Particle physics and cosmology with high-scale SUSY breaking in
  five-dimensional supergravity models
  We discuss a high-scale SUSY breaking scenario with the wino dark matter in
the five-dimensional supergravity model on $S^1/Z_2$. The extra U(1) symmetries
broken by the orbifold projection control the flavor structure of soft
SUSY-breaking parameters as well as the Yukawa couplings, and a scalar
component of the one of moduli multiplets, which arise from extra-dimensional
components of the U(1) vector multiplets, induces the slow-roll inflation.
Because of the supersymmetric moduli stabilization as well as the moduli
inflation, it is found that the correct dark matter relic abundance is
non-thermally generated by the gravitino decaying into the wino.
