A Matter Dominated Navigation Universe in Accordance with the Type Ia Supernova Data

We investigate a matter dominated navigation cosmological model.The influence of a possible drift(wind) in the navigation cosmological model makes the spacetime geometry change from Riemannian to Finslerian.The evolution of the Finslerian Universe is governed by the same gravitational field equation with the familiar Friedmann-Robertson-Walker one.However,the change of space geometry from Riemannian to Finslerian supplies us a new relation between the luminosity distant and redshift.It is shown that the Hubble diagram based on this new relation could account for the observations on distant Type Ia supernovae.     

Constraints from Type Ia supernovae on the Λ-CDM model in Randers-Finsler space

Gravitational field equations in Randers-Finsler space of approximate Berwald type are investigated. A modified Friedmann equation and a new luminosity distance-redshift relation is proposed. A best-fit to the Type Ia supernovae (SNe) observations yields that the Ω_Λ in the Λ-CDM model is suppressed to almost zero. This fact indicates that the astronomical observations on the Type Ia SNe can be described well without invoking any form of dark energy. The best-fit age of the universe is given. It is in agreement with the age of our galaxy.     

聚(3,4-乙撑二氧噻吩)导电织物的制备、结构及其电致变色性能

本文采用原位聚合法, 以耐酸性好的涤纶为基底, 制得了聚(3,4-乙撑二氧噻吩)/涤纶复合导电织物[Poly(3,4-ethylenedioxythiophene)/conducting terylene textile, PEDOT/CTT], 分析了该导电织物的形貌、导电性能及结构, 并对其电致变色性能进行了初步测试. 实验结果表明, 所得到的PEDOT/CTT具有良好的导电性和一定的电致变色性能, 有望在全固态电致变色织物的制备中获得应用.     

烷基锌与亚胺不对称加成反应的研究进展

综述了烷基锌与亚胺不对称加成反应的最新进展。参考文献31篇。     

石墨烯折角场发射特性

针对直立的石墨烯边沿悬挂键易吸附气体分子,影响发射稳定性的问题,本文将石墨烯转移到墙状绝缘结构上,获得石墨烯折角.结合电感耦合等离子体刻蚀和湿法腐蚀法在硅衬底上制得墙状绝缘结构,以石墨烯折角作为场发射尖端,测试研究了石墨烯折角的场发射特性和石墨烯中内导电流对场发射的影响.结果表明:石墨烯折角的场发射开启场强为9.6V/μm;在2 000V阳极电压下,当石墨烯两端偏压从0V增加到10V时,场发射电流从4.5μA增加到15μA.     

8-羟基喹啉与醋酸钴固相配位反应的热化学研究

用具有恒定温度环境的反应热量计,以 ４ ｍ ｏｌ· Ｌ－ １ Ｈ Ｃｌ溶液为量热溶剂,测得８羟基喹啉与醋酸钴固相反应焓Δｒ Ｈｍ ＝ ２９．６８ ｋ Ｊ·ｍ ｏｌ－ １,计算了配合物 Ｃｏ（ｏｘｉｎ）２ ·２ Ｈ２ Ｏ 的标准生成焓Δｆ Ｈｍ ＝ － ７６４．６ ｋ Ｊ·ｍ ｏｌ     

用稀土多元渗法制备钾稀土钨青铜KxLayWO3的XPS研究

Potassium tungsten bronze K_xLa_yWO₃ (x>0.5 and y<0.01) was synthesized by rare earth co-permeation method using α-K₇[SiMg₃(OH₂)₃W₉O₃₇] as the precursor. Binding energies of La, W, O and C were determined by XPS. From the XPS data, a peak at 34.21 eV indicates that some W⁶⁺ turned into W⁵⁺ by rare earth co-permeation. The binding energies La3d were the same in the surface and inner of the composite, showing that rare earth element La could diffuse into the body of the composite and the compound of K_xLa_yWO₃ was formed at the same time. The binding energies of O1s in K_xLa_yWO₃ surface were 531.4 eV and 532.0 eV, respectively, while peak at 531.4 eV disappeared through etching process. The result implies that the binding energy of 531.4 eV was due to the adsorbent O. In addition, the binding energies of C1s in the surface were 283.5 eV, 285.0 eV and 286.7 eV respectively, while the inner had only one peak at 285.0 eV due to standard C1s. This proves that there was no C in the core.     

暗物质寻找实验中CsI（T1）晶体反符合探测器实验研究

一个正在建设的位于韩国Y2L地下实验室的低能暗物质探测实验中,采用了CsI（T1）晶体反符合探测器作为主动屏蔽体.本工作对CsI（T1）晶体反符合探测器的实验性能进行了研究.通过FADC系统记录的脉冲波形数据,研究了探测器的能量分辨率和波形甄别的能力;研究相同能量γ射线入射到反符合探测器不同位置的相对光输出将有助于选择探测器的工作参数;为了解晶体自身放射性对暗物质测量的影响,利用低本底HPGe探测器对CsI（T1）晶体内部的放射性进行了测量,得到晶体内部Cs同位素的放射性活度.探测器系统进行了约18d的试运行取数.实验数据表明,CsI（T1）晶体探测器的反符合效率约为31%,HPGe探测器的本底计数率水平约为133cpd.为了进行暗物质探测研究,需要采取有效的方法进一步降低探测器的本底水平.     

考虑土体非线性特性的直埋管道——土体系统的动力反应分析

本文采用二维有限元方法对连续直埋管管道在动力荷载作用下的反应进行分析,管道周围土体采用等效线性粘弹性模型,为反映管－土间的相对滑移,在管单元与土单元间加入无厚度Goodman接触单元,并利用Wilson-θ法对管－土系统进行动力时程反应分析,本文研究了输入液频率,输入波幅值,管道埋深,土体类别和管－土间摩擦系数等因素对埋管动力反应的影响。