超短脉冲光束传输缓变包络近似理论的失效和空间奇异性的形成与消除

研究了单周期或更短的超短脉冲光束在真空中的传输.结果显示,在此情况下缓变包络近似理论已不再有效,其失效的原因是,该理论导致了脉冲光束解的空间奇异性,并使脉冲光束不再具有符合物理意义的光束行为,而通过复解析信号的分析方法可以消除这种空间奇异性.给出了时间波形为Gauss,Hyperbolic Secant和Lorentz的脉冲光束奇异性的计算模拟,并给出了解决这些奇异性的复解析信号解.同样,会发现在脉冲光束超过一定的长度后两种解是一致的.     

超短啁啾脉冲光束空间奇异性的形成与消除

研究了超短啁啾脉冲光束在真空中的传输行为以及在传输过程中时空奇异性的形成. 结果表 明，对于脉冲时间较长（相对于一个光学周期）的超短啁啾脉冲光束，啁啾导致的脉冲光谱 展宽仍然会导致脉冲光束空间奇异性的出现. 脉冲啁啾比脉冲长度对脉冲光束空间奇异性的 出现影响更大. 给出了超短啁啾高斯脉冲光束在不同参数下的数值模拟、空间奇异性出现的 条件等，并用复解析信号理论消除了空间奇异性的出现. 关键词： 单周期 缓变包络近似 奇异性 啁啾脉冲     

自由空间中超短啁啾洛仑兹脉冲光束的空间奇异性

给出了超短啁啾洛仑兹脉冲光束在自由空间中的传输方程，研究了啁啾对洛仑兹脉冲光束空间奇异性的影响．理论及数值模拟的结果表明，由于啁啾的作用，对于脉冲宽度大于一个光波振荡周期的洛仑兹脉冲光束同样存在空间奇异性．在初始位置，啁啾洛仑兹脉冲光束的空间奇异性出现在脉冲的前沿或后沿．当洛仑兹脉冲光束传输以后，啁啾洛仑兹脉冲光束的空间奇异性将更加强烈．     

类贝塞尔脉冲光束传输中的空间诱导色散效应

利用空间诱导色散概念,从理论上研究了等束腰宽度的类贝塞尔脉冲光束在自由空间中传输性质.在一阶近似的情况下,类贝塞尔脉冲光束的空间和时间部分可以做分离变量,空间部分在传输过程中保持类贝塞尔光束传输的特性,而时间波形部分的传输遵循空间诱导色散理论.利用数值模拟方法模拟了 Bessel-Gauss 脉冲光束和elegant Laguerre-Gauss脉冲光束的传输.结果证实,只要传输距离小于类贝塞尔光束的无衍射距离,空间诱导群速度色散理论能够很好地描述类贝塞尔脉冲光束脉冲形状的演化过程.     

超短脉冲复宗量厄米高斯光束

从超短高斯脉冲光束出发,根据复宗量厄米函数的性质,用理论解析推导的方法,给出了一组新的超短脉冲光束的解析解,称为超短复宗量厄米高斯脉冲光束。此脉冲光束解的每个频率分量都是复宗量厄米高斯光束,时间脉冲的形状是任意的,具有相同的衍射距离参量,并且可以描述短于一个光学周期的超短脉冲。对这种超短脉冲光束及其在自由空间中的传输过程进行了较为细致的研究,分析了超短复宗量厄米高斯脉冲光束的轴上光强、光强的横向分布、等衍射性质、脉冲极性反转、脉冲延迟等基本性质。讨论了引入缓变包络近似后出现的时空奇异性。     

超短脉冲复宗量拉盖尔-高斯光束

从超短高斯脉冲光束出发。根据拉盖尔多项式的性质,用理论解析推导的方法。给出了一组新的超短脉冲光束的解析解,称为超短复宗量拉盖尔-高斯脉冲光束。此脉冲光束解的每个频率分量都是复宗量拉盖尔-高斯光束。时间脉冲的形状是任意的,具有相同的衍射距离参量,并且可以描述短于一个光学周期的超短脉冲。对这种超短脉冲光束及其在自由空间中的传输过程进行了较为细致的研究,分析了超短复宗量拉盖尔一高斯脉冲光束的轴上光强、光强的横向分布、衍射性质、脉冲极性反转、脉冲延迟等。讨论了引入缓变包络近似后出现的时空奇异性。     

