Please use this identifier to cite or link to this item: http://hdl.handle.net/10261/33081
Share/Impact:
Título : N-body simulations with generic non-Gaussian initial conditions I: power spectrum and halo mass function
Autor : Wagner, Christian, Verde, Licia, Boubekeur, Lotfi
Fecha de publicación : Oct-2010
Editor: Institute of Physics Publishing
Citación : Journal of Cosmology and Astroparticle Physics (JCAP) 10: 022 (2010)
Resumen: We address the issue of setting up generic non-Gaussian initial conditions for N-body simulations. We consider inflationary-motivated primordial non-Gaussianity where the perturbations in the Bardeen potential are given by a dominant Gaussian part plus a non-Gaussian part specified by its bispectrum. The approach we explore here is suitable for any bispectrum, i.e. it does not have to be of the so-called separable or factorizable form. The procedure of generating a non-Gaussian field with a given bispectrum (and a given power spectrum for the Gaussian component) is not univocal, and care must be taken so that higher-order corrections do not leave a too large signature on the power spectrum. This is so far a limiting factor of our approach. We then run N-body simulations for the most popular inflationary-motivated non-Gaussian shapes. The halo mass function and the non-linear power spectrum agree with theoretical analytical approximations proposed in the literature, even if they were so far developed and tested only for a particular shape (the local one).
Versión del editor: http://dx.doi.org/10.1088/1475-7516/2010/10/022
URI : http://hdl.handle.net/10261/33081
ISSN: 1475-7516
DOI: 10.1088/1475-7516/2010/10/022
Appears in Collections:(IFIC) Artículos

Files in This Item:
File Description SizeFormat 
n-body.pdf610,81 kBAdobe PDFView/Open
Show full item record
 
CSIC SFX LinksSFX Query


Items in Digital.CSIC are protected by copyright, with all rights reserved, unless otherwise indicated.