  Inspired by the Generalized Proca Theory, we study a vector-tensor model of
inflation with massive vector fields and derivative self-interactions. The
action under consideration contains a usual Maxwell-like kinetic term, a
general potential term and a term with non-minimal derivative coupling between
the vector field and gravity, via the dual Riemann tensor. In this theory, the
last term contains a free parameter, $\lambda$, which quantifies the
non-minimal derivative coupling. In this scenario, taking into account a
spatially flat FRW universe and a general vector field, we obtain the general
expressions for the equation of motion and the total energy momentum tensor.
Choosing a Proca-type potential, a suitable inflationary regimen driven by
massive vector fields is studied. In this model, the isotropy of expansion is
guaranteed by considering a triplet of orthogonal vector fields. In order to
obtain an inflationary solution with this model, the quasi de Sitter expansion
was considered. In this case the vector field behaves as a constant. Finally,
slow roll analysis is performed and slow-roll conditions are defined for this
model, which, for suitable constraints of the model parameters, can give the
required number of e-folds for sufficient inflation.
