The CRESST dark matter experiment:: status and perspectives

被引：11
|
作者：
Sisti, M
Bravin, M
Bruckmayer, M
Bucci, C
Cooper, S
Di Stefano, P
Giordano, S
Von Feilitzsch, F
Frank, T
Jochum, J
Keeling, R
Kraus, H
Loidl, M
Marchese, J
Meier, O
Meunier, P
Nagel, U
Pergolesi, D
Pröbst, F
Ramachers, Y
Schnagl, J
Seidel, W
Sergeyev, I
Stodolsky, L
Uchaikin, S
Zerle, L
机构：
[1] Max Planck Inst Phys, D-80805 Munich, Germany
[2] Univ Oxford, Dept Phys, Oxford OX1 3RH, England
[3] Lab Nazl Gran Sasso, I-67010 Assergi, AQ, Italy
[4] Tech Univ Munich, D-85747 Garching, Germany
来源：
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT | 2000年 / 444卷 / 1-2期
关键词：
D O I：
10.1016/S0168-9002(99)01405-9
中图分类号：
TH7 [仪器、仪表];
学科分类号：
0804 ; 080401 ; 081102 ;
摘要：
The CRESST experiment in its first phase is using sapphire detectors with tungsten phase transition thermometers to search for dark matter WIMPs. At present Four 262 g detectors are performing first measurements under low background conditions. Detector performance as well as preliminary results from the background runs are presented. A second phase of CRESST using CaWO4 and simultaneous measurement of phonons and scintillation light is in preparation. (C) 2000 Elsevier Science B.V. All rights reserved.
引用
收藏
页码：312 / 314
页数：3
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