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首页> 外文期刊>Nuclear Instruments & Methods in Physics Research. Section A, Accelerators, Spectrometers, Detectors and Associated Equipment >Time-of-flight resolution of scintillating counters with Burle 85001 microchannel plate photomultipliers in comparison with Hamamatsu R2083
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Time-of-flight resolution of scintillating counters with Burle 85001 microchannel plate photomultipliers in comparison with Hamamatsu R2083

机译:Burle 85001微通道平板光电倍增管与Hamamatsu R2083相比,闪烁计数器的飞行时间分辨率

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摘要

Improvements in the time resolution of the CEBAF Large Acceptance Spectrometer (CLAS) below approximate to 50ps will be required for experiments using the planned upgraded accelerator facility at Jefferson Lab. The improved time resolution will allow particle identification using time-of-flight techniques to be used effectively up to the proposed operating energy of 12GeV. The challenge of achieving this time resolution over a relatively large area is compounded because the photomultipliers (PM) in the CLAS "time-zero" scintillating counters must operate in very high magnetic fields. Therefore, we have studied the resolution of "time-zero" prototypes with microchannel plate PMs 85001-501 from Burle. For reference and comparison, measurements were also made using the standard PMs R2083 from Hamamatsu using two timing methods. The cosmic ray method, which utilizes three identical scintillating counters (Bicron BC-408, 2 x 3 x 50cm(3)) with PMs at the ends, yields sigma(R2083) = 59.1 +/- 0.7 ps. The location method of particles from a radiative source with known coordinates has been used to compare timing resolutions of R2083 and 85001-501. This method yields sigma(R2083) = 59.5 +/- 0.7 ps and it also provides an estimate of the number of primary photoelectrons. For the microchannel plate PM from Burle the method yields sigma(85001) = 130 +/- 4 ps due to lower number of primary photoelectrons. (c) 2006 Elsevier B.V. All rights reserved.
机译:对于使用杰斐逊实验室计划中的升级加速器设施进行的实验,CEBAF大验收谱仪(CLAS)的时间分辨率必须低于50ps。改进的时间分辨率将允许使用飞行时间技术进行粒子识别,直至建议的12GeV工作能量有效使用。由于在CLAS“零时间”闪烁计数器中的光电倍增器(PM)必须在非常高的磁场中运行,因此在相对较大的区域上实现此时间分辨率的挑战更加复杂。因此,我们使用Burle的微通道板PMs 85001-501研究了“零时光”原型的分辨率。作为参考和比较,还使用Hamamatsu的标准PM R2083进行了两种计时方法的测量。宇宙射线方法使用三个相同的闪烁计数器(Bicron BC-408,2 x 3 x 50cm(3)),两端带有PM,产生sigma(R2083)= 59.1 +/- 0.7 ps。来自具有已知坐标的辐射源的粒子的定位方法已用于比较R2083和85001-501的时间分辨率。此方法产生的sigma(R2083)= 59.5 +/- 0.7 ps,并且还提供了一次光电子数量的估计。对于Burle的微通道板PM,由于一次光电子的数量较少,该方法的sigma(85001)= 130 +/- 4 ps。 (c)2006 Elsevier B.V.保留所有权利。

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