在大气湍流斜程传输中拉盖高斯光束的轨道角动量的研究

大气湍流引起大气折射率随机变化,导致空间不均匀性.拉盖高斯光束在大气湍流中传输时,空间不均匀性会使光子波函数改变,引起轨道角动量的变化.本文讨论了拉盖尔高斯光束在大气斜程传输时,湍流介质改变光子轨道角动量而形成不同的光子态.计算了螺旋谐波各分量所占光束总能量的权重,分析了拉盖高斯光束的轨道角动量的变化规律.     

"一把尘埃出激光"--介绍一种新的无序激光器

文章简略地介绍了新型无序激光的发现和确证过程，以及它产生相干光的机制．这种激光器没有腔镜，代替腔镜起作用的是无序介质中的光子囚禁效应．实验并显示了被囚禁的光子在介质中的分布．通过这种机制还可制成一个微米大小的微型激光器。     

光在随机增益介质中的放大

 结合环形腔理论，运用蒙特卡罗法模拟了光子在介质中的随机行走。研究了倍频Nd:YAG（脉宽6 ns，频率20 Hz）脉冲激光器作为泵浦光，在TiO₂ / 若丹明 B有机增益介质中，散射微粒的颗粒密度和泵浦光面积对随机激光器阈值强度的影响。模拟结果表明：随机激光阈值和光子在增益介质中的随机行走路程长度和光子通过边界返回增益区和非增益区的几率有关。随着泵浦光面积的增加，随机激光器阈值降低；增益介质中散射颗粒密度的增加降低了随机激光器的阈值。     

二维排列共振吸收介质的光学特性研究

从理论上提出了一种二维排列的共振吸收介质阵列，计算了介质阵列的透射、反射与吸收光谱，发现存在着类似一维主动光子晶体中的共振光子带隙，并且这种结构的布里渊区边界点与二维阵列中原子之间的频率共振是产生这种共振带隙的必要条件. 本文还进一步分析了光子带隙与结构参数、二维阵列中原子共振中心以及吸收线宽之间的依赖关系. 关键词： 二维共振吸收介质阵列 布里渊区 光子晶体     

海洋湍流对光子轨道角动量量子通信的影响

本文研究了基于光子轨道角动量的量子通信在水下量子信道中受海洋湍流运动的影响.基于Elamassie等提出的海洋湍流功率谱模型,本文建立了不同海洋湍流参数与光子轨道角动量量子通信的单光子探测概率、信道容量、密钥产生率以及双光子共生纠缠度的定量关系,并利用纠缠光子对的共生纠缠度在海洋湍流中的普适衰减特性进一步研究了轨道角动量纠缠光子对在海洋湍流中的最大纠缠距离.研究结果表明:水下量子通信性能和纠缠光子对的共生纠缠度都随海洋湍流的湍流动能耗散率的增大或温度方差耗散率的减小而降低;温度和盐度因素对海洋湍流贡献的比值对水下量子通信的影响在海水是否稳定分层的条件下具有显著的区别;在通过海洋湍流进行量子通信时,增加信号光子的初始轨道角动量量子数可以提高量子密钥分发的密钥产生率和纠缠光子的纠缠衰减抵抗性.     

二维Kagome格子光子晶体禁带的数值模拟

采用平面波展开法模拟计算了由空气背景中的介质柱构成的二维Kagome格子光子晶体的能带结构，得到了使完全光子禁带最大化的结构参量.计算结果表明:由圆形、正六边形和正四边形三种不同形状锗介质柱构成的Kagome格子光子晶体都出现了完全光子禁带，最大禁带分别为Δ=0.014(ωa/2πc)、Δ=0.013(ωa/2πc)、Δ=0.011(ωa/2πc)发现由圆形和正六边形两种介质柱构成的Kagome格子光子晶体在填充比连续变化的较大的范围内都有宽度较为稳定的完全禁带，且它们具有非常相似的能带结构.     

