低温暗物质搜索（CDMS）对 WIMP-核子截面给出的初步限制
天体物理学
2008-11-26 v1
摘要
我们正在开展一项实验，利用地面探测器搜寻银河系晕中的 WIMP（弱相互作用大质量粒子）。这一类假想粒子，其性质类似于粒子物理标准模型扩展所预言的性质，可能构成非重子暗物质的冷组分。我们描述了我们的实验，该实验基于低温恒温器中屏蔽的低本底锗和硅探测器。探测器通过同时测量声子和电离中的能量，实现了高程度的本底排斥。利用实验初始运行中约一千千克·天的曝光量，我们获得了与其他实验长时间运行结果相当的（初步的）WIMP-核子截面上限。
引用
@article{arxiv.astro-ph/9712343,
title = {Preliminary Limits on the WIMP-Nucleon Cross Section from the Cryogenic Dark Matter Search (CDMS)},
author = {DS Akerib and PD Barnes and DA Bauer and PL Brink and B Cabrera and DO Caldwell and RM Clarke and A Da Silva and AK Davies and BL Dougherty and KD Irwin and RJ Gaitskell and SR Golwala and EE Haller and J Jochum and WB Knowlton and V Kuzminov and SW Nam and V Novikov and MJ Penn and TA Perera and RR Ross and B Sadoulet and RW Schnee and T Shutt and A Smith and AH Sonnenschein and AL Spadafora and WK Stockwell and S Yellin and BA Young},
journal= {arXiv preprint arXiv:astro-ph/9712343},
year = {2008}
}
备注
5 LaTex pages, 5 eps figs, epsf.sty, espcrc2dsa2.sty. Proceedings of TAUP97, Gran Sasso, Italy, 7-11 Sep 1997, Nucl. Phys. Suppl., A. Bottino, A. di Credico and P. Monacelli (eds.). See also http://cfpa.berkeley.edu