直接探测非质子暗物质
天体物理学
2007-05-23 v1
摘要
弱相互作用巨质子 (WIMP) 是宇宙质量密度主导部分的主要候选物。本文通过举例介绍当前正在运行的实验，并呈现最具前景的未来项目，综述直接WIMP探测技术。
引用
@article{arxiv.astro-ph/0003434,
title = {Direct Detection of Nonbaryonic Dark Matter},
author = {Laura Baudis and H. V. Klapdor-Kleingrothaus},
journal= {arXiv preprint arXiv:astro-ph/0003434},
year = {2007}
}
备注
18 pages, latex, 8 eps figures, requires iopconf1.sty. To appear in Proceedings of Beyond the Desert '99, Second International Conference on Physics beyond the Standard Model, Castle Ringberg, Tegernsee, Germany, 6-12 June 1999