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We have performed high‐resolution cosmological  N ‐body simulations of a  concordance ΛCDM model to study the evolution of virialized, dark matter haloes in the presence of primordial non‐Gaussianity. Following a standard procedure, departures from Gaussianity are modelled through a quadratic Gaussian term in the primordial gravitational potential, characterized by a dimensionless non‐linearity strength parameter  f  NL . We find that the halo mass function and its redshift evolution closely follow the analytic predictions of Matarrese, Verde &amp; Jimenez. The existence of precise analytic predictions makes the observation of rare, massive objects at large redshift an even more attractive test to detect primordial non‐Gaussian features in the large‐scale structure of the Universe.

Evolution of massive haloes in non‐Gaussian scenarios