Detection of the primary scintillation light from dense Ar, Kr and Xe with novel photosensitive gaseous detectors

被引:105
作者
Periale, L
Peskov, V
Carlson, P
Francke, T
Pavlopoulos, P
Picchi, P
Pietropaolo, F
机构
[1] Royal Inst Technol, S-10044 Stockholm, Sweden
[2] Univ Turin, I-10126 Turin, Italy
[3] CERN, CH-1211 Geneva, Switzerland
[4] Ist Nazl Fis Nucl, I-35131 Padua, Italy
关键词
primary scintillation; micropattern gaseous detectors; CsI photocathode; GEM; capillaries;
D O I
10.1016/S0168-9002(01)01779-X
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
The detection of primary scintillation light in combination with the charge or secondary scintillation signals is an efficient technique in determining the events "t = 0" as well as particle photon separation in large mass TPC detectors filled with noble gases and/or condensed noble gases. The aim of this work is to demonstrate that costly photo-multipliers could be replaced by cheap novel photosensitive gaseous detectors: wire counters, GEMs or glass capillary plates coupled wish CsI photocathodes. We have performed systematic measurements with Ar, Kr And Xe gases at pressures in the range of 1-50 atm as well as some preliminary measurements with liquid Xe and liquid Ar. With the gaseous detectors we have succeeded in detecting a scintillation light produced by 22 KeV X-rays with an efficiency close to 100%. We also detected the scintillation light produced by beta's (5 keV deposit energy) with an efficiency close to 25%. Successful detection of scintillation from 22 keV X-rays open new experimental possibilities not only for nTOF and ICARUS experiments, but also in others, such as WIMP's search through nuclear recoil emission. (C) 2002 Elsevier Science B.V. All rights reserved.
引用
收藏
页码:377 / 383
页数:7
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