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2007

Renormalized Newtonian Cosmic Evolution with Primordial Non-Gaussianity

Izumi, Keisuke, Soda, Jiro

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We study Newtonian cosmological perturbation theory from a field theoretical point of view.

We derive a path integral representation for the cosmological evolution of stochastic fluctuations.
Our main result is the closed form of the generating functional valid for any initial statistics.
Moreover, we extend the renormalization group method proposed by Mataresse and Pietroni to the case of primordial non-Gaussian density and velocity fluctuations.

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T. Matsubara, arXiv:astro-ph/0006269

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