Relic density of dark matter in mSUGRA and non-universal SUGRA

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dc.creatorBelanger, G.
dc.creatorBoudjema, F.
dc.creatorCottrant, A.
dc.creatorPukhov, A.
dc.creatorSemenov, A.
dc.date2004-12-21
dc.date.accessioned2026-07-07T06:26:33Z
dc.date.available2026-07-07T06:26:33Z
dc.descriptionThe 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.
dc.description8 pages, 3 figures, Invited talk at Physics at LHC, Vienna, July 2004
dc.identifierhttps://arxiv.org/abs/hep-ph/0412309
dc.identifierhttp://arxiv.org/abs/hep-ph/0412309
dc.identifierCzech.J.Phys. 55 (2005) B205-B212
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/97141
dc.subjectHigh Energy Physics - Phenomenology
dc.titleRelic density of dark matter in mSUGRA and non-universal SUGRA
dc.typetext

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