Natural Dark Matter

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dc.creatorKing, S. F.
dc.creatorRoberts, J. P.
dc.date2006-09-15
dc.date2006-09-25
dc.date.accessioned2026-07-07T10:25:26Z
dc.date.available2026-07-07T10:25:26Z
dc.descriptionIn this talk we analyse the claim that supersymmetry (SUSY) naturally accounts for the observed dark matter density. In many cases, it is necessary to tune the parameters of a SUSY model to fit the WMAP data. We provide a quantitative analysis of the degree of tuning required for different annihilation channels. Some regions are natural, requiring no tuning at all, whereas others require tuning at the 0.1% level.
dc.descriptionReference added. Based on talk given at Physics at the LHC 2006, Cracow, Poland, 3-8 Jul 2006
dc.identifierhttps://arxiv.org/abs/hep-ph/0609147
dc.identifierhttp://arxiv.org/abs/hep-ph/0609147
dc.identifierActaPhys.Polon.B38:607-616,2007
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/176543
dc.subjectHigh Energy Physics - Phenomenology
dc.titleNatural Dark Matter
dc.typetext

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