一维光子晶体的电磁波理论及实现方法

对一维光子晶体的电磁波理论及周期介质中的Bloch波解做了详细的推导,给出了光子晶体中的禁带存在的理论依据,并以此分析了禁带的特征.同时,对一维光子晶体的光学理论做了阐释,并应用于一维光子晶体的设计实践.列举了两个多层周期介质膜的禁带特性.最后对光子晶体的应用和制造前景做了展望.     

具有缺陷结构的三角形二维光子晶体结构参量对本征模的影响

通过有限元数值计算得到并图示了具有缺陷结构三角形二维光子晶体本征频率和介质柱半径、晶格常量以及介质柱介电常量之间的关系.利用这些关系可以在一定的范围内增大介质柱半径而相应减小介质柱介电常量,而本征频率基本保持不变.由于光子晶体结构参量的不同,本征模对应的电磁场在晶体中的分布也不同,图示了电场强度的大小在一些结构中的分布.由此可以掌握光子晶体结构参量对缺陷本征模的影响.     

光子在真空和透明介质中的能量和动量问题

针对光子在真空和进入透明介质后的能量和动量问题进行探讨,探讨光子在透明介质中的微观运动与宏观观测中所定义的光子能量动量关系之间的联系,澄清对光子的能量动量关系和对质能关系认识上所存在的误区。     

由介质球构成的三维光子晶体能带结构的平面波研究

采用平面波展开方法计算由介质球构成的面心立方三维光子晶体的能带结构及透射性质.选 用合适的平面波个数研究了SiO₂蛋白石结构光子晶体的能带及透射性质，并采 用转移矩阵 方法计算了电磁波沿［111］方向的传输特性，两种方法得到的结果相符合.还研究了反蛋白 石结构光子晶体的全带隙.最后，研究了壳层介质球构成的面心立方结构光子晶体的能带特 性，发现在高介质球外面包裹适当厚度的低介电常数介质壳层所构成的光子晶体，可以增大 L点相对带隙宽度50％，并证明了其优化内外半径比值约为0．69. 关键词： 光子晶体 光子能带 平面波展开方法 Core-Shell结构     

Spherical Photon Orbits Around a Kerr Black Hole

Two circular photon orbits are known to exist in the equatorial plane of the Kerr black hole. In this paper, we investigate so-called spherical photon orbits—orbits with constant coordinate radii that are not confined to the equatorial plane. A one-parameter class of solutions is found, which includes the circular orbits as special cases. The properties of these spherical orbits are then analyzed, with the aim of classifying them by qualitative differences in their behavior. Finally, representative orbits from each class are plotted out, including a zero-angular momentum photon orbit and one with non-fixed azimuthal direction.     

Spherical photon orbits around a 5D Myers–Perry black hole

We study the motion of bound null geodesics with fixed coordinate radius around a five-dimensional rotating black hole. These spherical photon orbits are not confined to a plane, and can exhibit interesting quasiperiodic behaviour. We provide necessary conditions for the existence of these orbits, and explicitly compute the radii of circular orbits in the equatorial and polar planes. Finally, we plot representative examples of some of the types of possible orbits, commenting on their qualitative features.     

Gyroscopic Precession and Centrifugal Force in the Ernst Spacetime

The phenomenon of gyroscopic precession in the Ernst spacetime is studied within the framework of the Frenet-Serret formalism. General formulae are obtained for circular orbits. At the same time general relativistic analogues of inertial forces such as gravitational and centrifugal forces are also investigated in the Ernst spacetime. Reversal of gyroscopic precession as well as centrifugal force is considered at the circular photon orbits. These phenomena are examined in the Melvin universe as a special case of the Ernst spacetime by setting the mass parameter equal to zero.     

