  One common approach for cosmic inflation consists in couple Einstein's
gravity with a scalar field, often referred to inflaton field. In order to
derive analytic simple scenarios, we usually work in the {\it slow-roll}
regime. In such an approximation one considers the scalar field potentials to
be nearly flat. It is possible to directly generalize such an approach for
hybrid inflationary models, where the inflaton sector is composed of two or
more scalar fields. However, the Friedmann equations and the equations of
motion for such hybrid models are often hard to be analytically solved. Another
recent path to describe cosmic inflation is through the so-called {\it
fast-roll} regime, where one considers exactly flat potentials. Our purpose in
this work is to obtain solutions for a hybrid inflaton model in the fast-roll
regime. Cosmological interpretations through the behavior of Hubble, slow-roll,
and equation of state parameters are also presented.
