使用PTB7作为阳极修饰层提高有机发光二极管的性能

采用poly[[4,8-bis[(2-ethylhexyl)oxy]benzo[1,2-b:4,5-b’]dithiophene-2,6-diyl][3-?uoro-2-[(2-ethylhexyl)carbonyl]thieno[3,4-b]thiophenediyl]](PTB7)作为有机发光二极管器件的阳极修饰层,制备了结构为indium tin oxide(ITO)/PTB7(不同浓度)/N,N’-Bis(naphthalen-1-yl)-N,N’-bis(phenyl)benzidine(NPB,40 nm)/8-hydroxyquinoline(Alq3,60 nm)/LiF(1 nm)/Al的系列器件,同时研究了不同浓度的PTB7对器件性能的影响.PTB7的最佳浓度为0.25 mg/mL,器件性能得到明显的改善,起亮电压为4.3 V.当驱动电压为14.6 V时,最大亮度为45800 cd/m2,最大电流效率为9.1 cd/A.与没有PTB7修饰的器件相比,其起亮电压降低了1.9 V,最高亮度提升了78.5%.器件性能提高归因于PTB7的插入使得空穴注入和传输能力大大改善.     

铁钝化多孔硅的制备及光致发光机理研究

采用水热腐蚀法在相同环境下制备了不同晶型的铁钝化多孔硅样品。同一样品表面具有相似的孔隙结构,不同样品形貌存在差异。在300 nm光激发下,样品发光峰位于618 nm附近,半高宽约为132 nm。傅立叶红外变换光谱显示样品中有强的Si—Si、Si—O—Si、O y—Si—H x化学键振动吸收。结果表明,水热腐蚀法制备的铁钝化多孔硅表面形貌与腐蚀过程的局域电极分布关系密切。样品的光致发光行为可归因于量子限制-发光中心作用,并受非桥氧空穴发光中心数量影响。     

Ag掺杂对p型Pb0.5Sn0.5Te化合物热电性能的影响规律

采用熔融缓冷技术制备了不同Ag掺杂量的p型Ag_x(Pb_0.5Sn_0.5)_1-xTe化合物,系统地研究了Ag掺杂对所得材料的相组成、微结构及其热电传输性能.Ag的掺入显著增加了材料的空穴浓度,但是材料的空穴浓度远小于Ag作为单电子受主时理论空穴浓度,且在掺杂量为5%时未出现任何第二相,这表明Ag在可能进入晶格间隙位置而作为电子施主,起到补偿作用.随着Ag掺杂量的增加,样品的电导率逐渐增加,而Seebeck系数表现出复杂的变化趋势:在低于450 K时逐渐增加,而在温度大于450 K时逐渐降低,这主要源于材料复杂的价带结构.由于空穴浓度的优化和重空穴带的主导作用,1%Ag掺杂样品获得最大的功率因子,在750 K可达2.1 mW.m^-1.K^-2.此外,Ag的掺入引入的点缺陷大幅散射了传热声子,使得晶格热导率随着Ag掺量的增加逐渐降低.结果1%Ag掺杂样品在750 K时获得了最大的热电优值ZT=1.05,相比未掺样品提高了近50%,这一数值同商业应用的p型PbTe材料的性能相当.但是Sn取代显著降低了有毒重金属Pb的用量,这对PbTe基材料的商业化应用及其环境相适性具有重要意义.     

Coupling Losses for Resonators with Unequal Apertures for Extended Fresnel Numbers

Coupling losses have been calculated for laser resonators with unequal apertures and extended Fresnel Numbers. This was done using both, diffraction theory and a simple linear model.A close form expression was derived to calculate coupling losses with reasonable accuracies for a limited range of paramters. This should help in the preliminary design of hole coupling laser resonators.     

Hawking Radiation from Plane Symmetric Black Hole Covariant Anomaly

Based on the covariant anomaly cancellation method, which is believed to be more refined than the initial approach of Robinson and Wilczek, we discuss Hawking radiation from the plane symmetric black hole. The result shows that Hawking radiation from the non-spherical symmetric black holes also can be derived from the viewpoint of anomaly.     

Periodic Orbits Around Kerr Sen Black Holes

We investigate periodic orbits and zoom-whirl behaviors around a Kerr Sen black hole with a rational number q in terms of three integers(z,w,v),from which one can immediately read off the number of leaves(or zooms),the ordering of the leaves,and the number of whirls.The characteristic of zoom-whirl periodic orbits is the precession of multi-leaf orbits in the strong-field regime.This feature is analogous to the counterpart in the Kerr space-time.Finally,we analyze the impact of the charge parameter b on the zoom-whirl periodic orbits.Compared to the periodic orbits around the Kerr black hole,it is found that typically lower energies are required for the same orbits in the Kerr Sen black hole.     

Gravitational Deflection of Massive Particles by a Schwarzschild Black Hole in Radiation Gauge*

The exact metric of a Schwarzschild black hole in the true radiation gauge was recently reported.In this work, we base on this gravity and calculate the gravitational deflection of relativistic massive particles up to the fourth post-Minkowskian order. It is found that the result is consistent with the previous formulations for both the case of dropping the fourth-order contribution and the case of light deflection. Our result might be helpful for future high-accuracy observations.     

石墨烯包层结构光子晶体光纤的高双折射特性

将PG玻璃材料制作成的椭圆纤芯引入光子晶体光纤中心,设计了一种石墨烯包层结构的高双折射光子晶体光纤.基于有限元法对该光纤的双折射特性进行了数值模拟,研究了光纤孔径比、孔间距和纤芯椭圆对双折射特性的影响,并以该光子晶体光纤的模场面积和限制性损耗为依据进行了优化.研究结果表明:在波长1 550nm处,光纤双折射率高达0.13,满足高双折射要求;两偏振方向模场面积小于0.7μm2,限制性损耗低于10-6 dB/km.该光纤可有效保持光在传输系统中的偏振状态,为高稳定性超连续谱的产生提供依据.