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| Journal Article | PUBDB-2020-01567 |
; ;
2020
IOP
London
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Please use a persistent id in citations: doi:10.1088/1475-7516/2020/04/003 doi:10.3204/PUBDB-2020-01567
Report No.: DESY-19-176; arXiv:1911.04505
Abstract: We study the Schrödinger-Poisson (SP) method in the context of cosmological large-scale structure formation in an expanding background. In the limit 0ℏ &to; , the SP technique can be viewed as an effective method to sample the phase space distribution of cold dark matter that remains valid on non-linear scales. We present results for the 2D and 3D matter correlation function and power spectrum at length scales corresponding to the baryon acoustic oscillation (BAO) peak. We discuss systematic effects of the SP method applied to cold dark matter and explore how they depend on the simulation parameters. In particular, we identify a combination of simulation parameters that controls the scale-independent loss of power observed at low redshifts, and discuss the scale relevant to this effect.
Keyword(s): matter: correlation function ; oscillation: acoustic ; redshift: low ; dark matter ; structure ; power spectrum ; phase space ; background ; nonlinear ; formation ; baryon
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The Schrödinger-Poisson method for Large-Scale Structure
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