The results of a set of simulations of Alfvén modes driven by an energetic particle population are presented, with the specific aim of comparing single-n and multiple-n simulations (n being the toroidal mode number). The hybrid reduced O(3 0) MHD gyrokinetic code HMGC is used (0 ≡ a/R 0 being the inverse aspect ratio of the torus, with a and R 0 the minor and major radius, respectively), retaining both fluid (wave-wave) and energetic particles nonlinearities. The code HMGC retains selfconsistently, in the time evolution, the wave spatial structures as modified by the energetic particle (EP) term. Simulations with toroidal mode numbers 1 n 15 have been considered. For the specific energetic particle drive considered, single-n simulations are either stable (n=1), or weakly unstable (n = 2, 3, 13, 14, 15), or strongly unstable (4 n 12), with 4 n 12 modes exhibiting similar growth-rates, while n = 4 the largest saturated amplitude. A variety of modes are observed (TAEs, upper and lower KTAEs, EPMs). Nevertheless, no appreciable global modification of the EP density profile is observed at saturation. On the contrary, multi-n, fully nonlinear simulation exhibits an appreciable broadening of the EP radial density profile at saturation, thus showing an enhanced radial transport w.r.t. the single-n simulations. Moreover, the subdominant modes are strongly modified by the nonlinear coupling which results both from the MHD and from the Energetic Particle terms.