Supersymmetric dark matter in light of WMAP

被引：345

作者：

Ellis, J ^{[1
]}

Olive, KA

Santoso, Y

Spanos, VC

机构：

[1] CERN, Div TH, CH-1211 Geneva, Switzerland

[2] Univ Minnesota, William I Fine Theoret Phys Inst, Minneapolis, MN 55455 USA

来源：

PHYSICS LETTERS B | 2003年 / 565卷 / 1-4期

关键词：

D O I：

10.1016/S0370-2693(03)00765-2

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We re-examine the parameter space of the constrained minimal supersymmetric extension of the Standard Model (CMSSM), taking account of the restricted range of Omega(CDM)h(2) consistent with the WMAP data. This provides a significantly reduced upper limit on the mass of the lightest supersymmetric particle LSP: m(chi) less than or similar to 500 GeV for tan beta less than or similar to 45 and mu > 0, or tan beta less than or similar to 30 and mu < 0, thereby improving the prospects for measuring supersymmetry at the LHC, and increasing the likelihood that a 1-TeV linear a(+)e(-) collider would be able to measure the properties of some supersymmetric particles. (C) 2003 Published by Elsevier B.V.

引用

页码：176 / 182

页数：7