Loop corrections in nonlinear cosmological perturbation theory
- Department of Physics and Enrico Fermi Institute, University of Chicago, Chicago, Illinois 60637 (United States)
- NASA/Fermilab Astrophysics Center, Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, Illinois 60510 (United States)
Using a diagrammatic approach to Eulerian perturbation theory, we calculate analytically the variance and skewness of the density and velocity divergence induced by gravitational evolution from Gaussian initial conditions, including corrections {ital beyond} leading order. Except for the power spectrum, previous calculations in cosmological perturbation theory have been confined to leading order (tree level): we extend these to include loop corrections. For scale-free initial power spectra, {ital P}({ital k}){approximately}{ital k}{sup {ital n}} with {minus}2{le}{ital n}{le}2, the one-loop variance {sigma}{sup 2}{equivalent_to}{l_angle}{delta}{sup 2}{r_angle}={sigma}{sup 2}{sub {ital l}}+1.82{sigma}{sup 4}{sub {ital l}}, and the skewness {ital S}{sub 3}={l_angle}{delta}{sup 3}{r_angle}/{sigma}{sup 4}=34/7+9.8{sigma}{sup 2}{sub {ital l}}, where {sigma}{sub {ital l}} is the rms fluctuation of the density field to linear order. (These results depend weakly on the spectral index {ital n}, due to the nonlocality of the nonlinear solutions to the equations of motion.) Thus, loop corrections for the (unsmoothed) density field begin to dominate over tree-level contributions (and perturbation theory presumably begins to break down) when {sigma}{sup 2}{sub {ital l}}{approx_equal}1/2. For the divergence of the velocity field, loop dominance does not occur until {sigma}{sup 2}{sub {ital l}}{approx_equal}1. We also compute loop corrections to the variance, skewness, and kurtosis for several nonlinear approximation schemes, where the calculation can be easily generalized to one-point cumulants of higher order and arbitrary number of loops. We find that the Zeldovich approximation gives the best approximation to the loop corrections of exact perturbation theory, followed by the linear potential approximation (LPA) and the frozen flow approximation (FFA), in qualitative agreement with the relative behavior of tree-level results. (Abstract Truncated)
- OSTI ID:
- 383080
- Journal Information:
- Astrophysical Journal, Supplement Series, Vol. 105, Issue 1; Other Information: PBD: Jul 1996
- Country of Publication:
- United States
- Language:
- English
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