Realising Mutated Hilltop Inflation in Supergravity
  We present $\mathcal{N}=1$ supergravity models of mutated hilltop inflation
(MHI) for both large and small field sectors. Models with canonical kinetic
terms are developed based on a shift symmetric K\"ahler potential in inflaton
superfield, and with a superpotential linear in Goldstino superfield. We also
construct models with non-canonical kinetic terms for MHI by generalizing the
shift symmetry. We found that a good fraction of the models can address the
entire branch of MHI in a single framework.
