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In models for thermal baryogenesis from particle decays, the mass of thedecaying particle is typically many orders of magnitude above the TeV scale. Wewill discuss different ways to lower the energy scale of baryogenesis andpresent the corresponding lower bounds on the particle's mass. This is donespecifically for the inert doublet model with heavy Majorana neutrinos and thenwe indicate how to extrapolate the results to other scenarios. We also revisitthe question of whether or not dark matter, neutrino masses, and the cosmicbaryon asymmetry can be explained simultaneously at low energies in the inertdoublet model.

Mass bounds for baryogenesis from particle decays and the inert doublet model