2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/176543In 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.Reference added. Based on talk given at Physics at the LHC 2006, Cracow, Poland, 3-8 Jul 2006High Energy Physics - PhenomenologyNatural Dark Mattertext