Higgsino-like Dark Matter From Sneutrino Late Decays
  We consider Higgsino-like dark matter (DM) in the Minimal Supersymmetric
Standard Model (MSSM) with additional right-handed neutrino chiral superfields,
and propose a new non-thermal way of generating the right amount of relic DM
via sneutrino late decays. Due to the large DM annihilation cross-section,
decays must occur at lower temperatures than the freeze-out temperature $T_d\ll
T_{F,\tilde{\chi}^0_1}\sim \mu/25$, implying a mostly right-handed lightest
sneutrino with very small Yukawa interactions. In that context, the right
amount of Higgsino-like DM relic density can be accounted for if sneutrinos are
produced via thermal freeze-in in the early Universe.
