基于有限元的平面光波导粘接热应力分析

基于有限元理论对阵列光纤和波导芯片粘接情况进行了建模与仿真,分析了在温度变化下不同粘接区域厚度的热应力和微位移的产生和分布,结果表明粘接界面的边缘区域对温度变化最敏感.根据光弹效应定性分析了粘接区域的应力双折射,并利用光束传播法计算了由此微位移所导致的光功率损耗,结果表明若以附加损耗小于0.15 dB的标准考察,则必须要求粘胶厚度的理论值在16 μm以内.总结了温度变化和在相同条件下不同粘胶厚度对平面光波导封装性能的影响规律.     

微环耦合谐振光波导中的色散控制模型与数值仿真

本文利用传输矩阵法得到了微环耦合谐振光波导的色散关系,讨论了耦合损耗、传输损耗及耦合系数对微环耦合谐振光波导色散的影响,改变耦合损耗、传输损耗及耦合系数可控制其色散曲线的形状、位置、以及带宽,色散曲线的变化及控制对微环耦合谐振光波导在滤波、光信号延迟及缓存等方面的应用有重要意义. 关键词： 光波导 微环光波导 传输矩阵法     

低群速度色散和低损耗的二维光子晶体慢光波导

利用平面波展开(PWE)法分析了慢光在由介质柱和空气背景构成的二维三角晶格光子晶体耦合微腔波导中的传播特性.数值模拟结果表明:随着缺陷腔之间距离的增大,导模的群速度减小很快;兼顾色散和损耗的影响,当相邻微腔间距两倍于晶格常数时,耦合微腔波导单位厚度(mm)透射比为47%,带宽为1.97 GHz,导模有效群折射率为22....     

低功耗聚合物波导可调耦合器的优化设计

提出并研究了一种带隔热槽的马赫-曾德尔干涉结构聚合物波导可调耦合器。仿真分析了热光电极作用下有、无隔热槽的耦合器波导温度分布,表明设置隔热槽可以降低热光调谐所需的功耗。研究了铝电极作用下不同上包层厚度对光传输损耗的影响,确定了上包层厚度。根据隔热槽与电极之间距离对热光调谐功耗的影响,结合隔热槽对导波光模式的影响及波导制备工艺,确定了隔热槽的位置。最终设计的带隔热槽聚合物波导可调耦合器实现1～0的分束比所需功耗为2.20mW,是无隔热槽的47.4%。     

低偏振相关损耗聚合物光波导

表征了新合成的热光聚合物bisphenol A-aldehyde resin (BPA-resin)的独特性质。并且利用光刻和反应离子刻蚀技术(RIE)制备成功BPA-resin 聚合物的单模条波导.实验结果表明,对于TE和TM偏振,该聚合物波导在1.31 μm和1.55 μm波长下分别有低达0.43 dB/cm和0.51 dB/cm的传播损耗.在上述波长下,波导的低偏振相关损耗 (PDL)小于0.1 dB/cm.因此,是制备可调热光器件的良好导波模快.     

光脉冲在微环耦合谐振光波导中传输线性特性的数值仿真

利用传输矩阵法得到了微环耦合谐振光波导色散关系的一般表达式,并由色散关系出发讨论了光脉冲在微环耦合谐振光波导中传输时的线性特性,包括带宽、群速度、色散和线性相位变化,这些特性对微环耦合谐振光波导在光通信和光传感领域的应用有重要意义. 关键词： 微环光波导 光脉冲线性特性 传输矩阵法 数值仿真     

溶胶-凝胶法制备SiO2-TiO2平板光波导工艺研究

采用溶胶-凝胶法制备了SiO₂-TiO₂平板光波导,计算了平板光波导通光条件,分析了硅/钛溶胶-凝胶材料的热性能,观测了平板光波导的结构形貌,并测试了其通光损耗。结果表明：经过200℃,30 min干燥处理的凝胶薄膜呈疏松多孔状态,对于非对称平板波导,存在芯层通光截止厚度,而且当SiO₂-TiO₂芯层厚度为0.5 μm时,SiO₂下包层厚度至少有6 μm才能防止1550 nm波长光泄露入单晶硅衬底中。制备的光波导对于1550 nm波长光传输损耗最小值为0.34 dB/cm。     

质子交换Y分支光波导弯曲损耗研究

对采用退火质子交换技术(APE)制备的具有正弦型弯曲和余弦型弯曲两种不同的S型弯曲的Y分支光波导,利用宽角有限差分光束传播法,就过渡区长度、波导表面折射率增量、掩模版开口宽度等对波导弯曲损耗的影响进行了研究。结果表明,两种S弯曲下的Y分支波导的弯曲损耗,随波导结构参数的变化基本上是相同的,但二者的表现并不完全一致。数值计算结果为相应波导器件的设计和制备提供了一定的参考。     

