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1.
 分析了脉冲线加速器在放电过程中产生的预脉冲电压现象。为了减少预脉冲电压引起的等离子体发射对正常状态的影响,采用了一种冷阴极撬棒管,将它与阴极杆相连。实验证明在采用了这种器件后,预脉冲电压可以从150kV左右减少到50kV。相对论返波管和相对论磁控管的性能得以显著改善。  相似文献   
2.
利用宇宙射线进行探测器模型的性能测试是高能物理普遍采用的方法,其中最重要的步骤之一就是确定宇宙线入射的准确位置和径迹.多数采用丝室探测器来进行宇宙线的精确定位,需要很高的造价和复杂的电子学系统.本文介绍一种简单的定位方法,采用塑料闪烁体条加波移剂光纤编码读出的方式,可以实现精度为1cm的定位.据此建立了一套实验装置,对BESⅢ电磁量能器CsⅠ(Tl)晶体探测器单元的光输出强度和不均匀性进行了测量.  相似文献   
3.
武振华  李华  严亮星  刘炳灿  田强* 《物理学报》2013,62(9):97302-097302
本文采用分数维方法, 在讨论Al0.3Ga0.7As衬底上GaAs薄膜的分数维基础上, 计算了GaAs薄膜中的极化子结合能和有效质量. 随着薄膜厚度的增加, 极化子结合能和质量变化单调地减小. 当薄膜厚度Lw<70 Å并且衬底厚度Lb<200 Å时, 衬底厚度的变化对薄膜中极化子的结合能和质量变化的影响比较显著, 随着衬底厚度的增加, 薄膜中极化子的结合能和质量变化逐渐变大; 当薄膜厚度Lw>70 Å或者衬底厚度Lb>200 Å时, 衬底厚度的变化对薄膜中极化子的结合能和质量变化的影响不显著. 研究结果为GaAs薄膜电子和光电子器件的研究和应用提供参考. 关键词: 分数维方法 GaAs薄膜 极化子 低维异质结构  相似文献   
4.
刘炳灿  李华  严亮星  孙慧  田强 《物理学报》2013,62(19):197302-197302
本文用分数维方法研究AlxGa1-xAs衬底上GaAs薄膜中的极化子特性, 提出了确定GaAs薄膜的有效量子限制长度的一个新方法, 解决了原来方法中在衬底势垒处有效量子限制长度发散的困难, 得到了AlxGa1-xAs衬底上GaAs薄膜中的极化子的维数和结合能. 关键词: 分数维方法 极化子 GaAs薄膜  相似文献   
5.
This paper focuses mainly on the vertex reconstruction of resonance particles with a relatively long lifetime such as Ks^0, A, as well as on lifetime measurements using a 3-dimensional fit. The kinematic constraints between the production and decay vertices and the decay vertex fitting algorithm based on the least squares method are both presented. Reconstruction efficiencies including experimental resolutions are discussed. The results and systematic errors are calculated based on a Monte Carlo simulation.  相似文献   
6.
The reconstruction algorithm for BESⅢ Muon Counter, MucRecAlg, is developed with the objectoriented language C++ in BESⅢ offine software environment. MucRecAlg consists of the following functions:to find track seeds either from extrapolation of tracks in the main drift chamber or from the fired strips in muon counter, to select fired strips associated to the candidate tracks, to fit the candidate tracks with a linear or quadratic function and to calculate other parameters of the tracks for muon identification. Monte Carlo samples are generated to check the performance of the reconstruction package, such as reconstruction effciency, muon remaining rate and pion rejection rate, etc. The preliminary results show that the pion rejection rate is around 3%—4% while the muon remaining rate is better than 90% in 0.4—1.6 GeV/c momentum region, which meets the requirement as shown in the design report.  相似文献   
7.
In this paper, the kinematic fitting with the Lagrange multiplier method has been studied for BESⅢ experiment. First we introduce the Lagrange multiplier method and implement kinematic constraints. Then we present the performance of the kinematic fitting algorithm. With the kinematic fitting, we can improve the resolution of track parameters and reduce the background.  相似文献   
8.
Primary vertex reconstruction is crucial to estimate the beam profile in collision experiments. We study the principle of an iterative process, called the Kalman filter method, and apply it to primary vertex reconstruction at BESⅢ. A Newton procedure to find the zero point of the distance function's gradient is used for primary vertex finding in 3-dimensional space. Results are obtained based on raw data at BESⅢ.  相似文献   
9.
The principle of the method for the BESIII TOF calibration using cosmic ray data without magnetic field are reported in this paper. After applying calibration constants, the single-end readout time resolution could reach about 150 ps, and the time resolution for one layer is achieved to be about 110 ps. The paper also described the extraction scheme for the event start time of cosmic events.  相似文献   
10.
Software alignment is quite important for a tracking detector to reach its ultimate position accuracy and momentum resolution. We developed a new alignment algorithm for the BESⅢ Main Drift Chamber using the Kalman Filter method. Two different types of data which are helix tracks and straight tracks are used to test this algorithm, and the results show that the design and implementation is successful.  相似文献   
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