不同环境压强下溶剂退火对聚合物太阳能电池性能的影响

通过改变溶剂退火时的环境压强控制溶剂的蒸发速率,在不同压强下进行加压溶剂退火制备了基于聚-3己基噻吩:富勒烯衍生物(P3HT:PCBM)的体异质结聚合物太阳能电池。X射线衍射(XRD)、紫外-可见吸收光谱(UV-Vis)以及原子力显微镜(AFM)的测试结果表明,增大溶剂退火的环境气压改善了薄膜的结晶度,增强了有源层的光吸收,提高了P3HT和PCBM的相分离程度,更有利于激子的解离和载流子传输。与在常压下溶剂退火相比,在2.0 MPa压强下对有源层进行溶剂退火的器件的光电转换效率提高了29%,达到了3.69%。     

Stability Analysis of the Viscous Polytropic Dark Energy Model in Einstein Cosmology

The viscous polytropic gas model as one model of dark energy is hot-spot and keystone to the modern cosmology.We study the evolution of the viscous polytropic dark energy model interacting with the dark matter in the Einstein cosmology.Setting the autonomous dynamical system for the interacting viscous polytropic dark energy with dark matter and using the phase space analysis method to investigate the dynamical evolution and its critical stability,we find that the viscosity property of the dark energy creates a benefit for the stable critical dynamical evolution of the interaction model between dark matter and dark energy in the flat Friedmann-Robertson-Walker universe and the viscosity of dark energy will soften the coincidence problem just like the interacting dark energy model.     

Solution of the Fermi--Ulam Model in the Case of Periodic Perturbation

We discuss the evolution of the state and the average energy of the Fermi Ulam model in the case of periodic perturbation. By a perturbation technique, the time-dependent Sehr6dinger equation is solved and it is found that the particle will continuously absorb or radiate energy Jf the frequency of the oscillating wall meets the resonance condition. Usually, these two states cannot exist together at a certain frequency. However, there is an exception if the frequency is at some special values. We find these values and reveal that the energy for transmission has the minimum equivalent unit, which is in the form of a harmonic oscillator.     

平面旋转场诱导下磁流变液的结构模型

针对平面旋转场下磁流变液中诱导产生的层状结构 ,提出了恰当的理论模型 ,该模型成功的解释了层状结构在同步旋转状态下 :层间距随磁场的变化关系 ;旋转层的滞后角随旋转角频率以及其他物理量之间的关系 ;层半径与旋转角频率之间的关系 .理论结果与文献中发表的实验结果相吻合     

The Effect of Rotating Cylindrical Langmuir Probes in Magnetron Plasmas

Using a cylindrical Langmuir probe, the plasma properties (ion density, electron temperature, floating and plasma potentials) in a magnetron sputter source have been investigated, along one particular line‐of‐sight, but for different probe‐orientations with respect to the B‐field. The plasma in the region hosen for observation is haracterised by electrons, which are magnetised (Larmor radius r_le < both the electron mean‐free‐path λ_e, and plasma extension L) and ions, which are not (their Larmor radius r_I > L, λ_I). Through the development of a simple expression for the electron saturation current at different probe angles relative to the local B‐field, it is possible to correct for the diminished electron currents due to their restricted transport across the field. The results indicate that the measured ion density, electron temperature, floating and plasma potentials are unaffected by the probe orientation, however the electron saturation current is attenuated when the probe is aligned along the B‐field. A simple model for the collection of electrons indicates that classical electron diffusion may not operate in the magnetron, with cross‐field electron transport dominated by anomalous, possibly Bohm, diffusion.     

