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Large-Scale Structure of the Universe and Cosmological ...

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Fig. 28. Non-linear evolution <strong>of</strong> <strong>the</strong> variance (left panels) <strong>and</strong> <strong>of</strong> <strong>the</strong> skewness parameter<br />

S3 (right panels) from 10 realizations <strong>of</strong> flat CDM N-body simulations. Two<br />

models are considered, ΛCDM with Ωm + ΩΛ = 1 <strong>and</strong> Γ = 0.2, <strong>and</strong> SCDM with<br />

Ωm = 1 <strong>and</strong> Γ = 0.5, where Γ is <strong>the</strong> shape parameter <strong>of</strong> <strong>the</strong> power-spectrum [201].<br />

In <strong>the</strong> left panels, symbols show <strong>the</strong> ratio <strong>of</strong> <strong>the</strong> non-linear to <strong>the</strong> linear variance as<br />

a function <strong>of</strong> smoothing radius. The value <strong>of</strong> Γ is indicated on <strong>the</strong> panels, while σ 2 8<br />

st<strong>and</strong>s for <strong>the</strong> linear variance in a sphere <strong>of</strong> radius 8h −1 Mpc. The SC model predictions<br />

are shown as a short-dashed line while one-loop PT predictions are shown<br />

as a solid line. The arrows indicate where σl = 0.5. In <strong>the</strong> right panels, <strong>the</strong> output<br />

times correspond to σ8 = 0.5 (top) <strong>and</strong> σ8 = 0.7 (bottom). Squares <strong>and</strong> triangles<br />

correspond to measurements in Γ = 0.2 <strong>and</strong> Γ = 0.5 simulations, respectively. Each<br />

case is compared to <strong>the</strong> corresponding PT tree-level predictions (solid lines) <strong>and</strong> SC<br />

model (long-dashed). From [222].<br />

a number <strong>of</strong> studies considered <strong>the</strong> evolution <strong>of</strong> higher-order moments from<br />

non-Gaussian initial conditions given by cosmic strings [146,9] <strong>and</strong> texture<br />

models [252] using numerical simulations. Recently, measurements <strong>of</strong> higher-<br />

order moments in numerical simulations with χ 2 N<br />

initial conditions with N<br />

degrees <strong>of</strong> freedom were given in [689].<br />

General properties <strong>of</strong> one-point moments evolved from non-Gaussian initial<br />

conditions were considered using PT in [238,333,124,255,195]. To illustrate <strong>the</strong><br />

main ideas, let us write <strong>the</strong> PT expression for <strong>the</strong> first one-point moments:<br />

〈δ 2 〉 = 〈δ 2 1<br />

〉 +2<br />

〈δ1δ2 〉 <br />

+ 〈δ 2 2 〉 +2 〈δ1δ3 〉 +O(σ 5 ), (289)<br />

〈δ 3 〉 = <br />

〈δ 3 1 〉 <br />

+ 3 〈δ 2 1δ2 〉 + <br />

3 〈δ 2 2δ1 〉 +3 〈δ 2 1δ3 〉 <br />

+ O(σ 6 ), (290)<br />

〈δ 4 〉 = 〈δ 4 1<br />

〉 +4<br />

〈δ 3 1δ2 〉 <br />

+ 6 〈δ 2 1δ2 2 〉 +4 〈δ3 1δ3 〉 +O(σ 7 ), (291)<br />

where we simply use <strong>the</strong> PT expansion δ = δ1+δ2+. . .. Square brackets denote<br />

terms which scale as odd-powers <strong>of</strong> δ1, <strong>and</strong> thus vanish for Gaussian initial<br />

conditions. A first general remark one can make is that <strong>the</strong>se additional terms<br />

102

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