  In this work, we present results of numerical simulations of the Chern-Simons
Inflation Model proposed by Alexander, Marciano and Spergel. According to this
model, inflation begins with a fermion condensate interacting with a gauge
field. Crucial to the success of this mechanism is the assumption that the
Chern-Simons interaction would drive energy from the initial random spectrum
into a narrow band of frequencies at superhorizon scales. In this work we
numerically confirm this expectation. These gauge fields and currents, when
combined with the Friedmann equations, were broken into a system of hyperbolic
equations and numerically simulated. It was found in our simulation that, by
including the effects of the chiral anomaly for the axial vector current,
inflation ended satisfactorily after approximately 60 e-folds.
