  In Split-SUSY with BRpV we show that the Gravitino DM solution is consistent
with experimental evidence on its relic density and life time. We arrive at
this conclusion by performing a complete numerical and algebraic study of the
parameter space, including constraints from the recently determined Higgs mass,
updated neutrino physics, and BBN constraints on NLSP decays. The Higgs mass
requires a relatively low Split-SUSY mass scale, which is naturally smaller
than usual values for reheating temperature, allowing the use of the standard
expression for the relic density. We include restrictions from neutrino physics
with three generations, and notice that the gravitino decay width depends on
the atmospheric neutrino mass scale. We calculate the neutralino decay rate and
find it consistent with BBN. We mention some implications on indirect DM
searches.
