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 $\delta$ and momentum density $\mathbf\pi(\mathbf k)$ scale as $k^2$ and $k$, respectively. Third, we demonstrate that the common practice of introducing counterterms only in the Euler equation when one is interested in correlators of $ \delta$ is indeed valid to all orders.
| Original language | Undefined/Unknown |
|---|---|
| Pages (from-to) | 1-43 |
| Journal | Journal of Cosmology and Astroparticle Physics |
| DOIs | |
| Publication status | Published - 31 May 2016 |
Bibliographical note
28+14Keywords
- hep-th
- astro-ph.CO
Cite this
- APA
- Author
- BIBTEX
- Harvard
- Standard
- RIS
- Vancouver