  Stochastic gravity waves have been recently detected and characterised in
stars thanks to space asteroseismology and they may play an important role in
the evolution of stellar angular momentum. In this context, the observational
study of the CoRoT hot Be star HD 51452 suggests a potentially strong impact of
rotation on stochastic excitation of gravito-inertial waves in rapidly rotating
stars. In this work, we present our results on the action of the Coriolis
acceleration on stochastic wave excitation by turbulent convection. We study
the change of efficiency of this mechanism as a function of the waves' Rossby
number and we demonstrate that the excitation presents two different regimes
for super-inertial and sub-inertial frequencies. Consequences for rapidly
rotating early-type stars and the transport of angular momentum in their
interiors are discussed.
