Dark matter from particle physics

被引：2

作者：

Kane, GL ^{[1
]}

机构：

[1] Univ Michigan, Randall Lab Phys, Ann Arbor, MI 48109 USA

来源：

PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS | 1998年 / 307卷 / 1-4期

关键词：

95.35.+d*; ■;

D O I：

10.1016/S0370-1573(98)00043-X

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Eventually, the properties of particles relevant to the possible amounts of dark matter from various particle physics sources (lightest superpartner (LSP), massive neutrinos, axions, etc.) will be well determined. I discuss how well Omega(LSP)h(2) can be calculated once there is collider data on the properties of the LSP. Study of the supersymmetry Lagrangian implies that current limits on WIMPs are not general. (C) 1998 Elsevier Science B.V. All rights reserved.

引用

页码：197 / 200

页数：4

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