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arXiv physics/0602045physics.ins-det
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气体纯度对GEM在He和Ne中低温性能的影响

Gas Purity effect on GEM Performance in He and Ne at Low Temperatures

R. Galea, J. Dodd, Y. Ju, M. Leltchouk, W. Willis, P. Rehak, V. Tcherniatine, A. Buzulutskov, D. Pavlyuchenko

摘要:

在3-293 K温度范围内研究了气体电子倍增器(GEMs)在He、Ne、He+ H_2和Ne+ H_2中的性能。本文报道了以前发表的测量和额外的研究中的GEM性能进行评估的气体的纯度的影响。在他,在77和293 K之间的温度,三创业板结构在相当高的增益,超过1000。有迹象表明,这种高增益是通过气体中的杂质导致的潘宁效应实现的。在较低的温度下,增益电压特性显着修改可能是由于这些杂质的冻结。双GEM和单GEM结构可以在气体密度约为0.5 g/l时以仅达到几十的增益工作到3 K;在更高的密度下,最大增益进一步下降。在Ne中,最大增益也在低温下下降。在Ne+ H_2的Penning混合物中可以重新建立低温下Ne的增益下降:在30-77 K下,在相当于27 K下饱和Ne蒸气密度的9.2 g/l的密度下,在这些混合物中获得了超过104的非常高的增益。在He中添加少量H2也在30 K以上重新建立大的GEM增益,但在4 K和1.7 g/l的密度(对应于大约十分之一的饱和蒸气密度)下在He+H2中没有观察到增益。这些研究的一部分是在研制用于探测太阳中微子的两相He和Ne探测器时进行的。

英文摘要:

The performance of Gas Electron Multipliers (GEMs) in gaseous He, Ne, He+H2 and Ne+H2 was studied at temperatures in the range of 3-293 K. This paper reports on previously published measurements and additional studies on the effects of the purity of the gases in which the GEM performance is evaluated. In He, at temperatures between 77 and 293 K, triple-GEM structures operate at rather high gains, exceeding 1000. There is an indication that this high gain is achieved through the Penning effect as a result of impurities in the gas. At lower temperatures the gain-voltage characteristics are significantly modified probably due to the freeze-out of these impurities. Double-GEM and single-GEM structures can operate down to 3 K at gains reaching only several tens at a gas density of about 0.5 g/l; at higher densities the maximum gain drops further. In Ne, the maximum gain also drops at cryogenic temperatures. The gain drop in Ne at low temperatures can be re-established in Penning mixtures of Ne+H2: very high gains, exceeding 104, have been obtained in these mixtures at 30-77 K, at a density of 9.2 g/l which corresponds to saturated Ne vapor density at 27 K. The addition of small amounts of H2 in He also re-establishes large GEM gains above 30 K but no gain was observed in He+H2 at 4 K and a density of 1.7 g/l (corresponding to roughly one-tenth of the saturated vapor density). These studies are, in part, being pursued in the development of two-phase He and Ne detectors for solar neutrino detection.

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