  Granular matter under rapid flow conditions can be modeled as a granular gas,
namely, a gas of hard spheres dissipating part of their kinetic energy during
binary collisions (inelastic hard spheres, IHS). On the other hand, given that
collisions are inelastic one has to inject energy into the system to compensate
for the inelastic cooling and maintain it in rapid conditions. Although in real
experiments the external energy is supplied to the system by the boundaries, it
is quite usual in computer simulations to heat the system by the action of an
external driving force or thermostat. Despite thermostats have been widely
employed in the past, their influence on the dynamic properties of the system
(for elastic and granular fluids) is not yet completely understood. In this
work, we determine the transport properties of driven granular systems by using
two independent and complementary routes, one of them being analytic
(Chapman-Enskog method, BGK solution and Grad's moments method) and the other
one being computational (Monte Carlo simulations).
