On the non-linear scale of cosmological perturbation theory
On the non-linear scale of cosmological perturbation theory
On the non-linear scale of cosmological perturbation theory
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Padé improved PT vs N-body1.4z⩵01.4z⩵0.375PkPnowigglek1.3 1.2 1.1 1.0 0.90.00 0.05 0.10 0.15 0.20 0.25 0.301.4khMpcz⩵0.833PkPnowigglek1.3 1.2 1.1 1.0 0.9 0.00 0.05 0.10 0.15 0.20 0.25 0.301.4khMpcz⩵1.75PkPnowigglek1.31.2 1.1 1.0 PkPnowigglek1.31.2 1.1 1.0 0.90.00 0.05 0.10 0.15 0.20 0.25 0.30khMpc0.90.00 0.05 0.10 0.15 0.20 0.25 0.30khMpcMathias Garny (DESY Hamburg / CERN)<strong>On</strong> <strong>the</strong> <strong>non</strong>-<strong>linear</strong> <strong>scale</strong> <strong>of</strong> <strong>cosmological</strong> <strong>perturbation</strong> <strong>the</strong>ory
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