to define scattering coefficients in a room acoustics computer model

To predict acoustics of rooms using computer programs based on geometrical assumptions, it is important that scattering is included in the calculations. Therefore scattering is usually included in terms of scattering coefficients which are assigned to each surface telling the software the ratio between the part of the reflected energy which is not being reflected specularily and the total reflected energy. However the effective scattering coefficient of a surface depends not only on the roughness of the surface material indeed diffraction caused by limited dimensions of the surface as well as edge diffraction also causes scattering. For complex rooms it can be difficult to give a reasonable estimate to the magnitudes of scattering coefficients if these should also include diffraction and even if these frequency dependent coefficients could be obtained in the design phase, the processes of obtaining the data becomes quite time consuming thus increasing the cost of design. In this paper, practical methods to define scattering coefficients, which is based on an approach of modeling surface scattering and scattering caused by limited size of surface as well as edge diffraction are presented. The predicted and measured acoustic parameters in real rooms have been compared in order to verify the practical approaches recommended in the paper.