Implications of new CMB data for neutralino dark matter

被引:94
作者
Barger, V
Kao, C
机构
[1] Univ Wisconsin, Dept Phys, Madison, WI 53706 USA
[2] Univ Oklahoma, Dept Phys & Astron, Norman, OK 73019 USA
关键词
D O I
10.1016/S0370-2693(01)01046-2
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The combination of new cosmic microwave background data with cosmological priors has determined the physical cold dark matter (cdm) density to be Ωcdmh2 = 0.13 ± 0.01. We find the corresponding regions of parameters in the minimal supergravity model for which the lightest neutralino is the cdm particle. We then compare with the muon anomalous magnetic moment (aμ) measurement, the mass of the lighter CP-even Higgs boson (h0), the trilepton search at the upgraded Fermilab Tevatron collider, and a direct search for relic neutralinos. The intersection of Ωcdmh2 and aμ constraints selects tan β ≈ 40-45. © 2001 Published by Elsevier Science B.V.
引用
收藏
页码:117 / 122
页数:6
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