多气隙电阻板室的宇宙线测量结果

介绍了20多个多气隙电阻板室的宇宙线测量结果.测量所用的宇宙线平台可以同时测量同一个电阻板室的多个cell,其参考时间的时间分辨为70ps.在宇宙线的测量条件下,用国产材料制作的多气隙电阻板室的时间分辨可达到90ps.利用这套宇宙线测量系统,还对多气隙电阻板室的探测效率和cell间的相互串扰进行了研究.     

Micromegas prototypes with thermo-bond film separators

In this paper we report the results of Micromegas prototypes constructed by attaching micromesh to an anode using thermo-bond films. The excellent metal attaching ability and good dielectical property of this kind of film make it a promising material to be used as avalanche gap spacers. Several prototypes are successfully made. The electron transmission properties are first studied and then the gas gain is measured in argon-isobutane mixtures. The maximum gain of more than 10⁴ is easily obtained. The energy resolutions for ⁵⁵Fe 5.9 keV K_α ray can be better than 20% over one magnitude in gain for different operational gas mixtures and the best energy resolution of 13.7% (FWHM) can be achieved with the gas mixture of 94% argon concentration. The preliminary test results of the prototypes with sensitive area of 45 mm×45 mm without internal support show good uniformity across the sensitive area.     

一种新型时间测量探测器──多气隙电阻板室

介绍了具有6层气隙的电阻板室的结构和工作原理.用动量7GeV/c的粒子束测量了该探测器的性能,得到时间分辨为60—70ps,探测效率大于97%.在动量为3GeV/c的正电荷粒子束流测试中,用该探测器获得了p和π的时间谱,实现了很好的粒子分辨.     

闪烁光纤时间特性的蒙特卡罗模拟

用蒙特卡罗模拟的方法，研究了影响闪烁光纤时间分辨的物理因素，包括光子在光纤中的发射，传输，吸收和最后在光电倍增管输出端形成电泳冲等过程，并和实验结果进行了比较。     

A fast luminosity monitor for BEPCⅡ

The fast luminosity monitor counting the γ photons above a given energy threshold emitted from radiative Bhabha scattering has been operated in the BEPC Ⅱ to measure the relative luminosity bunch by bunch for the first time and used successfully in beam tuning of BEPC Ⅱ. In the relative mode the monitor is able to deliver the relative luminosities with an accuracy of 0.8 %. By steering the electron beam while observing the counting rate changes of the monitor the horizontal and vertical sizes of the bunch spots can be estimated as： Sxe＋ =Sxe =0.356 mm, Sye＋ =Sye- =0.011 mm.     

A new gaseous detector — micro mesh gaseous structure

The structure and working principle of Micromegas （MICRO Mesh Gaseous Structure） is discussed. Some radiation sources of α and X rays are used to test this detector. The optimized electric-field intensity of the conversion gap is obtained. The transmission of electrons and the uniformity of the amplification gap are also presented. The energy resolution of the 5.9 keV peak is better than 27%.     

Delay line readout of a large dimension multi-wire proportional chamber

A two dimensional multi-wire proportional chamber with delay line readout was developed, which has a large sensitive area of 30 cm× 30 cm. Two cathode planes using printed circuit boards are orthogonally placed to give two coordinates of the impact point of the particle. Signals collected from the cathode strips are amplified and discriminated from two ends of the delay line at each cathode board. By recording the time difference between the two discrimination pulses and the common gate pulse from anode wires, a coordinate position was reconstructed, and a position resolution of better than 1 mm could be obtained in the whole sensitive area along the anode wires.     

TOFr在STAR实验中的标定方法

基于多气隙电阻板室(MRPC)的STAR飞行时间探测器的一个板条的原型(TOFr)参加了2003年STAR实验的质子–质子对撞和氘–金对撞的物理运行.利用STAR实验中原有的赝顶点位置探测器(pVPD)和时间投影室(TPC),结合TOFr的时间及幅度信号,并考虑TOFr每个探测单元的尺寸,对影响时间分辨的各种因素进行了修正,实现了对TOFr的标定.实验数据给出的TOFr的本征时间分辨为85ps,在两倍标准方差下,其对π/K及K/p分辨的动量分别达到了1.6GeV/c和3.0GeV/c,大大提高了STAR探测器的粒子鉴别能力.     

(S_(nn))~(1/2)=200GeV下Au-Au中心碰撞中Di-omega产额上限的蒙特卡罗模拟(英文)

根据现有的关于(ΩΩ)0 的生成截面的理论计算,利用HIJING事例产生器研究了(S_(nn))~(1/2)=200GeV下Au- Au中心碰撞中(ΩΩ)0 和(NΩ)022产生过程,分别对(ΩΩ)0 的电磁作用产生过程和两步产生过程中的第一步过程进行了(ΩΩ)0 产率的计算,给出了(ΩΩ)0 产额的上限,对于电磁作用过程,其产率为(1.097±0.293)×10-10 同时我们也对(NΩ)022进行了初步的模拟,初步给出了它的产率为(0.894±0.005)×10-4.     

一个高时间分辨的多间隙电阻板室原型

研制了一种多气隙电阻板室原型并建立了相关的测试系统.利用宇宙线测试系统和欧洲核子中心的试验束装置T1?0对其性能进行了测试,给出了初步结果.时间分辨达到70ps,对最小电离粒子的探测效率大于95%.