Starobinsky-like inflation in no-scale supergravity Wess-Zumino model
  with Polonyi term
  We propose a simple modification of the no-scale supergravity Wess-Zumino
model of Starobinsky-like inflation to include a Polonyi term in the
superpotential. The purpose of this term is to provide an explicit mechanism
for supersymmetry breaking at the end of inflation. We show how successful
inflation can be achieved for a gravitino mass satisfying the strict upper
bound $m_{3/2}< 10^3$ TeV, with favoured values $m_{3/2}\lesssim\mathcal{O}(1)$
TeV. The model suggests that SUSY may be discovered in collider physics
experiments such as the LHC or the FCC.
