Induced-Gravity Inflation in no-Scale Supergravity and Beyond
  Supersymmetric versions of induced-gravity inflation are formulated within
Supergravity (SUGRA) employing two gauge singlet chiral superfields. The
proposed superpotential is uniquely determined by applying a continuous R and a
discrete Z_n symmetry. We select two types of logarithmic Kahler potentials,
one associated with a no-scale-type SU(2,1) / SU(2) x U(1)_R x Z_n Kahler
manifold and one more generic. In both cases, imposing a lower bound on the
parameter cR involved in the coupling between the inflaton and the Ricci scalar
curvature - e.g. cR > 76, 105, 310 for n=2,3 and 6 respectively -, inflation
can be attained even for subplanckian values of the inflaton while the
corresponding effective theory respects the perturbative unitarity. In the case
of no-scale SUGRA we show that, for every n, the inflationary observables
remain unchanged and in agreement with the current data while the inflaton mass
is predicted to be 3x10^13 GeV. Beyond no-scale SUGRA the inflationary
observables depend mildly on n and crucially on the coefficient involved in the
fourth order term of the Kahler potential which mixes the inflaton with the
accompanying non-inflaton field.
