Supersymmetric dark matter in light of WMAP

John Ellis; Keith A. Olive; Yudi Santoso; Vassilis C. Spanos

doi:10.1016/S0370-2693(03)00765-2

Supersymmetric dark matter in light of WMAP

John Ellis, Keith A. Olive, Yudi Santoso, Vassilis C. Spanos

Physics and Astronomy (Twin Cities)

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375 Scopus citations

Abstract

We re-examine the parameter space of the constrained minimal supersymmetric extension of the Standard Model (CMSSM), taking account of the restricted range of ω_CDMh² consistent with the WMAP data. This provides a significantly reduced upper limit on the mass of the lightest supersymmetric particle LSP: mχ ≲ 500 GeV for tan β≲ 45 and μ > 0, or tan β ≲ 30 and μ < 0, thereby improving the prospects for measuring supersymmetry at the LHC, and increasing the likelihood that a 1-TeV linear e⁺e^- collider would be able to measure the properties of some supersymmetric particles.

Original language	English (US)
Pages (from-to)	176-182
Number of pages	7
Journal	Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
Volume	565
Issue number	1-4
DOIs	https://doi.org/10.1016/S0370-2693(03)00765-2
State	Published - Jul 17 2003

Bibliographical note

Funding Information:
We would like to thank H. Baer and A. Belyaev for helpful discussions. The work of K.A.O., Y.S., and V.C.S. was supported in part by DOE grant DE-FG02-94ER-40823.

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Supersymmetric dark matter in light of WMAP

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