在SDSS DR8恒星光谱中自动搜寻稀有天体

SDSS DR8海量光谱中包含许多有研究价值的稀有天体,如特殊白矮星(DZ,DQ,DC)、碳星、白矮主序双星、激变变星等,如何在海量光谱中自动搜寻稀有天体有着极其重要的意义。提出一种基于核密度估计和K-近邻(K-nearest neighbor, KNN)相结合的方法在SDSS DR8 信噪比大于5的546 383个恒星光谱中搜寻稀有天体。首先对光谱进行高斯核密度估计,选取概率最小的5 000个光谱作为稀有类,概率最大的300 000个光谱作为普通类,然后进行KNN分类,同时也将5 000个稀有光谱的K个最近邻也作为稀有的天体,结果共有21 193条光谱。为了方便分析,对这些光谱聚类后进行人工检查。这些光谱主要包括由于数据缺失、红化、流量定标不准引起的问题光谱、行星状星云、没有物理联系的光谱双星、类星体、特殊白矮星(DZ,DQ,DC)、碳星、白矮主序双星、激变变星等。通过和SIMBAD,NED,ADS及一些主要的文献交叉验证,我们新发现了3个DZ白矮星、1个白矮主序双星、2个伴星为G型星的激变变星,3个激变变星的候选体、6个DC白矮星,1个DC白矮星候选体和1个 BL Lacertae(BL lac)候选体。还发现了1个有CaⅡ三重发射线和MgⅠ发射线的DA白矮星和1个光谱上表现出发射线的晚M恒星但测光图上像是一个星云或星系。     

Adaptive multitrack reconstruction for particle trajectories based on fuzzy c-regression models

In this paper, an approach to straight and circle track reconstruction is presented, which is suitable for particle trajectories in an homogenous magnetic field (or 0 T) or Cherenkov rings. The method is based on fuzzy c-regression models, where the number of the models stands for the track number. The approximate number of tracks and a rough evaluation of the track parameters given by Hough transform are used to initiate the fuzzy c-regression models. The technique effectively represents a merger between track candidates finding and parameters fitting. The performance of this approach is tested by some simulated data under various scenarios. Results show that this technique is robust and could provide very accurate results efficiently.     

Radiation and ionization energy loss simulation for the GDHsum rule experiment in Hall-A at Jefferson Lab

The radiation and ionization energy loss are presented for single arm Monte Carlo simulation for the GDH sum rule experiment in Hall-A at the Jefferson Lab. Radiation and ionization energy loss are discussed for ¹²C elastic scattering simulation. The relative momentum ratio Δp/p and ¹²C elastic cross section are compared without and with radiative energy loss and a reasonable shape is obtained by the simulation. The total energy loss distribution is obtained, showing a Landau shape for ¹²C elastic scattering. This simulation work will give good support for radiation correction analysis of the GDH sum rule experiment.     

全光纤量子保密通信中的偏振控制

介绍了在全光纤量子保密通信系统的量子信道中利用可转动光纤圈型偏振控制器实现对光纤偏振态的测量和调整.实验证明该方法能有效控制光纤中的偏振态.     

纳米粒子与单晶硅表面碰撞的反弹机理研究

应用分子动力学方法模拟了纳米粒子与单晶硅(001)表面碰撞、反弹飞离的现象，分析了粒子的反弹行为、基体弹性形变和塑性形变的原子构型特征，以及碰撞过程的能量转化.碰撞后单晶硅表面形成半球形的小坑，小坑周围的基体原子呈非晶态.碰撞过程中与颗粒相邻的基体原子立即非晶化，在非晶层外面基体以可恢复的(111)［110］滑移结构存储弹性形变能.在射入过程，基体发生压缩弹性形变；颗粒反弹时基体势能振荡下降,交替形成压缩形变构型和拉伸形变构型.射入过程中存贮的压缩弹性形变能的释放为颗粒提供了反弹、飞离的能量. 关键词： 碰撞 纳米粒子 单晶硅表面 分子动力学模拟     

Ti-Zr-Ni单相准晶合金的室温力学性能研究

以Ti40₄₀Zr40₄₀Ni20₂₀合金为研究对象，用铜 模吸铸法制备出直径为3mm的致密单相准晶棒，通过维氏显微硬度测定和单向压缩实验方 法研究了该合金的室温力学性能 .结果表明：Ti40₄₀Zr40₄₀Ni20₂₀准晶具有良好 的弹性变形能力，室温弹性应 变可达125%.同时，它具有相对高的室温硬度（约55GPa），是普通Ti合金的15倍.T i40_{40 关键词： 准晶 Ti-Zr-Ni合金 解理断裂}     

Oscillatory disturbance in force calibration of optical tweezers

In the calibration of the optical trap stiffness, it is found that there appears an attenuating oscillation as an oscillatory disturbance added to the trapped bead movement, when the scanner is driven by a triangular wave input.An equivalent oscillator model is put forward to explain the mechanism of the oscillatory disturbance. Both the measurements and calculations show that the attenuating oscillation comes from the oscillation of the scanner and the triangular wave drive causes this additional oscillation of the scanner. Furthermore, the analysis indicates that the oscillatory disturbance will become stronger, when the stiffness of the trap increases or the natural frequency of the scanner decreases. We adopt another driving way, i.e. a sinusoidal wave input is used instead of the triangular wave input. Our experiment has verified that in this case the oscillatory disturbance is eliminated completely.     

LD泵浦Nd∶GdVO4晶体Cr4+∶YAG被动调Q激光特性研究

考虑腔内光子数密度的空间高斯分布以及晶体热效应的影响,给出了LD泵浦Nd∶GdVO4晶体Cr4+∶YAG被动调Q 1.06 μm激光的耦合速率方程组.数值求解该方程组获得了输出激光的脉冲宽度、重复率、峰值功率以及单脉冲能量随泵浦功率的变化特性,其理论值与实验结果相符.     

一道伯克利数学问题的再讨论

对伯克利数学问题集中关于余弦函数的一个不等式建立了双边不等式.同时给出了关于反正弦函数、反余弦函数、反正切函数、反双曲正弦函数、反双曲正切函数的双边不等式.     

关于K_(2n)-E(C_m)的点可区别边色数

图G的一个k-正常边染色f被称为点可区别边染色是指任何两点的点及其关联边的色集合不同,所用最小的正整数k被称为G的点可区别边色数,记为X'_(vd)(G).用k_(2n)-E(C_m)表示2n阶完全图删去其中一条m阶路的边后得到的图,得到了K_(14)-E(C_4),K_(16)-E(C_4),K_(18)-E(C_5),K_(20)-E(C_5)的点可区别边色数分别为14,16,18,20.