Abstract
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.
Original language | English (US) |
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Pages (from-to) | 1312-1316 |
Number of pages | 5 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 325 |
Issue number | 4 |
DOIs | |
State | Published - Aug 21 2001 |
Keywords
- Large-scale structure of Universe
- Methods: numerical
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science