A fitting formula for the non-linear evolution of the bispectrum

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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.

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Scoccimarro, R., & Couchman, H. M. P. (2001). A fitting formula for the non-linear evolution of the bispectrum. Monthly Notices of the Royal Astronomical Society, 325(4), 1312–1316. https://doi.org/10.1046/j.1365-8711.2001.04281.x

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