  The discovery of the primordial B-mode polarisation by the BICEP2 experiment
indicates inflation with a relatively high energy scale. Taking this indication
into account, we propose consistent scenarios to account for the observed
baryon and dark matter densities in gravity and gauge mediated supersymmetry
breaking models. The baryon asymmetry is explained by the Afflck-Dine
mechanism, which requires relatively low reheating temperature to avoid a
sizable baryonic isocurvature perturbation. The low reheating temperature then
requires non-thermal production of dark matter to account for the correct relic
density of dark matter. Our scenarios can account for the observations of
baryon and dark matter density in gravity and gauge mediation and predict some
parameters, including the mass of dark matter.