利用羊八井中子监测器研究宇宙线的太阳日周期变化

通过对宇宙线周期变化研究可以得到宇宙线产生和传播区域的重要信息,是宇宙线长期研究的重要热点问题。利用位于西藏羊八井(地磁截止刚度:14.1 GeV) 的中子监测器2006 至2011年的观测数据,研究宇宙线的太阳日周期变化。在对中子监测器观测数据进行气压修正后,通过Lomb-Scargle 傅立叶变换法对修正后的数据进行周期分析,发现宇宙线计数率存在超过地球公转运动Compton-Getting 效应的太阳日周期变化,该周期变化可能是地球公转效应和宇宙线传播物理过程调制效应以及剩余气象效应的叠加。计算分析了1 日周期信号的振幅和初相位随时间的变化,发现1 日周期变化的初相位存在较为明显的年周期变化规律,这可能是地球公转和自转合成运动的结果;1 日周期变化幅度在2010 年后出现增大趋势。这些结果对宇宙线周期变化和各向异性的研究具有重要参考意义。With the study of the cosmic rays' solar diurnal variation we can get the important information about Cosmic Ray's production and propagation. It's important issues of cosmic rays' studies. We analyze the temporal variation of cosmic rays rate observed with the Yangbajing neutron monitor during 2006 to 2011, and nd semidiurnal and diurnal period signals included in the rates of cosmic rays with vertical rigidity equal to 14.1 GV. We have checked the time dependence of the phase and the amplitude of semidiurnal and diurnal anisotropy, and nd that the phase of diurnal signal varies yearly, it could be a synthetic movement of the earth's rotation and revolution. The amplitude before 2010 is obvious smaller than that after 2010. These results are of great reference value for studying the anisotropy and time variation of cosmic rays.     

The Effect of Morphologies of Embedded Plasmonic Cu-nanoparticles on Solar Absorption of Perovskite Solar Cells. A Comprehensive Study

Optics and Spectroscopy - In this work we aim to reduce the production costs of perovskite solar cells (PSCs) and achieve high solar absorbance with the inclusion of different shapes of plasmonic...     

大气湍流对轨道角动量态复用系统通信性能的影响

通过数值仿真,以多个相位屏模拟大气湍流,研究大气湍流对轨道角动量(Orbital Angular Momentum,OAM)态复用通信系统质量的影响.改变大气湍流折射率结构常量C2n和传输距离z,分析其对OAM态复用系统归一化接收功率、误码率等的作用.研究结果表明当大气湍流强度增加和传输距离增长时,复用系统归一化接收功率下降、误码率增加.当C2n增大到5×10-13 m-2/3时,系统归一化接收功率下降到0.2以下,误码率增大到0.3以上;当传输距离增大到10 000m,系统归一化接收功率下降到0.3以下,误码率增大到0.35以上.同时,对比不同方位角指数l取值的两个OAM态复用系统受大气湍流的影响,发现:l取值越接近的系统,受大气湍流影响越大.在等同光学信噪比下大气湍流导致OAM态复用系统误码率性能降低2至3个数量级.该研究对OAM态复用系统的实用化具有积极的参考作用.     

阳极缓冲层修饰对聚合物太阳能电池性能的影响

为提高聚合物太阳能电池的能量转换效率,将聚乙二醇(PEG)掺入PEDOT∶PSS阳极缓冲层,研究了阳极缓冲层修饰对聚合物太阳能电池性能的影响。首先研究了聚乙二醇对PEDOT∶PSS薄膜电导率的影响,发现PEG会与PEDOT和PSS相互作用,使得PEDOT链重新排布,有利于电荷载流子的传输,从而显著改善了PEDOT∶PSS薄膜的电导率,当PEDOT∶PSS中掺入体积分数为2%~4%的PEG时,可得到较大的电导率。然后,以PEG修饰的PEDOT∶PSS薄膜作为阳极缓冲层制备了聚合物太阳能电池,研究了PEG的掺入对聚合物太阳能电池性能的影响。实验发现,PEG改善的PEDOT∶PSS电导率有利于提高电池的短路电流密度和填充因子,从而改善了器件光伏性能。当PEDOT∶PSS中掺入体积分数为2%的PEG时,聚合物太阳能电池的能量转换效率最高,比未掺杂的器件提高了24.4%。     

p-InGaN层厚度对p-i-n结构InGaN太阳电池性能的影响及机理

研究了p-lnGaN层厚度对p-i-n结构InGaN太阳电池性能的影响.模拟计算发现,随着p-InGaN层厚度的增加,InGaN太阳电池效率降低.较差的p-InGaN欧姆接触特性会破坏InGaN太阳电池性能.计算结果还表明,无论欧姆接触特性好坏,随着p-InGaN层厚度的增加,短路电流下降是导致InGaN电池效率降低的主要原因.选择较薄的p-InGaN层有利于提高p-i-n结构InGaN太阳电池的效率.     

