Non-baryonic dark matter

被引：2
|
作者：
Bergstrom, L [1 ]
机构：
[1] Stockholm Univ, Dept Phys, SE-11385 Stockholm, Sweden
来源：
NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS | 1999年 / 70卷
关键词：
D O I：
10.1016/S0920-5632(98)00385-5
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：
The need for dark matter is briefly reviewed. A wealth of observational information points to the existence of a non-baryonic component. To the theoretically favoured candidates today belong axions, supersymmetric particles, and to some extent massive neutrinos. The theoretical foundation and experimental situation for each of these is reviewed. In particular, indirect detection methods of supersymmetric dark matter are described. Present experiments are just reaching the required sensitivity to discover or rule out some of these candidates, and major improvements are planned over the next few years.
引用
收藏
页码：31 / 42
页数：12
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