Coupling effects of depletion interactions in a three-sphere colloidal system

In a three-sphere system, the middle sphere is acted upon by two opposite depletion forces from the other two spheres. It is found that, in this system, the two depletion forces are coupled with each other and result in a strengthened depletion force. So the difference of the depletion forces of the three-sphere system and its corresponding two two-sphere systems is introduced to describe the coupling effect of the depletion interactions. The numerical results obtained by Monte-Carlo simulations show that this coupling effect is affected by both the concentration of small spheres and the geometrical confinement. Meanwhile, it is also found that the mechanisms of the coupling effect and the effect on the depletion force from the geometry factor are the same.     

大尺寸单元自组装准晶研究评述

不同于传统的晶体,准晶由非单一的结构单元以一种非重复的方式铺满空间而构成.准晶的形成依赖于短程序和长程序之间微妙的协同,因此准晶常常只在很窄的参数窗口内能得到.近年来,人们利用纳米以至微米级的结构单元,通过溶液中自组装或者在模板上生长,成功地获得了多种大尺寸结构单元的准晶结构.近年的研究还发现,在自然界的矿物中和中世纪伊斯兰建筑装饰上都能找到准晶结构.对准晶结构的多角度、多学科探索,有助于实现准晶的人工设计和生长.     

在分光计实验中的几何关系探究

从空间几何的角度来对分光计的构造、结构以及调节方法等方面来加以说明,以便从根本上掌握分光计设计的原理、调节的思路以及拓展的方法。     

(CoO)_n(n≤6)合金团簇的结构和磁性理论研究

采用密度泛函理论中的广义梯度近似(DFT-GGA)对(CoO)_n(n≤6)合金团簇进行了系统的几何、电子结构和磁性质研究.研究结果表明(CoO)n(n≤6)团簇最稳定结构除(CoO)6团簇为三维立体结构外,其余团簇均呈二维平面结构,且(CoO)_n(n=1,2,3,4和6)结构均表现明显的钴氧分离特征,而(CoO)5团簇表现明显的Co—Co聚合和O—O分离特征.团簇的总磁矩在n=1,3,4时,以3μB为单元成倍增长,(CoO)5团簇显著降低,减小至1μB,(CoO)6团簇又有所增加,增大至6μB.(CoO)n(n≤6)团簇磁性变化的起因也从电荷转移、磁性耦合、电子差分密度和态密度进行了详细阐释.     

L_p-对偶几何表面积

Lutwak结合Lp-混合体积给出了Lp-几何表面积的概念,本文结合Lp-对偶混合体积,给出了Lp-对偶几何表面积的概念,并且证明了相关不等式.     

颗粒超导体临界电流密度的尺寸效应

假设颗粒超导体内某点临界电流密度是该处磁场强度平均值的某种函数,计算了其实测临界电流密度与样品尺寸的关系.发现对目前实验中所用的烧结样品,实验测得的 YBaCuo超导体的临界电流密度有显著的尺寸效应.     

^1H自旋扩散方法研究离子化聚氨酯的相态结构

本文用改进的Goldman-Shen脉冲序列研究了聚丁二烯加MDI离子化聚氨酯体系中磁化矢量的自旋扩散过程,通过一些合理的简化,求解了扩散方程,得到了一种可定量的求出多相高聚物微区尺寸的简便方法.     

n分量φ4模型薄膜的尺寸效应

我们用场论重整化群方法讨论了周期边界的n分量φ⁴模型薄膜的单纯尺寸效应,发现仅当维数满足d_<+1>时尺寸效应具有Fisher的标度形式,其他情况下它是不可标度的。同时也讨论了维数渡越现象及状态方程。 关键词：     

Geometry optimization in planetary rotation stage for thickness uniformity of films on spherical substrates

We report the simulation results on the thickness uniformity of optical coatings deposited on spherical substrates by optimizing the geometric configuration parameters, such as tilting angle of the substrate holder and position of the evaporation source in a 1 000-mm-diameter planetary rotation stage （PRS）. We reveal that good film uniformity on convex spherical surfaces or flat substrates, as well as concave surfaces with weak to moderate curvatures can be obtained through appropriate tilting of the substrate holder. For 300-mm-diameter substrates with clear aperture to radius of curvature （CA/RoC） between 0.3 and 0.7, the achievable film uniformity is above 99%. The source position is optimized to achieve good film uniformity.