CRESST暗物质搜索的结果与计划
天体物理学
2007-05-23 v1
摘要
CRESST于2000年使用基于262克砖石晶体的制冷探测器系统所采集的数据用于限制银河暗 halo中的WIMP暗物质。该探测器对低质量WIMP（具有自旋相关截面）尤其敏感，并在该区域改进了现有限制。CRESST正在为第二阶段做准备，该阶段将使用10公斤探测器，包含300克CaWO4晶体，同时检测声子和色素发光以降低背景。
引用
@article{arxiv.astro-ph/0106314,
title = {Results and plans of the CRESST dark matter search},
author = {M. Altmann and G. Angloher and M. Bruckmayer and C. Bucci and S. Cooper and C. Cozzini and P. DiStefano and F. von Feilitzsch and T. Frank and D. Hauff and Th. Jagemann and J. Jochum and R. Keeling and H. Kraus and J. Macallister and F. Proebst and Y. Ramachers and J. Schnagl and W. Seidel and I. Sergeyev and M. Stark and L. Stodolsky and H. Wulandari},
journal= {arXiv preprint arXiv:astro-ph/0106314},
year = {2007}
}
备注
23 pages, 15 figures, Paper contributed to the X International Symposium on Lepton and Photon Interactions at High Energies, 23rd-28th July 2001, Rome, Italy