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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Result for Padé resummed small-k limit1.15Correction to Pk,z rel. to oneloopPk,zP 1loop k,z1.101.051 loop2 loop3 loopK 01padeK 02padeK 11pade1.000 2 4 6 8 10redshift zblack=SPT, solid=Padé resummed resultMathias 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