Loop corrections in nonlinear cosmological perturbation theory. II. two-point statistics and self-similarity

Román Scoccimarro, Joshua A. Frieman

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    Abstract

    We calculate the lowest order nonlinear contributions to the power spectrum, two-point correlation function, and smoothed variance of the density field for Gaussian initial conditions and scale-free initial power spectra, P(k) ∼ kn. These results extend and, in some cases, correct previous work in the literature on cosmological perturbation theory. Comparing with the scaling behavior observed in N-body simulations, we find that the validity of nonlinear perturbation theory depends strongly on the spectral index n. For n< -1, we find excellent agreement over scales where the variance σ2(R) ≲ 10; however, for n ≥ -1, perturbation theory predicts deviations from self-similar scaling (which increase with n) not seen in numerical simulations. This anomalous scaling suggests that the principal assumption underlying cosmological perturbation theory, namely, that large-scale fields can be described perturbatively even when fluctuations are highly nonlinear on small scales, breaks down beyond leading order for spectral indices n≥ -1. For n < -1, the power spectrum, variance, and correlation function in the scaling regime can be calculated using dimensional regularization.

    Original languageEnglish (US)
    Pages (from-to)620-644
    Number of pages25
    JournalAstrophysical Journal
    Volume473
    Issue number2 PART I
    DOIs
    StatePublished - Jan 1 1996

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    Keywords

    • Galaxies: clusters: general
    • Large-scale structure of universe
    • Methods: Numerical

    ASJC Scopus subject areas

    • Astronomy and Astrophysics
    • Space and Planetary Science

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