Nonlinear approximations to gravitational instability: A comparison in second-order perturbation theory

Abstract

view Abstract Citations (28) References (10) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Nonlinear Approximations to Gravitational Instability: A Comparison in Second-Order Perturbation Theory Munshi, Dipak ; Starobinsky, Alexei A. Abstract Nonlinear approximation methods such as the Zeldovich approximation, and more recently the frozen flow and linear potential approximations, are sometimes used to simulate nonlinear gravitational instability in the expanding Universe. We investigate the relative accuracy of these approximations by comparing them with the exact solution using second order perturbation theory. We evaluate the density and velocity fields in these approximations to second order, and also determine the skewness parameter $S_3 = \langle \delta^3 \rangle / \langle (\delta^{(1)})^2\rangle ^2$ for each of the approximations again in second order. We find that $S_3 = 4, ~3, ~3.4$ for the Zeldovich approximation, the frozen flow and the linear potential approximations respectively as compared to $S_3 = {34/7}$ for the exact solution. Our results show that, of all the approximations considered, the Zeldovich approximation is the most accurate in describing the weakly nonlinear effects of gravity. Moreover, the Zeldovich approximation is much closer to the exact results for matter and velocity distributions than the other approximations if the slope of the power spectrum of density perturbations is $-3< n \le -1$. Publication: The Astrophysical Journal Pub Date: June 1994 DOI: 10.1086/174255 arXiv: arXiv:astro-ph/9311056 Bibcode: 1994ApJ...428..433M Keywords: Approximation; Computational Astrophysics; Dynamic Stability; Galactic Structure; Gravitational Fields; Nonlinear Equations; Accuracy; Density Distribution; Perturbation Theory; Velocity Distribution; Astronomy; GRAVITATION; INSTABILITIES; COSMOLOGY: LARGE-SCALE STRUCTURE OF UNIVERSE; Astrophysics E-Print: Latex file, pages 20 , Two figures (available at 144.16.31.6 through anonymous ftp), IUCAA 31/93 full text sources arXiv | ADS |