Compton散射下等离子体中电子相轨道的演化

用KMR模型研究了等离子体中多光子非线性Compton散射下电子相轨道的演化,发现电子与光子进行能量交换后,只有未被俘获电子的相轨道才能从周期性向非周期性、随机型演化,其演化剧烈程度随电子吸收光子数的增大而加剧,随电子与光子碰撞非弹性成分和碰撞前初始速度的增大而迅速减弱,但低于强激光场中的剧烈程度。当电子被光场俘获时,这种演化过程结束并做稳定的运动,光子不再为电子提供能量。     

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用KMR模型研究了等离子体中多光子非线性Compton散射下电子相轨道的演化,发现电子与光子进行能量交换后,只有未被俘获电子的相轨道才能从周期性向非周期性、随机型演化,其演化剧烈程度随电子吸收光子数的增大而加剧,随电子与光子碰撞非弹性成分和碰撞前初始速度的增大而迅速减弱,但低于强激光场中的剧烈程度。当电子被光场俘获时,这种演化过程结束并做稳定的运动,光子不再为电子提供能量。     

Chaotic shadows of black holes: a short review

We give a brief review on the formation and the calculation of black hole shadows. Firstly, we introduce the concept of a black hole shadow and the current works on a variety of black hole shadows. Secondly, we present the main methods of calculating photon sphere radius and shadow radius, and then explain how the photon sphere affects the boundary of black hole shadows. We review the analytical calculation for black hole shadows which have analytic expressions for shadow boundary due to the integrable photon motion system. And we introduce the fundamental photon orbits which can explain the patterns of black hole shadow shape. Finally, we review the numerical calculation of black hole shadows with the backward ray-tracing method and introduce some chaotic black hole shadows with self-similar fractal structures. Since the gravitational waves from the merger of binary black holes have been detected, we introduce a couple of shadows of binary black holes, which all have eyebrowlike shadows around the main shadows with the fractal structures. We discuss the invariant phase space structures of the photon motion system in black hole space-time, and explain the formation of black hole shadow is dominated by the invariant manifolds of certain Lyapunov orbits near the fixed points.     

Random lasing in porous scattering medium

The spectrum behavior evolution and the threshold of random lasing depending on the way of photon walk randomization in an active random medium were investigated. The following three ways of photon walk randomization were implemented: multiple light scattering by corundum and silica particles embedded into a solid polymer solution of dye (astrafloxin), multiple light reflection at sub-millimeter extensive air pores (mean diameter 200 μm) produced in the medium, and the combined action of both these effects. The most effective lasing is observed in the case of an active medium with air pores and scattering particles in the interpore space. Such a combined porous scattering medium acts as a network of dielectric waveguides transmitting effectively the random light. This spatial structure of the random active medium significantly increases the photon path in the medium, thereby promoting photon multiplication due to stimulated emission. In this combined medium the random lasing reveals the narrowest spectrum, the lowest threshold, and the highest density of spectral energy in the spectrum maximum.     

Monte Carlo simulation of photon migration path in turbid media

A new method of Monte Carlo simulation is developed to simulate the photon migration path in a scattering medium after an ultrashort-pulse laser beam comes into the medium.The most probable trajectory of photons at an instant can be obtained with this method.How the photon migration paths are affected by the optical parameters of the scattering medium is analyzed.It is also concluded that the absorption coefficient has no effect on the most probable trajectory of photons.     

Position determination and strong field parallax effects for photon emitters in the Schwarzschild spacetime

Position determination of photon emitters and associated strong field parallax effects are investigated using relativistic optics when the photon orbits are confined to the equatorial plane of the Schwarzschild spacetime. We assume the emitter is at a fixed space position and the receiver moves along a circular geodesic orbit. This study requires solving the inverse problem of determining the (spatial) intersection point of two null geodesic initial data problems, serving as a simplified model for applications in relativistic astrometry as well as in radar and satellite communications.     

Gyroscopic Precession and Inertial Forces in Axially Symmetric Stationary Spacetimes

We study the phenomenon of gyroscopic precession and the analogues of inertial forces within the framework of general relativity. Covariant connections between the two are established for circular orbits in stationary spacetimes with axial symmetry. Specializing to static spacetimes, we prove that gyroscopic precession and centrifugal force both reverse at the photon orbits. Simultaneous non-reversal of these in the case of stationary spacetimes is discussed. Further insight is gained in the case of static spacetime by considering the phenomena in a spacetime conformal to the original one. Gravi-electric and gravi-magnetic fields are studied and their relation to inertial forces is established.