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Performance of the optimized Post-Zel'dovich approximation for CDM models in arbitrary FLRW cosmologies

Takashi Hamana

astro-pharXiv:astro-ph/9808346

Abstract

We investigate the performance of the optimized Post-Zel'dovich approximation in three cold dark matter cosmologies. We consider two flat models with Ω0=1 (SCDM) and with Ω0=0.3 (ΛCDM) and an open model with Ω0=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 ΛCDM 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)/D2(a), is insensitive to the background cosmologies.

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