Universal Non-Gaussian Initial Conditions for N-body Simulations
Cosmology and Nongalactic Astrophysics
2013-05-30 v1
Abstract
In this paper we present the implementation of an efficient formalism for the generation of arbitrary non-Gaussian initial conditions for use in N-body simulations. The methodology involves the use of a separable modal approach for decomposing a primordial bispectrum or trispectrum. This approach allows for the far more efficient generation of the non-Gaussian initial conditions already described in the literature, as well as the generation for the first time of non-separable bispectra and the special class of diagonal-free trispectra. The modal approach also allows for the reconstruction of the spectra from given realisations, a fact which is exploited to provide an accurate consistency check of the simulations.
Cite
@article{arxiv.1108.3813,
title = {Universal Non-Gaussian Initial Conditions for N-body Simulations},
author = {D. M. Regan and M. M. Schmittfull and E. P. S. Shellard and J. R. Fergusson},
journal= {arXiv preprint arXiv:1108.3813},
year = {2013}
}
Comments
7 pages, 3 figures