h-BN型超晶格等离子体光子晶体能带特性研究

六方氮化硼(h-BN)晶格结构是一种类六方对称复式超晶格结构。具有h-BN晶格构型的光子晶体以其宽光子带隙特点受到国内外学者的广泛关注。本文利用不同尺度低压气体放电管与Al₂O₃介质棒周期性排列，构建了新型h-BN型超晶格等离子体光子晶体，实现其空间结构和等离子体参数的动态调控。利用微波透射谱对比研究了h-BN型超晶格与简单三角晶格等离子体光子晶体禁带位置、宽度和数目。分析了放电电流、介质棒阵列数对不同频段光子带隙的影响，以及电磁波入射角度对电磁传输特性的影响。结果表明：等离子体的引入不仅能够形成新的光子带隙，而且可以选择性地使部分禁带位置发生移动；相对于简单三角晶格，h-BN型超晶格等离子体光子晶体呈现出更多光子带隙；Al₂O₃介质棒阵列数对等离子体光子晶体禁带位置、宽度和数目均具有重要影响。电磁波入射角度变化越大，电磁传输特性差别越显著，透射谱相关性越差。本文所设计的新型h-BN型超晶格等离子体光子晶体为制作可调谐光子晶体提供了新的思路，在微波和太赫兹波控制领域具有潜在应用价值。     

Dynamical Evolution of Globular Clusters in the Galaxy

Given the initial conditions of spatial density distribution, velocity distribution and mass function, the dynamical evolution of globular clusters in the Milky Way is investigated in details by means of Monte Carlo simulations.Four dynamic mechanisms are considered: stellar evaporation, stellar evolution, tidal shocks due to both the disc and bulge, and dynamical friction. It is found that stellar evaporation dominates the evolution of low-mass clusters and all four are important for massive ones. For both the power-law and lognormM initial clusters mass functions, we can find the best-fitting models which can match the present-day observations with their main features of the mass function almost unchanged after evolution of severM Gyr. This implies that it is not possible to determine the initial mass function only based on the observed mass function today. The dispersion of the modelled mass functions mainly depends on the potential wells of host galaxies with the almost constant peaks,which is consistent with current observations.     

Mass of Open Cluster NGC 7789

Mass of open duster NGC 7789 in the Galaxy is determined by three methods： the photometric method based on mass-luminosity relations of stars in the duster Mpho= 7712.5M⊙; the dynamical method based on virial theorem Mvir=6996.1M⊙; and the tidal radius method based on the interaction between the cluster and the Galaxy Mtid= 5152.5M⊙. The mean mass of this cluster is estimated to be Mc =6620.4 4- 762.5M⊙.     

腹板V形加劲冷弯薄壁卷边槽钢柱试验研究

为了解腹板V形加劲冷弯薄壁卷边槽钢构件的受压性能,对8根短柱和中长柱进行了轴心受压试验研究。在试验之前首先用有限条和有限元方法对柱试件进行了详细的设计,以确保发生畸变屈曲失效。柱受压试验结果发现：所有试件均发生畸变屈曲失效破坏,同时在峰值荷载时中长柱试件有绕弱轴的弯曲产生,畸变屈曲和局部屈曲一样也有一定的屈曲后强度。在总结分析现有国内外规范计算理论的基础上,提出了基于直接强度法设计腹板V形加劲冷弯薄壁卷边槽钢轴压构件畸变屈曲承载力的计算方法。采用该建议方法计算所得结果与试验值和参数分析值吻合较好,其设计过程简便且安全可靠。     

Lieb晶格等离子体光子晶体基元结构原位调控

利用独特设计的阵列-液体电极介质阻挡放电装置,率先获得了Lieb晶格等离子体光子晶体,并实现了其基元大小、形状和微观形貌的多自由度原位调控。采用光电倍增管对Lieb晶格等离子体光子晶体的时空动力学行为进行了时空分辨测量。基于有限元计算,对不同基元结构的Lieb晶格等离子体光子晶体的色散关系和能带变化规律进行了系统研究。结果表明：Lieb晶格等离子体光子晶体由两套不同四方子晶格相互嵌套形成,具有优异的时空稳定性和周期性;随着Lieb晶格基元构型的改变,光子带隙发生显著变化,形成了偶然简并的类狄拉克锥结构,以及不同频段的完全带隙和非完全带隙;基元的几何形状对光子带隙数目、位置和宽度均具有重要影响。     

Orbital Phase Dependence of Globular Cluster＇s Tidal Radii

The orbits for a sample of 45 galactic globular clusters are calculated using positions and spatial velocities based on recent compilations as well as new measurements of their absolute proper motions.The perigalactic positions of each cluster are used to determine their theoretical tidal radii in the given galactic model.The orbital phase dependence between the theoretical and observed tidal radii is evidenced.