Status and low background considerations for the CRESST dark matter search

被引：33

作者：

Buhler, M

Zerle, L

Probst, F

Rulofs, A

Schanda, U

Seidel, W

Absmaier, C

Booth, NE

Bucci, C

Colling, P

Cooper, S

vonFeilitzsch, F

Ferger, P

Forster, G

Gabutti, A

Hoss, C

Hohne, J

Igalson, J

Kellner, E

Koch, M

Loidl, M

Meier, O

Nucciotti, A

Nagel, U

vanderPuute, MJJ

Salmon, GL

Sisti, M

Stodolsky, L

Stolovich, A

机构：

[1] TECH UNIV MUNICH,D-85747 GARCHING,GERMANY

[2] MAX PLANCK INST PHYS & ASTROPHYS,D-80805 GARCHING,GERMANY

[3] UNIV OXFORD,OXFORD OX1 3RH,ENGLAND

[4] LAB NAZL GRAN SASSO,I-67010 ASSERGI,ITALY

[5] POLISH ACAD SCI,INST PHYS,PL-02668 WARSAW,POLAND

[6] INST CHEM PHYS & BIOPHYS,TALLINN 0026,ESTONIA

[7] INST PHYS,TARTU 2400,ESTONIA

来源：

NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT | 1996年 / 370卷 / 01期

关键词：

D O I：

10.1016/0168-9002(95)01095-5

中图分类号：

TH7 [仪器、仪表];

学科分类号：

0804 ; 080401 ; 081102 ;

摘要：

We are preparing the CRESST experiment to search for dark matter WIMPs using cryogenic detectors with superconducting phase transition thermometers. In the first stage we plan to use four 250 g sapphire detectors with thresholds of 0.5 keV and resolutions of 0.2 keV at 1 keV. This will provide sensitivity to WIMP masses below 10 GeV, and is thus complementary to other dark matter searches.

引用

页码：237 / 240

页数：4

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