English

Systematic Renormalization of the Effective Theory of Large Scale Structure

High Energy Physics - Theory 2016-06-08 v1 Cosmology and Nongalactic Astrophysics

Abstract

A perturbative description of Large Scale Structure is a cornerstone of our understanding of the observed distribution of matter in the universe. Renormalization is an essential and defining step to make this description physical and predictive. Here we introduce a systematic renormalization procedure, which neatly associates counterterms to the UV-sensitive diagrams order by order, as it is commonly done in quantum field theory. As a concrete example, we renormalize the one-loop power spectrum and bispectrum of both density and velocity. In addition, we present a series of results that are valid to all orders in perturbation theory. First, we show that while systematic renormalization requires temporally non-local counterterms, in practice one can use an equivalent basis made of local operators. We give an explicit prescription to generate all counterterms allowed by the symmetries. Second, we present a formal proof of the well-known general argument that the contribution of short distance perturbations to large scale density contrast δ\delta and momentum density π(k)\mathbf\pi(\mathbf k) scale as k2k^2 and kk, respectively. Third, we demonstrate that the common practice of introducing counterterms only in the Euler equation when one is interested in correlators of δ \delta is indeed valid to all orders.

Keywords

Cite

@article{arxiv.1509.07886,
  title  = {Systematic Renormalization of the Effective Theory of Large Scale Structure},
  author = {Ali Akbar Abolhasani and Mehrdad Mirbabayi and Enrico Pajer},
  journal= {arXiv preprint arXiv:1509.07886},
  year   = {2016}
}

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