Modeling Nonlinear Evolution of Baryon Acoustic Oscillations: Convergence Regime of IV-Body Simulations and Analytic Models
We used a series of cosmological N-body simulations and various analytic models to study the evolution of the matter power spectrum in real space in a A cold dark matter universe. We compared the results of A 7-body simulations against three analytical model predictions; standard perturbation theory, renormalized perturbation theory, and a closure approximation. We included the effects from a finite simulation box size under comparison. We determined the values of the maximum wavenumbers, klim1% and klim3%, below which the analytic models and the simulation results agree with accuracy to within 1 and 3 percent. We then provided a simple empirical function that describes the convergence regime determined by comparisons between our simulations and the analytical models. We found that if we use the Fourier modes within the convergence regime alone, the characteristic scale of baryon acoustic oscillations can be determined with an accuracy of 1% from future surveys with a volume of a few h-3Gpc3 at z ~ 1 or z ~ 3 in the absence of any systematic distortion of the power spectrum.
T. Nishimichi et al., "Modeling Nonlinear Evolution of Baryon Acoustic Oscillations: Convergence Regime of IV-Body Simulations and Analytic Models," Publications of the Astronomical Society of Japan, vol. 61, no. 2, pp. 321-332, Astronomical Society of Japan, Apr 2009.
Keywords and Phrases
Cosmology: large-scale structure of universe; Methods: statistical
International Standard Serial Number (ISSN)
Article - Journal
© 2009 Astronomical Society of Japan, All rights reserved.
01 Apr 2009