  This article presents a possible inflation scenario as a consequence of
non-minimal gravitational couplings in the Conformal Standard Model. The model
consists, in comparison to the SM, of additional right-chiral neutrinos and
complex scalars coupled to the right-chiral neutrinos but not to the SM
particles. The inflation is driven by two non-minimally coupled fields one
being the usual Higgs and the other one of the sterile scalars. It turns out
that in this model the tensor to scalar ratio and spectral index can match the
current data for a wide range of parameters.