洛仑兹脉冲光束的复振幅包络解和复解析信号解的比较研究

使用复振幅包络表示式和复解析信号表示式推导了洛仑兹脉冲光束的传输公式. 通过具体数 值计算对脉冲光束的复振幅包络解和复解析信号解在不同带宽时的传输进行了对比研究. 数 值结果表明脉冲光束为窄带时，在传输方向轴中心的一定范围内两种解是一致的，而对于宽 带脉冲光束，复振幅包络解在轴中心较近的距离即表现出奇异性，复解析信号解才是符合物 理意义的表示式. 由数值计算得出了选择脉冲光束研究方法的条件，并从所得公式对复振幅 包络解出现奇异性的现象进行了解释. 关键词： 复振幅包络 复解析信号 窄带脉冲 宽带脉冲     

部分空间相干部分光谱相干厄米-高斯脉冲电磁光束的偏振特性

基于非稳态场的相干理论,对部分空间相干部分光谱相干二维厄米-高斯脉冲电磁光束在自由空间传输时的偏振特性做了详细的数值研究.结果表明,脉冲电磁光束的偏振度分布由光束阶数、光束的空间相关长度、时间相干长度和场点位置等因素共同决定.研究表明,当空间相关长度趋于零或无穷大时,轴上点偏振度趋于一固定值,与光束阶数和场点位置无关....     

发散光束抽运的宽带光参量啁啾脉冲放大系统的理论研究

对发散光束抽运的光参量啁啾脉冲放大器的增益带宽进行了系统的理论研究.采用空间傅里叶变换和四阶Runge-Kutta算法，分别模拟了非衍射极限情况下的高斯光束和空间频谱为矩形的发散光束作为抽运光时的增益曲线.结果表明：不管是在可见光或是在近红外光谱区，用发散光束均可以明显地改善光参量啁啾脉冲放大系统的增益带宽.选取合适的发散角和抽运光强，可以获得高增益、宽谱带的信号光输出. 关键词： 光参量啁啾脉冲放大 增益带宽 发散角 高斯光束     

大气湍流中部分相干聚焦涡旋光束的传输特性

基于广义惠更斯-菲涅耳原理和相位结构函数的平方近似,研究了部分相干高斯-谢尔模型涡旋光束被聚焦后在大气湍流中的传输特性,得到了焦平面上光强解析表达式.利用该表达式,详细研究了该类光束在大气湍流中传输焦平面上的光强分布特性.结果表明：在大气湍流中,随着传输距离的增加,涡旋光束的奇异性逐渐降低.对于拓扑荷大的以及空间相干长度较长的涡旋光束,光束奇异性的保持相对要好.在一定的焦距长度和湍流大气条件下,我们可以通过调整光源的拓扑荷和相干长度控制焦面光强分布和焦斑大小.另外,有一定拓扑荷的涡旋光束可以在一定程度上降低大气湍流对传输光束焦面光强分布的影响.     

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.     

Design and analysis of the tunnel connecting the beamcorridor and the spectrum hall of the CSNS

There is a tunnel connecting the beamcorridor and the target station in the spectrum hall in the CSNS project.The length of the tunnel is about 20 m.The shielding design of the tunnel is very significant for the persons working in the spectrum hall because the tunnel is not covered ed soil for shielding.In order to reduce the dose rate at the exit of the cable ducts,we use the ISIS construction,which is designed with four turnings,as a reference for the tunnel design.The thickness of the shielding is obtained by a simulationwith the Monte Carlo Code FLUKA.The result is compared with the data obtained with Moyer Mode and the reliability of the simulation is proved.This paper provides the basis for the design of the tunnel.     

Design and analysis of the tunnel connecting the beamcorridor and the spectrum hall of the CSNS

There is a tunnel connecting the beamcorridor and the target station in the spectrum hall in the CSNS project. The length of the tunnel is about 20 m. The shielding design of the tunnel is very significant for the persons working in the spectrum hall because the tunnel is not covered by soil for shielding. In order to reduce the dose rate at the exit of the cable ducts, we use the ISIS construction, which is designed with four turnings, as a reference for the tunnel design. The thickness of the shielding is obtained by a simulation with the Monte Carlo Code FLUKA. The result is compared with the data obtained with Moyer Mode and the reliability of the simulation is proved. This paper provides the basis for the design of the tunnel.     

