Uncertainties in the Prediction of the Relic Density of Supersymmetric Dark Matter

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dc.creatorAllanach, B. C.
dc.creatorBélanger, G.
dc.creatorBoudjema, F.
dc.creatorPukhov, A.
dc.date2004-10-04
dc.date.accessioned2026-07-07T03:53:35Z
dc.date.available2026-07-07T03:53:35Z
dc.descriptionWe investigate how well the relic density of dark matter can be predicted in mSUGRA. We determine the parameters to which the relic density is most sensitive and quantify the collider accuracy needed to match the accuracy of WMAP and PLANCK.
dc.description4 pages, 1 figure, presented at LCWS, Paris, April 2004
dc.identifierhttps://arxiv.org/abs/hep-ph/0410049
dc.identifierhttp://arxiv.org/abs/hep-ph/0410049
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/43895
dc.subjectHigh Energy Physics - Phenomenology
dc.titleUncertainties in the Prediction of the Relic Density of Supersymmetric Dark Matter
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