We present a fitting formula for the non-linear evolution of the bispectrum in cold dark matter (CDM) models, obtained from measurements in high-resolution numerical simulations. The formula interpolates between the perturbative and highly non-linear regimes, and generalizes previous results obtained for scale-free initial conditions.
No takes yet. Share an insight, caveat, or question.
A 2001 study studied this question.
Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context: