Dark matter, massive neutrinos and SUSY particles

被引：0

作者：

Pretzl, K ^{[1
]}

机构：

[1] Univ Bern, High Energy Phys Lab, CH-3012 Bern, Switzerland

来源：

STRUCTURE AND DYNAMICS OF ELEMENTARY MATTER | 2004年 / 166卷

关键词：

D O I：

暂无

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

Recent experimental observations show that the universe is flat and consists of 27% matter and 73% dark energy. Most of the matter is invisible and of unknown nature. Weakly interacting massive particles (so-called WIMPs) like massive neutrinos and/or particles predicted by Super Symmetry (SUSY) are possible candidates for the dark matter in the universe. The latest developments in this field of research and the possible direct search for WIMPs with earthbound detectors is discussed in this paper.

引用

页码：289 / 302

页数：14

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