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Permanent URL to this publication: http://dx.doi.org/10.5167/uzh-16769

Heitmann, K; Lukić, Z; Fasel, P; Habib, S; Warren, M S; White, M; Ahrens, J; Ankeny, L; Armstrong, R; O’Shea, B; Ricker, P M; Springel, V; Stadel , J; Trac , H (2008). The cosmic code comparison project. Computational Science & Discovery, 1(1):015003.

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Abstract

Current and upcoming cosmological observations allow us to probe structures on smaller and smaller scales, entering highly nonlinear regimes. In order to obtain theoretical predictions in these regimes, large cosmological simulations have to be carried out. The promised high accuracy from observations makes the simulation task very demanding: the simulations have to be at least as accurate as the observations. This requirement can only be fulfilled by carrying out an extensive code verification program. The first step of such a program is the comparison of different cosmology codes including gravitational interactions only. In this paper, we extend a recently carried out code comparison project to include five more simulation codes. We restrict our analysis to a small cosmological volume which allows us to investigate properties of halos. For the matter power spectrum and the mass function, the previous results hold, with the codes agreeing at the 10% level over wide dynamic ranges. We extend our analysis to the comparison of halo profiles and investigate the halo count as a function of local density. We introduce and discuss ParaView as a flexible analysis tool for cosmological simulations, the use of which immensely simplifies the code comparison task.

Item Type:Journal Article, not refereed, original work
Communities & Collections:07 Faculty of Science > Institute for Computational Science
DDC:530 Physics
Language:English
Date:October 2008
Deposited On:06 Mar 2009 10:57
Last Modified:29 Jun 2014 23:22
Publisher:Institute of Physics Publishing
ISSN:1749-4699
Publisher DOI:10.1088/1749-4699/1/1/015003
Related URLs:http://arxiv.org/abs/0706.1270
Citations:Google Scholar™
Scopus®. Citation Count: 29

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