最小偏向角法测三棱镜折射率的相图探究

三棱镜折射率的测量是大学物理实验的重要组成部分,对培养学生的基本实验技能、加深对经典光学理论的理解具有重要作用。本文依据几何光学原理探究了最小偏向角法中在有出射光时最小偏向角与三棱镜顶角、折射率所对应的函数关系,建立了有出射光时入射角、折射率、顶角间以及最小偏向角时折射率、顶角、最小偏向角间的相图,阐明了两相图的物理意义。该研究拓展了三棱镜折射率实验的研究思路。     

T and S dualities and the cosmological evolution of the dilaton and the scale factors

Cosmologically stabilizing radion along with the dilaton is one of the major concerns of low energy string theory. One can hope that T and S dualities can provide a plausible answer. In this work we study the impact of S and T duality invariances on dilaton gravity. We have shown various instances where physically interesting models arise as a result of imposing the mentioned invariances. In particular S duality has a very privileged effect, in that the dilaton equations partially decouple from the evolution of the scale factors. This makes it easy to understand the general rules for the stabilization of the dilaton. We also show that certain T duality invariant actions become S duality invariance compatible. That is, they mimic S duality when the extra dimensions stabilize.     

第一讲微波背景辐射的各向异性、偏振及宇宙电离的历史

文章对微波背景辐射的各向异性、偏振及宇宙电离的历史给出了评述性介绍．从大爆炸理论的预言，到观测的发现，到其各向异性及偏振的探测，微波背景辐射(CMB)向人们揭示了丰富的宇宙学信息．文章在对基本理论作了简单介绍后，着重讲述了最新的CMB的观测结果及其物理意义．特别对微波背景各向异性探测器(Wilkinson Microwave Anisotropy Probe，WMAP)的偏振观测及其对宇宙重新电离的限制给出了较详细的叙述．     

Symmetries and the mass ratio of the electron and muon

A model of symmetries and gauge interactions relating the electron and muon is considered. The model is based on the U_L(1)?U_R(1)?R_L?R_R group where U_L(1)?U_R(1) denotes the chiral e-μ rotation and R_L?R_R the chiral reflection of the electron field. The invariance under this group is spontaneously broken by the vacuum expectation values of scalar fields. A zeroth-order vacuum is found for which the zeroth-order electron mass vanishes, while one-loop corrections lead to a finite $\text{m}{}_{\mathrm{<mtext>e</mtext>}}\text{mμ}$ ratio. The decay process μ → e + γ is strictly forbidden in this model.     

Violations of the Pauli principle and the interior of the sun

The consequences of a violation of the Pauli principle for the physics of the solar interior are explored. It is found that a bound state of two protons becomes possible. This leads to an increase in the rate of hydrogen burning in the sun. Because a very large cross section for this reaction is in clear contradiction with the theory of stellar structure when compared with observations of solar luminosity, radius and mechanical oscillations, stringent limits on a violation of the Pauli principle in the two nucleon system can be given. However, a very small violation of the Pauli principle in the two nucléon system might solve the longstanding solar neutrino problem.     

Operations and performance of the Matera laser station and estimation of the position of the European stations

Summary Since September 1983, the Matera laser station started regular tracking activities with the geodetic satellites Lageos and Starlette. The Matera station operates in co-ordination with the international network of geodetic laser stations, and participates to the NASA Crustal Dynamics Project and to the MERIT Campaign promoted by IAU. The first part of this paper reports on the operational activities at the station and on the performance of the instrumentation. The second part describes the models adopted for data processing and presents the results obtained through the analysis of the Lageos observations acquired from September '83 to August '84. The preliminary estimates of the geodetic co-ordinates of five European laser stations and of their baselines are given. The activity reported in this paper is performed under the contract of Consiglio Nazionale delle Ricerche-Piano Spaziale Nazionale-to Telespazio for Matera laser station operation and performance analysis.