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Relic density of dark matter in mSUGRA and non-universal SUGRA
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Relic density of dark matter in mSUGRA and non-universal SUGRA
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hep-ph
keywords
densitymodelsrelicdarkmattermsugrabinoconstrain
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The measurements of WMAP on the relic density of dark matter strongly constrain supersymmetric models. In mSUGRA where the neutralino LSP is mostly a bino only rather fine-tuned models survive. On the other hand the relic density upper limit can be easily satisfied in models with a Higgsino or wino LSP.
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