Non-Gaussianities in the Extended EFT of Inflation
  In earlier works, we studied the validity of Extended Effective Field Theory
of Inflation (EEFToI) in the regime where initial conditions are set with
dispersion relations $\omega^2 \propto k^6$. We had also evaluated and examined
the power spectrum for some interesting corners of the parameter space. In this
paper, we compute the bispectrum in the EEFToI, take a closer look at the
strong coupling constraints and calculate the size of the non-Gaussianities in
those regions of parameter space. We also investigate the shape of triangles
that contribute to the enhancement of non-Gaussianities in this regime. We find
that there are allowed parts of parameter spaces where EEFToI description with
initial conditions set with $\omega^2 \propto k^6$ is sensible and interesting.