丁香对低密度脂蛋白氧化过程中荧光特性变化的影响

低密度脂蛋白(LDL)氧化修饰是导致动脉粥样硬化(AS)的关键因素,LDL在氧化修饰过程中荧光特性会发生一系列改变。为评价丁香对LDL氧化过程中荧光的抑制效果,采用传统荧光及三维荧光等高线光谱研究丁香对LDL氧化修饰过程中荧光特性的影响。结果显示： LDL氧化孵育荧光特性的最佳测定时间为48 h;丁香粗提物对LDL氧化修饰过程中色氨酸(Trp)荧光猝灭、荧光发色团红移、氧化产生的活性醛修饰apoB 100所含赖氨酸(Lys)残基变化、荧光物质和脂褐素产生及三维荧光的变化均具有较好的抑制作用,且抑制作用与粗提物浓度成正相关。在此基础上进一步发现,丁香各极性成分(正己烷相(丁香精油)、乙酸乙酯相、正丁醇相及水相)对LDL氧化修饰过程荧光特征的变化影响不一。其中,正己烷相对Trp荧光猝灭、荧光发色团红移及三维荧光变化的抑制作用最强,而乙酸乙酯相抑制活性醛修饰Lys残基、荧光物质和脂褐素的产生效果最好。结果表明,丁香对LDL氧化修饰过程中荧光特性的变化具有较好的抑制作用,抑制作用的主要物质集中在正己烷相和乙酸乙酯相。该研究为后续丁香组成分析及其功能食品研发提供参考。     

当量比对圆盘结构下旋转爆震波传播的影响

为研究反应物当量比对旋转爆震波传播过程的影响,在圆盘形旋转爆震发动机上进行H₂/air的旋转爆震实验研究,并统计分析了当量比对爆震波传播模态及参数的影响规律.实验结果表明,固定质量流率,同一种传播模态下,随着当量比的增大,爆震波的压力峰值及传播速度增大,且旋转爆震波的传播过程更加稳定.不同质量流率条件下,当量比对传播模态的影响规律不同.空气质量流率小于100 g/s时,旋转爆震波皆以单波模态传播.空气质量流率大于150 g/s时,随着当量比的增大,旋转爆震波的传播模态由单波模态向双波模态转变,再转变为不对称双波模态,最后又回到单波模态.并且在不对称双波模态中发现了低频振荡现象,振荡频率约为300 Hz.质量流率继续增大,燃烧室中发现了同向三波传播模态.随着质量流率的增加,双波模态的当量比下限降低,不对称双波模态的当量比上限增大,而双波与不对称双波模态的分界线受质量流率的影响较小.      

Effect of Coma Aberration on Orbital Angular Momentum Spectrum of Vortex Beams

Spiral spectra of vortex beams with coma aberration are studied. It is shown that the orbital angular momentum （OAM） states of vortex beams with coma aberration are different from those aberration-free vortex beams. Spiral spectra of beams with coma aberration are spreading. It is found that in the presence of coma aberration, the vortex beams contain not only the original OAM component but also other components. A larger coma aberration coefficient and/or a larger beam waist will lead to a wider spreading of the spiral spectrum. The results may have potential applications in information encoding and transmittance.     

出流角对旋转涡轮叶片前缘气膜冷却影响

基于频闪拍照和稳态液晶测温技术,实验研究了不同气膜孔出流角对旋转态整级涡轮叶片前缘外壁面的气膜冷却特性的影响。实验中,叶片前缘处的主流雷诺数为6.3378×104。实验转速为574 r/min,对应的旋转数为0.0018。平均吹风比从0.5变化到1.25。射流采用N2,其对应的密度比为1.04。结果表明:展向平均气膜冷效是随吹风比的增加而单调增加的,其中最佳吹风比为M=1.25。对于所有吹风比,在-4.3相似文献