We use large volume, high resolution, N-body simulations of three different
Lambda CDM models, with different clustering strengths, to generate dark-m
atter halo merging histories. Over the reliable range of halo masses, rough
ly galaxy groups to rich clusters of galaxies, we quantify the number densi
ty of major mergers for two different time intervals and compare them with
analytic predictions based on the extended Press-Schechter theory.