论文标题
宇宙射线测试中BESIII CGEM检测器的基于轨道的对齐
Track-based alignment for the BESIII CGEM detector in the cosmic-ray test
论文作者
论文摘要
北京电子光谱仪III(BESIII)是在北京电子正电子撞机II(BEPCII)上运行的多功能检测器。经过十年以上的运行,主漂移室(MDC)内层的效率显着下降。为了解决这个问题,BESIII合作计划用三层圆柱三层燃气电子乘数(CGEM)替换MDC的内部。 CGEM的横平空间分辨率必须为120美元或更高。为了满足这一目标,必须对检测器进行仔细的校准,以充分利用CGEM检测器的潜力。在所有校准中,检测器对齐起着提高检测器精度的重要作用。 CGEM探测器与Milleepede算法的基于轨道的对齐是为了减少命中位置测量的不确定性。使用两层设置在2020年获得的宇宙射线数据,外层相对于内层的位移和旋转由同时应用于160000多个轨道的同时拟合确定。已经达到了良好的一致性精度,可以保证将来可以满足设计请求。将CGEM安装到BESIII检测器后,将使用来自宇宙射线的曲目和碰撞的曲目组合信息进行进一步的对齐。
The Beijing Electron Spectrometer III (BESIII) is a multipurpose detector operating on the Beijing Electron Positron Collider II (BEPCII). After more than ten year's operation, the efficiency of the inner layers of the Main Drift Chamber (MDC) decreased significantly. To solve this issue, the BESIII collaboration is planning to replace the inner part of the MDC with three layers of Cylindrical triple Gas Electron Multipliers (CGEM). The transverse plane spatial resolution of CGEM is required to be 120 $μ$m or better. To meet this goal, a careful calibration of the detector is necessary to fully exploit the potential of the CGEM detector. In all the calibrations, the detector alignment plays an important role to improve the detector precision. The track-based alignment for the CGEM detector with the Millepede algorithm is implemented to reduce the uncertainties of the hit position measurement. Using the cosmic-ray data taken in 2020 with the two layers setup, the displacement and rotation of the outer layer with respect to the inner layer is determined by a simultaneous fit applied to more than 160000 tracks. A good alignment precision has been achieved that guarantees the design request could be satisfied in the future. A further alignment is going to be performed using the combined information of tracks from cosmic-ray and collisions after the CGEM is installed into the BESIII detector.