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
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
收藏
页码:176 / 182
页数:7
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