期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 325, 期 4, 页码 1312-1316出版社
OXFORD UNIV PRESS
DOI: 10.1046/j.1365-8711.2001.04281.x
关键词
methods : numerical; large-scale structure of Universe
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.
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