三维脊型光波导模斑转换器的设计和优化

在三维有限差分束传播法对脊形光波导的结构参数分析和优化的基础上,对单模光纤和脊形光波导连接耦合用模斑转换器进行了深入的研究,重点分析了影响模斑转换器性能的各种因素,如侧面边界、长度、大端宽度和厚度,以及连接光纤和模斑转换器的过渡波导的有关参数.仿真结果表明,三维锥形光波导模斑转换器大端宽度和厚度在11.5~13.5μm和4.5~6.5μm之间,且长度为200~500μm时插入损耗可低达2dB,比二维锥形光波导模斑转换器的插入损耗约减小2dB,其对横向偏移的容差也远远高于二维锥形光波导模斑转换器,合理的使用非线性边界的模斑转换器可以获得比线性边界的模斑转换器更小的插入损耗;过渡波导的宽度、芯层厚度应和三维锥形光波导模斑转换器的大端宽度和厚度一致,且其长度为150μm左右时损耗较小;另外,此类模斑转换器在减小耦合损耗的同时,还可以有效的进行光波模式的转换.     

数码照相法测量离子交换平面光波导损耗特性

利用数码相机对离子交换平面玻璃光波导传输线进行数字成像,根据传输线上的光强分布拟合出光强传输衰减曲线,计算出波导的传输损耗.对光波导进行退火处理,研究了波导退火前后的传输损耗特性.退火后0阶模式下传输损耗由2.148 9 dB·cm-1降为0.746 0 dB·cm-1.结果表明,波导的传输损耗是随着模阶数的增加而递增,适当的退火处理明显改善了离子交换波导的质量.     

关于"太阳在银河系中所受引力与到银心距离r的关系"的讨论

讨论了银道面内的引力场强分布和太阳在银河系中所受引力与到银心距离r的关系，指出引力场强g并不是与r的平方成反比，这是由于银河系的大小和形状不能忽略造成的．强调了万有引力定律的适用条件．     

On the calculation of the bremsstrahlung in the region of the plasma frequency

On the basis of the classical theory of radiation produced in incomplete Coulomb interaction, a formula is derived for the coefficient of the bremsstrahlung of fully ionized plasma. In the region of rectilinear approximation a comparison is made with the results of the quantum formula derived from the Born approximation. Furthermore, the influence of dispersion upon the emission coefficient is taken into account; some relations for the region of dispersion are given.     

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.     

On the predictability of the positions of the convergence zones in the ocean

The disagreement between the experimental and calculated positions of the first convergence zone are known from many publications. The most probable cause for such a disagreement, namely, the incorrect specification of the input data for the calculations, is considered. The lack of simultaneity between the hydrological surveys of the region and the acoustic experiments is emphasized. The experimental data obtained by the author in five ocean regions are presented. These data characterize the diurnal variability of the distance from the source to the nearest boundary of the convergence zone. The relations proposed by different researchers for calculating the sound speed from the temperature, salinity, and hydrostatic pressure are analyzed. It is shown that these relations lead to a substantial difference in the estimated depth dependence of the hydrostatic gradient of the sound speed. The position of the first convergence zone is calculated for the propagation conditions determined by vertical temperature and salinity profiles with the subsequent recalculation of these profiles into sound speed profiles by using eight different formulas known from the literature. It is shown that different formulas lead to different values of the distance to the first zone; this difference is substantially greater than that between the calculations and experiment. The necessity of improving the recalculation relations in view of the experimental data on sound propagation in natural oceanic waveguides, including the data on the actual positions of the convergence zones, is emphasized.     

Extracting the wavefunction of the LSP at the LHC

We consider associated production of squarks and gluinos with the lightest supersymmetric particle (LSP), or states nearly degenerate in mass with it. Though sub-dominant to pair production of color SU(3)-charged superpartners, these processes are directly sensitive to the wavefunction composition of the lightest neutralinos. Exploiting event-shape variables - including some introduced here for the first time - we are able to identify the composition of the LSP by selecting events involving a single high-pT jet recoiling against missing transverse energy. We illustrate the proposed technique on a set of benchmark cases and propose methods for applying these results in more realistic experimental environments.     

Set the controls for the heart of the Sun

In this paper we describe experiments conducted with high-power lasers that are attempting to replicate, for a very short time and in miniature, conditions found in the Sun. Experiments to date have reached conditions in the outer part of the Sun. To reach the Sun's centre requires compression of material to very much greater than solid density and heating to over ten million degrees. To achieve this, a new class of experiments and a new generation of high-power lasers are required.     

On the Question of the Source of the Apokamp

Technical Physics - The object of this work is the apokamp—a new type of plasma jet, which is formed from a bright offshoot emerging at the bending point of a channel of a high-voltage...