Response of superheated droplet detectors of the PICASSO dark matter search experiment

被引:63
作者
Barnabé-Heider, M
Di Marco, M
Doane, P
Genest, MH
Gornea, R
Guénette, R
Leroy, C [1 ]
Lessard, L
Martin, JP
Wichoski, U
Zacek, V
Clark, K
Krauss, CB
Noble, AJ
Behnke, E
Feighery, W
Levine, I
Muthusi, C
Kanagalingam, S
Noulty, R
机构
[1] Univ Montreal, Dept Phys, Montreal, PQ H3C 3J7, Canada
[2] Queens Univ, Dept Phys, Kingston, ON K7L 3NG, Canada
[3] Indiana Univ, Dept Phys & Astron, South Bend, IN 46634 USA
[4] Indiana Univ, Dept Chem, South Bend, IN 46634 USA
[5] Bubble Technol Ind, Chalk River, ON K0J 1J0, Canada
基金
加拿大自然科学与工程研究理事会; 加拿大创新基金会;
关键词
detectors; cold dark matter; superheated droplet detectors; neutrons; alpha particles;
D O I
10.1016/j.nima.2005.09.015
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
We present results of systematic studies of the radiation response of superheated liquid droplet detectors, which are used in the PICASSO dark matter search experiment. This detection technique is based on the phase transitions of superheated liquid Freon droplets dispersed and trapped in a polymerized gel. Phase transitions can be induced by nuclear recoils following particle interactions and, in particular, interactions with Weakly Interacting Massive Particles (WIMPs). These detectors are threshold devices since a minimal energy deposition is necessary to induce a phase transition and their sensitivity to various types of radiation depends strongly on the operating temperature and pressure. The sensitivity to neutrons, g-particles and T-rays was determined as a function of these operating parameters and the results are compared with simulations. In particular, we present a complete characterization of the response of detector modules already in use for a dark matter search at the SNO site to detect WIMPs and discuss possible background sources. (c) 2005 Elsevier B.V. All rights reserved.
引用
收藏
页码:184 / 204
页数:21
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