Geometrical measures of non-Gaussianity generated from single field
  Inflationary models
  We have calculated the third order moments of scalar curvature perturbations
in configuration space for different inflationary models. We developed a robust
numerical technique to compute the bispectrum for different models that have
some features in the inflationary potential. From the bispectrum we evaluated
moments analytically in the slow roll regime while we devised a numerical
mechanism to calculated these moments for non slow roll single field
inflationary models with standard kinetic term that are minimally coupled to
gravity. With help of these third order moments one can directly predict many
non-Gaussian and geometrical measures of CBM distributions in the configuration
space. Thus, we have devised a framework to calculate different third order
moments and geometrical measures, e.g. Minkowski functionals or skeleton
statistic, generated by different single field models of inflation.
