Dark matter candidate with new strong interactions

被引：16

作者：

Banks, T ^{[1
]}

Mason, JD

O'Neil, D

机构：

[1] Rutgers State Univ, NHETC, Dept Phys & Astron, Princeton, NJ 08540 USA

[2] Univ Calif Santa Cruz, SCIPP, Dept Phys, Santa Cruz, CA 95064 USA

来源：

PHYSICAL REVIEW D | 2005年 / 72卷 / 04期

关键词：

D O I：

10.1103/PhysRevD.72.043530

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We study the possibility that dark matter is a baryon of a new strongly interacting gauge theory, which was introduced in the low energy theory of Cosmological SUSY Breaking (CSB). This particle can fit the observed dark matter density if an appropriate cosmological asymmetry is generated. The same mechanism can also explain the dark/baryonic matter ratio in the universe. The mass of the dark matter particle is in the multiple TeV range, and could be as high as 20 TeV.

引用

页码：1 / 5

页数：5

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