Minimal Supersymmetric Standard Model with gauge mediated supersymmetry breaking has all the necessary ingredients for a successful sub-eV Hubble scale inflation H _ { inf } \sim 10 ^ { -3 } -10 ^ { -1 } eV .
The model generates the right amplitude for scalar density perturbations and a spectral tilt within the range , 0.90 \leq n _ { s } \leq 1 .
The reheat temperature is T _ { R } \mathrel { \lower 4.0 pt \vbox { \hbox { $ < $ } \hbox { $ \sim$ } } } 10 TeV , which strongly prefers electroweak baryogenesis and creates the right abundance of gravitinos with a mass m _ { 3 / 2 } \mathrel { \lower 4.0 pt \vbox { \hbox { $ > $ } \hbox { $ \sim$ } } } 100 keV to be the dark matter .