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

页码：312 / 314

页数：3

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