arXiv · astro-ph/9808346
Performance of the optimized Post-Zel'dovich approximation for CDM models in arbitrary FLRW cosmologies
Abstract
We investigate the performance of the optimized Post-Zel'dovich approximation in three cold dark matter cosmologies. We consider two flat models with $Ω_0=1$ (SCDM) and with $Ω_0=0.3$ ($Λ$CDM) and an open model with $Ω_0=0.3$ (OCDM). We find that the optimization scheme proposed by Weiß, Gottlöber & Buchert (1996), in which the performance of the Lagrangian perturbation theory was optimized only for the Einstein-de Sitter cosmology, shows the excellent performances not only for SCDM model but also for both OCDM and $Λ$CDM models. This universality of the excellent performance of the optimized Post-Zel'dovich approximation is explained by the fact that a relation between the Post-Zel'dovich order's growth factor $E(a)$ and Zel'dovich order's one $D(a)$, $E(a)/D^2(a)$, is insensitive to the background cosmologies.
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Takashi Hamana. 1998-08-31. Performance of the optimized Post-Zel'dovich approximation for CDM models in arbitrary FLRW cosmologies. https://doi.org/10.1086/311683
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