Dark matter search with CRESST cryogenic detectors

被引：7

作者：

Angloher, G ^{[1
]}

Altmann, M ^{[1
]}

Bruckmayer, M ^{[1
]}

Bucci, C ^{[1
]}

Cooper, S ^{[1
]}

Cozzini, C ^{[1
]}

Di Stefano, P ^{[1
]}

von Feilitzsch, F ^{[1
]}

Frank, T ^{[1
]}

Hauff, D ^{[1
]}

Jagemann, T ^{[1
]}

Jochum, J ^{[1
]}

Keeling, R ^{[1
]}

Kraus, H ^{[1
]}

Macallister, J ^{[1
]}

Pröbst, F ^{[1
]}

Ramachers, Y ^{[1
]}

Schnagl, J ^{[1
]}

Seidel, W ^{[1
]}

Sergeyev, I ^{[1
]}

Stark, M ^{[1
]}

Stodolsky, L ^{[1
]}

Wulandari, H ^{[1
]}

机构：

[1] Univ Oxford, Dept Phys, Oxford, England

来源：

PHYSICS OF ATOMIC NUCLEI | 2003年 / 66卷 / 03期

关键词：

D O I：

10.1134/1.1563712

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

Results of the CRESST experiment at Gran Sasso using 262-g sapphire calorimeters with tungsten phase transition thermometers are presented. Calibration and analysis methods are described. Data taken in 2000 have been used to place limits on WIMP dark matter particles in the Galactic halo. The sapphire defectors are especially sensitive to low-mass WIMPs with spin-dependent interaction and improve on existing limits in this region. (C) 2003 MAIK "Nauka/Interperiodica".

引用

页码：494 / 496

页数：3

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