Dynamical Generation of the Weak Scale and Inflation in High-Scale
  Supersymmetry
  Combination of Plank and BICEP2 data reported that tensor to scalar ratio
$r\simeq 0.16$ and scalar spectral index $n_{s}\simeq 0.96$. In this short
note, it is shown that chaotic inflation with quadratic potential, which
perfectly accounts for present fit to $r$ and $n_s$, and relatively heavy Higgs
mass for fine-tuned MSSM, are both suggested to be consequences of high-scale
supersymmetry (SUSY) breaking. Following this idea, we find that inflaton mass
is of same order as soft mass, flatness of inflation potential doesn't need a
shift symmetry, and scale of inflation energy density automatically agrees with
SUSY-breaking scale. A simple realization of such high-scale SUSY breaking, in
which inflaton with tri-linear superpotential serves as {\it modulus}, is
discussed in terms of ISS-like model.
