Non linear predictions from linear theories in models with Dark Energy

We study the cluster mass function and its evolution in different models with Dark Energy arising from a self–interacting scalar field, with Ratra-Peebles and SUGRA potentials. Computations are based on a Press & Schechter approximation. The mass functions we obtain are compared with results holding for open models or models with Dark Energy due to a cosmological constant. Evolution results, in the Dark Energy cases, closely approach open models.