On Second-order Perturbation Theories of Gravitational Instability in Friedmann-Lemaitre Models

Abstract

The Eulerian and Lagrangian second-order perturbation theories are solved explicitly in closed forms in $\Omega \ne 1$ and $\Lambda \ne 0$ {}Friedmann-Lema\^ıtre models. I explicitly write the second-order theories in terms of closed one-dimensional integrals. In cosmologically interested cases ($\Lambda =0$ or $\Omega +\lambda =1$), they reduce to elementary functions or hypergeometric functions. For arbitrary $\Omega$ and $\Lambda$, I present accurate fitting formula which are sufficient in practice for the observational cosmology. It is reconfirmed for generic $\Omega$ and $\Lambda$ of interest that second-order effect only weakly depends on these parameters.

9 pages, LaTeX, to appear in Progress of Theoretical Physics (Letters)

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