超对称大统一中的暗物质
高能物理 - 唯象学
2008-02-03 v2 天体物理学
摘要
在受约束的最小超对称标准模型中，bino型最轻超对称粒子是唯一的暗物质中性候选者。因此，在不引入定义不明确的精细调节约束的情况下，通常可以将所有超对称质量谱限制在约1-2 TeV以下。
关键词
引用
@article{arxiv.hep-ph/9405363,
title = {Dark Matter from Supersymmetric Grand Unification},
author = {G. L. Kane and Chris Kolda and Leszek Roszkowski and James D. Wells},
journal= {arXiv preprint arXiv:hep-ph/9405363},
year = {2008}
}
备注
invited talk given by LR at the Astrophysics Symposium and Workshop on Dark Matter ``Critique of the Sources of Dark Matter in the Universe'', Los Angeles, California, February 16--18, 1994; 14 pages of text in Latex plus 4 figures in PS (3 included, 1 available by email); University of Michigan preprint UM-TH-94-17 (April 1994). CHANGES: 3 figures added, abstract in the listing corrected