Limits on WIMP dark matter using sapphire cryogenic detectors

被引：179

作者：

Angloher, G

Bruckmayer, M

Bucci, C

Bühler, M

Cooper, S

Cozzini, C

DiStefano, P

von Feilitzsch, F

Frank, T

Hauff, D

Jagemann, T

Jochum, J

Jörgens, V

Keeling, R

Kraus, H

Loidl, M

Marchese, J

Meier, O

Nagel, U

Pröbst, F

Ramachers, Y

Rulofs, A

Schnagl, J

Seidel, W

Sergeyev, I

Sisti, M

Stark, M

Uchaikin, S

Stodolsky, L

Wulandari, H

Zerle, L

机构：

[1] Max Planck Inst Phys & Astrophys, D-80805 Munich, Germany

[2] Univ Oxford, Dept Phys, Oxford OX1 3RH, England

[3] Lab Nazl Gran Sasso, I-67010 Coppito, Italy

[4] Tech Univ Munich, Dept Phys, D-85747 Munich, Germany

[5] Joint Inst Nucl Res, Dubna 141980, Russia

来源：

ASTROPARTICLE PHYSICS | 2002年 / 18卷 / 01期

关键词：

D O I：

10.1016/S0927-6505(02)00111-1

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Data taken by CRESST with a cryogenic detector system based on 262 g sapphire crystals has been used to place limits on WIMP dark matter in the Galactic Halo. The experiment was especially sensitive for low-mass WIMPs with spin-dependent cross sections and improves on existing limits in this region. (C) 2002 Elsevier Science B.V. All rights reserved.

引用

页码：43 / 55

页数：13

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