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We examine the stau-neutralino coannihilation (CA) mechanism of the early universe.
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PGS is a parameterized detector simulator. We use version 4 ( http://www.physics.ucdavis.edu/~conway/research/software/pgs/pgs4-general.htm ) in the CMS detector configuration. We assume the τ \tau identification efficiency with p T vis > 20 GeV \mbox{$p_{\rm T}^{\rm vis}$}>20\ \mbox{${\rm GeV}$} is 50%, while the probability for a jet being mis-identified as a τ \tau is 1%
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All uncertainties are statistical. The systematic uncertainties will be evaluated correctly once the LHC starts
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The Ω χ ~ 1 0 h 2 \Omega_{\mbox{$\tilde{\chi}_{1}^{0}$}}h^{2} is calculated at tree-level. Since the dominant diagrams involve only non-colored particles the one loop QCD corrections are also very small
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