  Minimal Supersymmetric Standard Model with gauge mediated supersymmetry
breaking has all the necessary ingredients for a successful sub-eV Hubble scale
inflation $H_{\rm inf} \sim 10^{-3}-10^{-1}$ 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 $T_{\rm R} \ls 10$
TeV, which strongly prefers electroweak baryogenesis and creates the right
abundance of gravitinos with a mass $m_{3/2} \gs 100$ keV to be the dark
matter.
